<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.2 20190208//EN" "http://jats.nlm.nih.gov/publishing/1.2/JATS-journalpublishing1.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="1.2" xml:lang="en">
    <front>
        <journal-meta>
            <journal-id journal-id-type="pmc">F1000Research</journal-id>
            <journal-title-group>
                <journal-title>F1000Research</journal-title>
            </journal-title-group>
            <issn pub-type="epub">2046-1402</issn>
            <publisher>
                <publisher-name>F1000 Research Limited</publisher-name>
                <publisher-loc>London, UK</publisher-loc>
            </publisher>
        </journal-meta>
        <article-meta>
            <article-id pub-id-type="doi">10.12688/f1000research.133292.2</article-id>
            <article-categories>
                <subj-group subj-group-type="heading">
                    <subject>Research Article</subject>
                </subj-group>
                <subj-group>
                    <subject>Articles</subject>
                </subj-group>
            </article-categories>
            <title-group>
                <article-title>Development of a magneto-optical Kerr microscope using a 3D printer</article-title>
                <fn-group content-type="pub-status">
                    <fn>
                        <p>[version 2; peer review: 1 approved, 1 not approved]</p>
                    </fn>
                </fn-group>
            </title-group>
            <contrib-group>
                <contrib contrib-type="author" corresp="no">
                    <name>
                        <surname>Uebo</surname>
                        <given-names>Koki</given-names>
                    </name>
                    <role content-type="http://credit.niso.org/">Conceptualization</role>
                    <role content-type="http://credit.niso.org/">Investigation</role>
                    <role content-type="http://credit.niso.org/">Methodology</role>
                    <role content-type="http://credit.niso.org/">Writing &#x2013; Original Draft Preparation</role>
                    <xref ref-type="aff" rid="a1">1</xref>
                </contrib>
                <contrib contrib-type="author" corresp="no">
                    <name>
                        <surname>Shiokawa</surname>
                        <given-names>Yuto</given-names>
                    </name>
                    <role content-type="http://credit.niso.org/">Conceptualization</role>
                    <role content-type="http://credit.niso.org/">Investigation</role>
                    <role content-type="http://credit.niso.org/">Methodology</role>
                    <xref ref-type="aff" rid="a1">1</xref>
                </contrib>
                <contrib contrib-type="author" corresp="no">
                    <name>
                        <surname>Takahashi</surname>
                        <given-names>Ryunosuke</given-names>
                    </name>
                    <role content-type="http://credit.niso.org/">Conceptualization</role>
                    <role content-type="http://credit.niso.org/">Investigation</role>
                    <role content-type="http://credit.niso.org/">Methodology</role>
                    <xref ref-type="aff" rid="a1">1</xref>
                </contrib>
                <contrib contrib-type="author" corresp="no">
                    <name>
                        <surname>Nakata</surname>
                        <given-names>Suguru</given-names>
                    </name>
                    <role content-type="http://credit.niso.org/">Conceptualization</role>
                    <role content-type="http://credit.niso.org/">Investigation</role>
                    <role content-type="http://credit.niso.org/">Methodology</role>
                    <role content-type="http://credit.niso.org/">Writing &#x2013; Review &amp; Editing</role>
                    <xref ref-type="aff" rid="a1">1</xref>
                </contrib>
                <contrib contrib-type="author" corresp="yes">
                    <name>
                        <surname>Wadati</surname>
                        <given-names>Hiroki</given-names>
                    </name>
                    <role content-type="http://credit.niso.org/">Conceptualization</role>
                    <role content-type="http://credit.niso.org/">Investigation</role>
                    <role content-type="http://credit.niso.org/">Methodology</role>
                    <role content-type="http://credit.niso.org/">Writing &#x2013; Review &amp; Editing</role>
                    <uri content-type="orcid">https://orcid.org/0000-0001-5969-8624</uri>
                    <xref ref-type="corresp" rid="c1">a</xref>
                    <xref ref-type="aff" rid="a1">1</xref>
                    <xref ref-type="aff" rid="a2">2</xref>
                </contrib>
                <aff id="a1">
                    <label>1</label>Department of Material Science, Graduate School of Science, University of Hyogo, Ako, Hyogo, 678-1297, Japan</aff>
                <aff id="a2">
                    <label>2</label>Institute of Laser Engineering, Osaka Univerisity, Suita, Osaka, 565-0871, Japan</aff>
            </contrib-group>
            <author-notes>
                <corresp id="c1">
                    <label>a</label>
                    <email xlink:href="mailto:wadati@sci.u-hyogo.ac.jp">wadati@sci.u-hyogo.ac.jp</email>
                </corresp>
                <fn fn-type="conflict">
                    <p>No competing interests were disclosed.</p>
                </fn>
            </author-notes>
            <pub-date pub-type="epub">
                <day>5</day>
                <month>1</month>
                <year>2024</year>
            </pub-date>
            <pub-date pub-type="collection">
                <year>2023</year>
            </pub-date>
            <volume>12</volume>
            <elocation-id>860</elocation-id>
            <history>
                <date date-type="accepted">
                    <day>3</day>
                    <month>1</month>
                    <year>2024</year>
                </date>
            </history>
            <permissions>
                <copyright-statement>Copyright: &#x00a9; 2024 Uebo K et al.</copyright-statement>
                <copyright-year>2024</copyright-year>
                <license xlink:href="https://creativecommons.org/licenses/by/4.0/">
                    <license-p>This is an open access article distributed under the terms of the Creative Commons Attribution Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
                </license>
            </permissions>
            <self-uri content-type="pdf" xlink:href="https://f1000research.com/articles/12-860/pdf"/>
            <abstract>
                <sec>
                    <title>Background</title>
                    <p>Magneto-optical Kerr effect (MOKE) microscopes are powerful experimental tools to observe magnetic domains in magnetic materials. These devices are, however, typically large, unportable, and expensive (&#x223c; several million yen), and therefore prevent many researchers in the field of materials science from easy access to study real-space images of magnetic domains.</p>
                </sec>
                <sec>
                    <title>Methods</title>
                    <p>To overcome these issues, we utilized data from &#x201c;The OpenFlexure Project&#x201d; developed by the University of Bath and the University of Cambridge. The purpose of this project is to make high-precision mechanical positioning of the studied sample available to anyone with a 3D printer, especially for use in microscopes. We built a low-cost and portable MOKE microscope device with a 3D printer. We redesigned the 3D modeling data of an ordinary optical microscope provided by The OpenFlexure project and incorporated additional elements, such as optical polarizers and an electromagnetic coil into the primarily designed microscope that did not originally have these elements.</p>
                </sec>
                <sec>
                    <title>Results</title>
                    <p>We successfully observed magnetic domains and their real-space motions induced by magnetic fields using the palm-sized low-cost MOKE microscope, which costs approximately 30,000 yen in raw materials to construct.</p>
                </sec>
                <sec>
                    <title>Conclusions</title>
                    <p>Our methodology to assemble a low-cost MOKE microscope will enable researchers working in the field of materials science to observe magnetic domains more easily without commercial equipment.</p>
                </sec>
            </abstract>
            <kwd-group kwd-group-type="author">
                <kwd>The OpenFlexure project</kwd>
                <kwd>Magneto-Optical Kerr microscope</kwd>
                <kwd>3D printing technology</kwd>
                <kwd>low-cost</kwd>
            </kwd-group>
            <funding-group>
                <award-group id="fund-1">
                    <funding-source>MEXT Q-LEAP</funding-source>
                    <award-id>JPMXS0118068681</award-id>
                </award-group>
                <award-group id="fund-2">
                    <funding-source>Asahi Glass Foundation</funding-source>
                </award-group>
                <award-group id="fund-3">
                    <funding-source>The Japan Science Society</funding-source>
                </award-group>
                <award-group id="fund-4" xlink:href="http://dx.doi.org/10.13039/501100001691">
                    <funding-source>Japan Society for the Promotion of Science</funding-source>
                    <award-id>JP19H05824</award-id>
                </award-group>
                <funding-statement>This work was supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Number JP19H05824&#13;
(to HW), the Ministry of Education, Culture, Sports, Science and Technology (MEXT) Quantum Leap (Q-LEAP) Flagship&#13;
Program under Grant No. JPMXS0118068681 (to HW), the Asahi Glass Foundation (to HW), and the Sasakawa Scientific&#13;
Research Grant from The Japan Science Society (to RT)</funding-statement>
                <funding-statement>
                    <italic>The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.</italic>
                </funding-statement>
            </funding-group>
        </article-meta>
        <notes>
            <sec sec-type="version-changes">
                <label>Revised</label>
                <title>Amendments from Version 1</title>
                <p>The main revisions are the following. 1. We find that the OpenFlexure Project was mentioned several times in the introduction and Hardware Design sections. Therefore, we revised some sentences in these sections to avoid clutter. We also revised the English expressions throughout the text. 2. We included the information on the power supply as DC power supply 6,000, Kungber stabilized power supply, 0-30V, 0-5A in Table 1. We also revised the information in this table. The total cost was changed from 20000 to 30000 yen. 3. In Fig. 3, we changed the external field unit of the right loop from kAm-1 to mT by using the relationship of 1 mT = 0.7958 kAm-1. 4. We revised the information in Reference 4 as 
                    <italic>Opt. Express.</italic> 2022;30(13):23216&#x2013;23298. 10.1364/OE.461910. 5. We added References 10-12.</p>
            </sec>
        </notes>
    </front>
    <body>
        <sec id="sec1" sec-type="intro">
            <title>Introduction</title>
            <p>In recent years, the &#x201c;provision of goods and services that meet diverse needs without disparity&#x201d; in Society 5.0 and &#x201c;production that does not waste resources&#x201d; in the Sustainable Development Goals (SDGs) have been of importance in our society.
                <sup>
                    <xref ref-type="bibr" rid="ref1">1</xref>
                </sup> In this respect, 3D printing technology plays a key role in many occasions from manufacturing and construction to hobbies, in which one can create new objects from conceptions regardless of age, lifestyle, and occupation. In the field of science, 3D printing technology is being used to significantly reduce the cost of experimental equipment and to develop new optical elements such as optical choppers, filter brackets, and rails.
                <sup>
                    <xref ref-type="bibr" rid="ref2">2</xref>
                </sup> It is, therefore, expected that researchers can conduct more experiments along this research direction with a finite budget since low-cost experimental equipment becomes available and experiments can be conducted without buying expensive equipment. One of the applications of 3D printing technology is to design and build microscopes with various external parameters such as magnetic fields. Combining optical systems and data processing methods with a 3D printed microscope, observations with the in-plane resolution of several hundred nanometers have recently been achieved.
                <sup>
                    <xref ref-type="bibr" rid="ref3">3</xref>
                </sup>
                <sup>,</sup>
                <sup>
                    <xref ref-type="bibr" rid="ref4">4</xref>
                </sup> Furthermore, it has been reported that the sample stage can be moved with the precision of several tens of nanometers.
                <sup>
                    <xref ref-type="bibr" rid="ref5">5</xref>
                </sup>
                <sup>,</sup>
                <sup>
                    <xref ref-type="bibr" rid="ref6">6</xref>
                </sup> The mechanism of these sample stages was developed in the project called &#x201c;
                <ext-link ext-link-type="uri" xlink:href="https://openflexure.org/projects/microscope/build">The OpenFlexure Project</ext-link>&#x201d;, developed by the University of Bath and the University of Cambridge, in which the slight expansion and contraction of the plastic material is adjusted by a rubber band (O-ring). These recent technical developments enable the stage movement along any direction in three dimensions, which is often required for the practical use of optical microscopes. The 3D printed microscopes with nanometer scale in-plane resolution and precision of stage movement are already easily available for end-users with a 3D printer.</p>
            <p>In this article, we report the development of a 3D printed microscope to observe a real-space image of magnetic domains in magnetic materials by means of the magneto-optical Kerr effect (MOKE), i.e., a phenomenon that the polarization of the reflected light is rotated by a magnetic material in response to an applied linearly polarized light. To observe these magnetic domains, large and expensive equipment such as optical tables and polarizing microscopes have routinely been used since deflecting elements are required. Nevertheless, we successfully made a compact and low-cost MOKE microscope using 3D printing technology without large-scale commercial equipment. The sample observed in this study is a magneto-optical (MO) sensor to demonstrate the feasibility of our new 3D-printed microscope in the present work. We choose the MO sensor particularly because a material with perpendicular magnetic anisotropy enables us to observe magnetic domains and their motions appearing on the surface of a magnetic sample with MOKE. We incorporated an electromagnet into the microscope to scrutinize the motions of magnetic domains caused by magnetic fields. Our 3D-printed microscope to observe magnetic domains can be applied to a range of materials, including thin films of NiCo
                <sub>2</sub>O
                <sub>4</sub>, iron garnet, Pt/Co and CoFeB,
                <sup>
                    <xref ref-type="bibr" rid="ref7">7</xref>
                </sup>
                <sup>&#x2013;</sup>
                <sup>
                    <xref ref-type="bibr" rid="ref12">12</xref>
                </sup> which are attracting attention towards next-generation electronic device applications.</p>
        </sec>
        <sec id="sec2">
            <title>Hardware design</title>
            <p>The MOKE microscope device using 3D printing technology was fabricated based on a microscope device distributed in 
                <ext-link ext-link-type="uri" xlink:href="https://openflexure.org/projects/microscope/build">The OpenFlexure Project</ext-link>. 
                <xref ref-type="fig" rid="f1">Figure 1</xref> shows a 3D-printed MOKE microscope device that we have built in the present study. A key development of our study is to make it possible to build a portable MOKE microscope. The actuator gear is used for the X-Y stage movements. This gear makes the microscope portable because this gear does not require a large space. Specifically, the dimensions of the microscope are 105 &#x00d7; 105 &#x00d7; 160 mm
                <sup>3</sup>. Therefore, they are considerably smaller than conventional microscopes. In the following, we will examine details of the 3D printed MOKE microscope and its applications to studies of magnetic materials. Firstly, we elaborate on optical paths, components, and the design of our MOKE microscope, referring to the cost and performance of each optical element. Also, we describe actual measurements of magnetic domains and their motions caused by magnetic fields in a magnetic material to demonstrate the performance of our newly developed MOKE microscope.</p>
            <fig fig-type="figure" id="f1" orientation="portrait" position="float">
                <label>Figure 1. </label>
                <caption>
                    <title>MOKE (Magneto-optical Kerr effect) microscope fabricated by a 3D printer.</title>
                    <p>(a-c)(Left) Original 3D modeling data.
                        <sup>
                            <xref ref-type="bibr" rid="ref5">5</xref>
                        </sup> (Right) Modified 3D modeling data of the counterpart components used in this study. The red frames indicate the main parts that we redesigned. Note that the angle of the rod for Polarizer 1, shown in panel b, can vary from -75 to 75 degrees in the microscope.</p>
                </caption>
                <graphic id="gr1" orientation="portrait" position="float" xlink:href="https://f1000research-files.f1000.com/manuscripts/155207/b8e61fee-ca5a-4aaf-be6a-455633c15d73_figure1.gif"/>
            </fig>
            <p>The optical path of the microscope can be seen in 
                <xref ref-type="fig" rid="f2">Figure 2</xref>. The light path from the light source to the sample is as follows: Light-emitting diode (LED) &#x2192; Condenser Lens &#x2192; Polarizer1 &#x2192; Beam splitter &#x2192; Tube Lens &#x2192; Objective Lens &#x2192; Sample. The light reflected from the sample reaches the camera through the following optical path: Sample &#x2192; Objective Lens &#x2192; Tube Lens &#x2192; Beam splitter &#x2192; Polarizer2 &#x2192; Camera for imaging. This microscope employs the K&#x00f6;hler illumination method, where the illuminated light becomes collimated on the sample surface by using the three lenses. This ensures the uniformity of the LED illumination.
                <sup>
                    <xref ref-type="bibr" rid="ref13">13</xref>
                </sup> A vital development of this microscope is a polarizing element to observe magnetic domains using MOKE. Another distinctive feature of our design is the stage movement using O-rings and the ability to easily change the design of the device using 3D modeling data taken from OpenFlexure and edited with software 
                <ext-link ext-link-type="uri" xlink:href="https://www.autodesk.co.jp/products/fusion-360/overview">Fusion360 (ver2.0.14569</ext-link>). Note that 3D modeling data edited in Fusion360 here can also be edited in other software available for free, such as 
                <ext-link ext-link-type="uri" xlink:href="https://www.freecad.org/index.php">FreeCAD</ext-link>. To move the sample stage, one can rotate the actuator gear shown in 
                <xref ref-type="fig" rid="f1">Figure 1</xref>, making the O-ring expand and contract, which in turn moves the X-Y stage shown in 
                <xref ref-type="fig" rid="f1">Figure 1</xref>. 
                <xref ref-type="fig" rid="f1">Figure 1(a)-(c)</xref> show our upgrades of three components in our microscope. These revised components are important to make the MOKE microscope for practical use. We elaborate on these modifications in the following. The body (
                <xref ref-type="fig" rid="f1">Figure 1(a)</xref>) was edited to sufficiently change the position of the sample stage along the Z-axis. We got rid of the black part indicated by a red rectangle shown in 
                <xref ref-type="fig" rid="f1">Figure 1(a)</xref> to insert the rods (
                <xref ref-type="fig" rid="f1">Figure 1(b)</xref>) to rotate the polarizer1. With this modification, the distance from the objective lens to the sample can be adjusted when the objective lens with different magnification is replaced. As shown in 
                <xref ref-type="fig" rid="f1">Figure 1(b)</xref>, we added two rods to rotate the polarizing element because the MOKE microscope requires adjustment of the rotation angle of the polarizing element during measurements depending on the Kerr angles of magnetic materials, which in general differ from sample to sample. The rod can be mechanically rotated by hand. The angle of the holder can vary from -75 to 75 degrees in the current setup. 
                <xref ref-type="fig" rid="f1">Figure 1(c)</xref> displays a component to install an electromagnet on top of the sample, enabling the application of a magnetic field perpendicular to the sample. To calibrate the magnitude of the magnetic field, a tesla meter (TM-801, KANETEC) was used. The measuring portion of the tesla meter instrument was placed at the position of the sample to be observed, and the instrument was calibrated after confirming that the sample was illuminated by light. We carefully measured the magnitude of the magnetic field at the position of the sample.</p>
            <fig fig-type="figure" id="f2" orientation="portrait" position="float">
                <label>Figure 2. </label>
                <caption>
                    <title>Schematic cross-sectional view of the MOKE (Magneto-optical Kerr effect) microscope.</title>
                    <p>The reflective geometry is realized using an LED as a light source and a beam splitter. The electromagnet storage and polarizers are additional components to make an ordinary optical microscope into a MOKE microscope.</p>
                </caption>
                <graphic id="gr2" orientation="portrait" position="float" xlink:href="https://f1000research-files.f1000.com/manuscripts/155207/b8e61fee-ca5a-4aaf-be6a-455633c15d73_figure2.gif"/>
            </fig>
            <p>We refer to the cost and performance of each optical element used to assemble our microscope in 
                <xref ref-type="table" rid="T1">Table 1</xref>. The total cost of filaments (ingredients of the 3D printing) and all the components to fabricate the MOKE microscope is 30,000 yen. This is an excellent cost performance in comparison with standard commercial MOKE microscopes. For instance, 
                <ext-link ext-link-type="uri" xlink:href="https://www.wakenyaku.co.jp/ctg/det.php?i=228">ZEISS Axio Imager</ext-link> costs &gt;2,000,000 yen. Instead of purchasing such an expensive instrument, it is thus possible to access a MOKE microscope whose parameters can easily be improved with better optical elements such as objective lenses and tube lenses depending on the requirements of specific measurements.</p>
            <table-wrap id="T1" orientation="portrait" position="float">
                <label>Table 1. </label>
                <caption>
                    <title>List of optical elements used in the present work and their performance.</title>
                </caption>
                <table content-type="article-table" frame="hsides">
                    <thead>
                        <tr>
                            <th align="left" colspan="1" rowspan="1" valign="top">Elements used</th>
                            <th align="left" colspan="1" rowspan="1" valign="top">Price (yen)</th>
                            <th align="left" colspan="1" rowspan="1" valign="top">Product name</th>
                            <th align="left" colspan="1" rowspan="1" valign="top">Performance</th>
                        </tr>
                    </thead>
                    <tbody>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">LED</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">10</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.amazon.co.jp/dp/B07BXJ6RZT">DiCUNO light emitting diode 5 mm</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">12 candela</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Objective lens</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">2,100</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.amazon.co.jp/dp/B07PM73VFD">Wal frontxdsn3102k8</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">10&#x00d7;, Objective lens length 31.3 mm</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Electromagnet</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">1,600</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.monotaro.com/p/5043/3383/">NaRiKa for general contractors</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <italic toggle="yes">&#x03d5;</italic>0.4 mm (Enameled wire), 400 rolls, Iron (Core material)</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Camera</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">4,100</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://ja.aliexpress.com/item/32908728111.html">AliExpress HBVCAM-1710-H264 V33</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">Pixel size 2.2 &#x03bc;m &#x00d7; 2.2 &#x03bc;m, RGB</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Condenser lens</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">100</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.amazon.co.jp/dp/B07SB48KYG">Easybuyseller G100008</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <italic toggle="yes">&#x03d5;</italic>17 mm, 3.2 mm (Lens thickness), 28 mm (Focal length)</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Tube lens</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">7,500</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.thorlabs.co.jp/thorproduct.cfm?partnumber=AC127-050-A">THORLABS AC127-050-A</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <italic toggle="yes">&#x03d5;</italic>12.7 mm, 5.0 mm (Lens thickness), 50.0 mm (Focal length)</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Half mirror</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">3,000</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.shibuya-opt.co.jp/harf_mirror01.html">Shibuya Optical Co., Ltd. H282</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">1.5 mm (Mirror thickness), Transmission: Reflectance = 1:1</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">Polarizer</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">1,200</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.thorlabs.co.jp/thorproduct.cfm?partnumber=LPVISE2X2">THORLABS LPVISE2X2</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">Extinction ratio 100:1 or more in the visible light range</td>
                        </tr>
                        <tr>
                            <td align="left" colspan="1" rowspan="1" valign="top">DC power supply</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">6,000</td>
                            <td align="left" colspan="1" rowspan="1" valign="top">
                                <ext-link ext-link-type="uri" xlink:href="https://www.amazon.co.jp/dp/B0923KKYTG">Kungber stabilized power supply</ext-link>
                            </td>
                            <td align="left" colspan="1" rowspan="1" valign="top">0-30 V, 0-5 A</td>
                        </tr>
                    </tbody>
                </table>
            </table-wrap>
            <p>The microscope fabricated in this study was used to image patterns of magnetic domains appearing on the surface of a magnetic sample. An electromagnet is placed above the sample, and the magnetic field is controlled by a DC power supply. Images were generated with a USB camera connected to a standard computer. The sample measured in this work is a MO sensor (Matesy GmbH: Magneto-optical sensors with mirror and DLC protection (type-A)), whose magnetic domains of the sample surface can be controlled by applying a magnetic field. The magnetic domain patterns were binarized with image analysis software (
                <ext-link ext-link-type="uri" xlink:href="https://www.wavemetrics.com/">Igor 6.0</ext-link> and 
                <ext-link ext-link-type="uri" xlink:href="https://imagej.nih.gov/ij/index.html">ImageJ 1.53e</ext-link>). Such image analyses implemented in Igor can also be carried out in primitive programming languages such as 
                <ext-link ext-link-type="uri" xlink:href="https://www.python.org/">Python</ext-link>. The camera properties, such as brightness, vividness, exposure, and backlight correction, were specified during imaging using free software called 
                <ext-link ext-link-type="uri" xlink:href="https://freesoft-100.com/review/webcamsetting.html">WebCamSetting 1.1.0.0</ext-link>. Specifically, the brightness and vividness were set to the minimum value of 0, whereas the exposure and backlight correction were kept as default. This setting allows us to observe MOKE images clearly.</p>
        </sec>
        <sec id="sec3" sec-type="methods">
            <title>Methods</title>
            <p>Here, we describe the methods of data acquisition and analysis. A USB camera was connected to the computer for the data acquisition and camera images were obtained using default camera settings. To binarize the images, we used the iterated binarization method in the Igor software. Since the ratio of dark and bright areas can be quantified with ImageJ, the data format was converted from image data to numerical values of &#x00b1;1 to obtain the Kerr intensity in 
                <xref ref-type="fig" rid="f3">Figure 3</xref> quantitatively. Care was taken to record the data at the same areas of the sample surfaces while taking images with 10 different magnetic fields (&#x00b1;7.6, &#x00b1;3.8, &#x00b1;1.9, &#x00b1;1.1 and &#x00b1;0.76 mT) to evaluate magnetic field effects on the images.</p>
            <fig fig-type="figure" id="f3" orientation="portrait" position="float">
                <label>Figure 3. </label>
                <caption>
                    <title>(Left) Magnetic field dependence of the Kerr intensity and the magnetic domains of the MO (magneto-optical) sensor observed with our 3D printed Kerr effect microscope and plotted by using Igor6.0. The measurements were carried out at room temperature (~ 290 Kelvin) and 10 different magnetic fields (&#x00b1;7.6, &#x00b1;3.8, &#x00b1;1.9, &#x00b1;1.1 and &#x00b1;0.76 mT). The Kerr intensity is defined as the differential areas of the respective domains within the scope and thereby represents the macroscopic magnetization of the sample. The numbers next to the data points in the graph indicate the original images used to estimate the Kerr intensity. (Right) Magnetic field dependence of the magnetization, which is estimated by the Faraday rotation data provided by Matesy GmbH.</title>
                </caption>
                <graphic id="gr3" orientation="portrait" position="float" xlink:href="https://f1000research-files.f1000.com/manuscripts/155207/b8e61fee-ca5a-4aaf-be6a-455633c15d73_figure3.gif"/>
            </fig>
            <p>To eliminate the background signals in the image data shown in 
                <xref ref-type="fig" rid="f3">Figure 3</xref>, the darkest image at &#x2212;7.6 mT (the single magnetic domain, mirroring the macroscopically saturated magnetization by enough magnetic field) is used as a representing background signal. Magnetic domain images at 10 different magnetic fields are subtracted from the image (1) with software (ImageJ converts the image data into numerical values).</p>
        </sec>
        <sec id="sec4" sec-type="results">
            <title>Results</title>
            <p>The data associated with this article are available in 
                <italic toggle="yes">Underlying data.</italic>
                <sup>
                    <xref ref-type="bibr" rid="ref14">14</xref>
                </sup> 
                <xref ref-type="fig" rid="f3">Figure 3</xref> shows images of the magnetic domains of the MO sensor under magnetic fields varying from &#x2212;7 mT to +7 mT using the electromagnet placed above the sample. These data were collected at room temperature, and a white LED shown in 
                <xref ref-type="table" rid="T1">Table 1</xref> was used as a light source. The image is monochromatic dark when enough magnetic field was applied. This is an expected behavior for ferromagnets when the total magnetization is saturated by the external field. Upon the application of a magnetic field, we clearly observed domains in the bright color (we characterized color as either bright or dark), which indicates that the magnetic domains along the other direction are induced by the field (
                <xref ref-type="fig" rid="f3">Figure 3</xref> (1) and (2)). It is also appreciable that the entire contrast of the image is drastically changed when the sign of the field is reversed (
                <xref ref-type="fig" rid="f3">Figure 3</xref> (3) and (4)). The image is dominated by domains in the bright color and is finally monochromatic bright when the substantial field was applied along the opposite direction to the initial field (
                <xref ref-type="fig" rid="f3">Figure 3</xref> (5)). Considering these real-space observations, we have analyzed the contrast of the images to estimate the magnetic field dependence of the net magnetization of the MO sensor. The Kerr intensity is defined as the differential areas of the respective domains within the scope and thereby represents the macroscopic magnetization of the sample. The magnetic field dependence of the Kerr intensity is consistent with the observations of the original images and reminiscent of the typical 
                <italic toggle="yes">M</italic>-
                <italic toggle="yes">H</italic> curve of ferromagnets. Specifically, the coercive field inferred from the Kerr intensity is 2 mT, which quantitatively agrees with the experimental data of Faraday rotation provided by the company Matesy GmbH in 
                <xref ref-type="fig" rid="f3">Figure 3</xref> (right).</p>
        </sec>
        <sec id="sec5" sec-type="conclusions">
            <title>Conclusions</title>
            <p>In conclusion, we have assembled a MOKE microscope using 3D printing technology. The total price is less than 2% of that of the standard commercial MOKE microscope, based on the comparisons we have made (for example, ZEISS Axio Imager costs &gt;2,000,000 yen). To substantially reduce the size of the MOKE microscope, we utilized the 3D modeling provided by the OpenFlexure Project (and such an attempt to assemble a 3D printed MOKE microscope is for the first time to the best of our knowledge). The feasibility of our 3D-printed MOKE microscope is well confirmed by the measurements of the real-space images of the magnetic domains of the MO sensor under the magnetic fields and the analysis of the macroscopic magnetization estimated from these images.</p>
            <p>On the experimental front, one can extend the maximum values of the magnetic field by replacing the electromagnet with the one which can tolerate higher electrical currents or superconducting magnets. The real-space resolution can be improved by increasing the magnification of the objective lens. These amplifications of the external parameters should be straightforward for end-users and can be achieved with reasonable costs compared to the price of conventional commercial MOKE microscopes. We thus believe that MOKE microscopes will be more easily available and customizable in the field of materials science along the direction we present in this work.</p>
        </sec>
    </body>
    <back>
        <sec id="sec8" sec-type="data-availability">
            <title>Data availability</title>
            <sec id="sec9">
                <title>Underlying data</title>
                <p>The original 3D printing data from &#x201c;The OpenFlexure Project&#x201d; is available for download here: 
                    <ext-link ext-link-type="uri" xlink:href="https://openflexure.org/projects/microscope/build">https://openflexure.org/projects/microscope/build</ext-link>.</p>
                <p>Zenodo: koki-u/3d_microscope: Kerr microscope. 
                    <ext-link ext-link-type="uri" xlink:href="https://doi.org/10.5281/zenodo.7950835">https://doi.org/10.5281/zenodo.7950835</ext-link>.
                    <sup>

                        <xref ref-type="bibr" rid="ref14">14</xref>
</sup>
                </p>
                <p>This project contains the following underlying data:
                    <list list-type="bullet">
                        <list-item>
                            <label>&#x2022;</label>
                            <p>Modified (3D print files).</p>
                        </list-item>
                        <list-item>
                            <label>&#x2022;</label>
                            <p>Image (image files).
</p>
                        </list-item>
                    </list>
                </p>
                <p>Data are available under the terms of the 
                    <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0 International license</ext-link> (CC-BY 4.0).</p>
            </sec>
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    <sub-article article-type="reviewer-report" id="report235789">
        <front-stub>
            <article-id pub-id-type="doi">10.5256/f1000research.155207.r235789</article-id>
            <title-group>
                <article-title>Reviewer response for version 2</article-title>
            </title-group>
            <contrib-group>
                <contrib contrib-type="author">
                    <name>
                        <surname>Rodriguez</surname>
                        <given-names>Aurelio Hierro</given-names>
                    </name>
                    <xref ref-type="aff" rid="r235789a1">1</xref>
                    <role>Referee</role>
                    <uri content-type="orcid">https://orcid.org/0000-0001-6600-7801</uri>
                </contrib>
                <contrib contrib-type="author">
                    <name>
                        <surname>Cascales-Sandoval</surname>
                        <given-names>Miguel Angel</given-names>
                    </name>
                    <xref ref-type="aff" rid="r235789a2">2</xref>
                    <role>Co-referee</role>
                </contrib>
                <aff id="r235789a1">
                    <label>1</label>University of Oviedo (Ringgold ID: 16763), Oviedo, Asturias, Spain</aff>
                <aff id="r235789a2">
                    <label>2</label>Technische Universitat Wien, Vienna, Vienna, Austria</aff>
            </contrib-group>
            <author-notes>
                <fn fn-type="conflict">
                    <p>
                        <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                </fn>
            </author-notes>
            <pub-date pub-type="epub">
                <day>9</day>
                <month>4</month>
                <year>2024</year>
            </pub-date>
            <permissions>
                <copyright-statement>Copyright: &#x00a9; 2024 Rodriguez AH and Cascales-Sandoval MA</copyright-statement>
                <copyright-year>2024</copyright-year>
                <license xlink:href="https://creativecommons.org/licenses/by/4.0/">
                    <license-p>This is an open access peer review report distributed under the terms of the Creative Commons Attribution Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
                </license>
            </permissions>
            <related-article ext-link-type="doi" id="relatedArticleReport235789" related-article-type="peer-reviewed-article" xlink:href="10.12688/f1000research.133292.2"/>
            <custom-meta-group>
                <custom-meta>
                    <meta-name>recommendation</meta-name>
                    <meta-value>reject</meta-value>
                </custom-meta>
            </custom-meta-group>
        </front-stub>
        <body>
            <p>The author hasn't included my suggestion in detail.</p>
            <p>Is the work clearly and accurately presented and does it cite the current literature?</p>
            <p>No</p>
            <p>If applicable, is the statistical analysis and its interpretation appropriate?</p>
            <p>No</p>
            <p>Are all the source data underlying the results available to ensure full reproducibility?</p>
            <p>Yes</p>
            <p>Is the study design appropriate and is the work technically sound?</p>
            <p>Partly</p>
            <p>Are the conclusions drawn adequately supported by the results?</p>
            <p>No</p>
            <p>Are sufficient details of methods and analysis provided to allow replication by others?</p>
            <p>No</p>
            <p>Reviewer Expertise:</p>
            <p>Nanomagnetism, X-ray Transmission Microscopy, Magneto-optics, Magnetic Thin Films</p>
            <p>We confirm that we have read this submission and believe that we have an appropriate level of expertise to state that we do not consider it to be of an acceptable scientific standard, for reasons outlined above.</p>
        </body>
        <sub-article article-type="response" id="comment11414-235789">
            <front-stub>
                <contrib-group>
                    <contrib contrib-type="author">
                        <name>
                            <surname>Wadati</surname>
                            <given-names>Hiroki</given-names>
                        </name>
                        <aff>University of Hyogo, Japan</aff>
                    </contrib>
                </contrib-group>
                <author-notes>
                    <fn fn-type="conflict">
                        <p>
                            <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                    </fn>
                </author-notes>
                <pub-date pub-type="epub">
                    <day>12</day>
                    <month>4</month>
                    <year>2024</year>
                </pub-date>
            </front-stub>
            <body>
                <p>The reviewer should specify which suggestions are required so that we can respond appropriately.</p>
                <p> </p>
                <p> Regards,</p>
                <p> Hiroki Wadati</p>
            </body>
        </sub-article>
    </sub-article>
    <sub-article article-type="reviewer-report" id="report215081">
        <front-stub>
            <article-id pub-id-type="doi">10.5256/f1000research.146271.r215081</article-id>
            <title-group>
                <article-title>Reviewer response for version 1</article-title>
            </title-group>
            <contrib-group>
                <contrib contrib-type="author">
                    <name>
                        <surname>Rodriguez</surname>
                        <given-names>Aurelio Hierro</given-names>
                    </name>
                    <xref ref-type="aff" rid="r215081a1">1</xref>
                    <role>Referee</role>
                    <uri content-type="orcid">https://orcid.org/0000-0001-6600-7801</uri>
                </contrib>
                <contrib contrib-type="author">
                    <name>
                        <surname>Cascales-Sandoval</surname>
                        <given-names>Miguel Angel</given-names>
                    </name>
                    <xref ref-type="aff" rid="r215081a2">2</xref>
                    <role>Co-referee</role>
                </contrib>
                <aff id="r215081a1">
                    <label>1</label>University of Oviedo (Ringgold ID: 16763), Oviedo, Asturias, Spain</aff>
                <aff id="r215081a2">
                    <label>2</label>Technische Universitat Wien, Vienna, Vienna, Austria</aff>
            </contrib-group>
            <author-notes>
                <fn fn-type="conflict">
                    <p>
                        <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                </fn>
            </author-notes>
            <pub-date pub-type="epub">
                <day>25</day>
                <month>10</month>
                <year>2023</year>
            </pub-date>
            <permissions>
                <copyright-statement>Copyright: &#x00a9; 2023 Rodriguez AH and Cascales-Sandoval MA</copyright-statement>
                <copyright-year>2023</copyright-year>
                <license xlink:href="https://creativecommons.org/licenses/by/4.0/">
                    <license-p>This is an open access peer review report distributed under the terms of the Creative Commons Attribution Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
                </license>
            </permissions>
            <related-article ext-link-type="doi" id="relatedArticleReport215081" related-article-type="peer-reviewed-article" xlink:href="10.12688/f1000research.133292.1"/>
            <custom-meta-group>
                <custom-meta>
                    <meta-name>recommendation</meta-name>
                    <meta-value>reject</meta-value>
                </custom-meta>
            </custom-meta-group>
        </front-stub>
        <body>
            <p>The authors report on the development and implementation of a cheap 3D printed Kerr Microscope based on the main design of &#x201c;The OpenFlexure Project&#x201d;. The idea is very interesting and really brings the capability of performing Kerr Microscopy with small and cheap instruments. However, there are several and important flaws in the work, from its redaction to the discussion and conclusions, passing through the experimental details, that prevent us from recommending this manuscript for its publication. Here follows our indications and comments.</p>
            <p> </p>
            <p> As a general first comment, the content is sometimes repetitive which makes the general reading difficult, thus the style should be improved.</p>
            <p> </p>
            <p> In the introduction, current literature on 3D printing is referenced, however, no citations appear about other Kerr Microscope setups for information and comparison with current state of the art techniques. As this work is focused on Kerr Microscopy, it should be very important to have this framework well defined.</p>
            <p> </p>
            <p> Also in the introduction, it is not clear for me what the authors mean with the sentence saying that the stage can be moved several tens of nanometers. Is this indicating the precision of the movement using the 3D printed stage actuators, or is the total displacement possible per axis? If it is the first case, then there is a clear problem as tens of nanometers is a very limited movement range for an optical microscope. Clarify.</p>
            <p> </p>
            <p> Also in the introduction section, what is the meaning of depth resolution at the end of the first paragraph? Is that the depth of focus or the precision of the Z stage? If it is the first, then this strongly depends on the objective used and it is usually in the range of ~1 um.</p>
            <p> </p>
            <p> In the second paragraph of the introduction, the application of the method to be discussed is focused towards a very specific material (NiCo2O4). If this work is devoted to present a general purpose and cheap Kerr Microscope, a wider discussion about systems where it could be used as a useful characterization tool should be cited and discussed briefly.</p>
            <p> </p>
            <p> In the Hardware design section, a more thorough description of the polarization optics should be done as it is the key for a proper functioning of a Kerr Microscope. It would be great if comparison with in-plane magnetization sensitive microscopes would be done, as there are plenty of systems where in-plane magnetization is the main actor.</p>
            <p> </p>
            <p> As a comment, in figure 1 caption, maybe it is not necessary to include the citation for the OpenFlexure Project as it is already in the main text. The caption should focus on the figure itself.</p>
            <p> </p>
            <p> There is a typo in the description in the main text of figure 1(a): &#x201c;by a red rectangular&#x201d; should be &#x201c;by a red rectangle&#x201d;.</p>
            <p> </p>
            <p> The maximum rotation of the analyser should be indicated in the description of panel b of figure 1 as this is important for the tuning of the microscope. Could it be possible to include a retarder waveplate in the design in addition to the analyser too as it exists in other KM for signal optimization? A comment about this would be helpful as this would indicate that the authors have reviewed current Kerr Microscope setups in detail.</p>
            <p> </p>
            <p> We find the discussion about the electromagnet design very obscure. As it is a very important part of the microscope, it should be described with more detail indicating core material, remanent field, possible heating problems such as 3D printed plastic deformation? Also, stability of the microscope while utilization with the magnetic field on. Interference of the magnetic field with magnetic parts of the objective?</p>
            <p> </p>
            <p> Just a minor comment, probably, the price of the power supply for the electromagnet should be included in the total price of the microscope.</p>
            <p> </p>
            <p> In the discussion about the domain imaging and analysis of the Magneto-optic sensor provided by Matesy Gmbh, we have a lot of doubts.</p>
            <p> </p>
            <p> First of all, why the authors binarize the data for its processing? The intensity of the signal recorded by the camera if it works in a linear manner is very important and can give useful information about the orientation of the magnetization within the system (vector sensitivity inherent to the MO effect). Here it is important also to indicate the dynamic range of the camera used as well as its relation with the smallest signal that the microscope can measure. A thorough discussion about this is mandatory as this work is describing a characterization technique.</p>
            <p> </p>
            <p> Another important point here is the fact that the sample used for demonstrating the proof of concept does not really use the Kerr effect, but the Faraday effect which gives a huge signal when compared with polar Kerr for instance. The rotation indicated in figure 3 by the manufacturer of the sensor indicates a rotation of +/-8 degrees between saturations. This is very easy to measure and is adequate for an initial demonstration, but real samples measured using Kerr configuration will most probably show way smaller rotations of the polarization. In this regard, how are the low extinction ratio polarizers going to work? At this point we think that in order to demonstrate real capabilities of the proposed microscope, a real sample where Kerr effect is used for its characterization is mandatory, as is in this configuration where the microscope should work.</p>
            <p> </p>
            <p> Finally, two comments about figure 3. The external field units of the two loops (half-loops) presented should be the same, and the normalization protocol used for removing background and getting magnetic signal should be better clarified. As it is now, I understand that image 1 (-3.8 mT) is the one used for normalization, which shows stripes. If this is the image taken for normalization, why aren&#x2019;t these stripes present always in all the images? A fully flat image should be taken to work as reference and then the microscope would be working in differential mode. Have the authors observed strong Faraday effects due to the objective optics in combination with the external field from the electromagnet? Please clarify this point.</p>
            <p>Is the work clearly and accurately presented and does it cite the current literature?</p>
            <p>No</p>
            <p>If applicable, is the statistical analysis and its interpretation appropriate?</p>
            <p>No</p>
            <p>Are all the source data underlying the results available to ensure full reproducibility?</p>
            <p>Yes</p>
            <p>Is the study design appropriate and is the work technically sound?</p>
            <p>Partly</p>
            <p>Are the conclusions drawn adequately supported by the results?</p>
            <p>No</p>
            <p>Are sufficient details of methods and analysis provided to allow replication by others?</p>
            <p>No</p>
            <p>Reviewer Expertise:</p>
            <p>Nanomagnetism, X-ray Transmission Microscopy, Magneto-optics, Magnetic Thin Films</p>
            <p>We confirm that we have read this submission and believe that we have an appropriate level of expertise to state that we do not consider it to be of an acceptable scientific standard, for reasons outlined above.</p>
        </body>
        <sub-article article-type="response" id="comment10788-215081">
            <front-stub>
                <contrib-group>
                    <contrib contrib-type="author">
                        <name>
                            <surname>Wadati</surname>
                            <given-names>Hiroki</given-names>
                        </name>
                        <aff>University of Hyogo, Japan</aff>
                    </contrib>
                </contrib-group>
                <author-notes>
                    <fn fn-type="conflict">
                        <p>
                            <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                    </fn>
                </author-notes>
                <pub-date pub-type="epub">
                    <day>19</day>
                    <month>12</month>
                    <year>2023</year>
                </pub-date>
            </front-stub>
            <body>
                <p>The authors report on the development and implementation of a cheap 3D printed Kerr Microscope based on the main design of &#x201c;The OpenFlexure Project&#x201d;. The idea is very interesting and really brings the capability of performing Kerr Microscopy with small and cheap instruments. However, there are several and important flaws in the work, from its redaction to the discussion and conclusions, passing through the experimental details, that prevent us from recommending this manuscript for its publication. Here follows our indications and comments.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We thank the reviewers for their careful reading of our manuscript and for providing us with constructive comments. In the following, we answer their concerns one by one and point out the changes made in the manuscript to improve both the discussion and the figures following his suggestions.</p>
                <p> </p>
                <p> 1. As a general first comment, the content is sometimes repetitive which makes the general reading difficult, thus the style should be improved.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We find that the OpenFlexure Project was mentioned several times in the introduction and Hardware Design sections. Therefore, we revised some sentences in these sections to avoid clutter. We also revised the English expressions throughout the text.</p>
                <p> </p>
                <p> 2. In the introduction, current literature on 3D printing is referenced, however, no citations appear about other Kerr Microscope setups for information and comparison with current state of the art techniques. As this work is focused on Kerr Microscopy, it should be very important to have this framework well defined.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We added Refs. 12-14 to include the information on other Kerr Microscope setups for thin films of iron garnet, Pt/Co, and CoFeB.</p>
                <p> </p>
                <p> 3. Also in the introduction, it is not clear for me what the authors mean with the sentence saying that the stage can be moved several tens of nanometers. Is this indicating the precision of the movement using the 3D printed stage actuators, or is the total displacement possible per axis? If it is the first case, then there is a clear problem as tens of nanometers is a very limited movement range for an optical microscope. Clarify.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>The tens of nanometers indicated the precision of the movement. The movement range is a few millimeters. Now we wrote, Furthermore, it has been reported that the sample stage can be moved with the precision of several tens of nanometers.</p>
                <p> </p>
                <p> 4. Also in the introduction section, what is the meaning of depth resolution at the end of the first paragraph? Is that the depth of focus or the precision of the Z stage? If it is the first, then this strongly depends on the objective used and it is usually in the range of ~1 um.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply:</bold> We would like to thank the referee for pointing this out. We removed &#x201c;depth resolution&#x201d; in the introduction to avoid confusion since the depth resolution is beyond our interest in the present study.&#x00a0;</p>
                <p> </p>
                <p> 5. In the second paragraph of the introduction, the application of the method to be discussed is focused towards a very specific material (NiCo2O4). If this work is devoted to present a general purpose and cheap Kerr Microscope, a wider discussion about systems where it could be used as a useful characterization tool should be cited and discussed briefly.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We added Refs. 12-14 to include the information on more general setups for observing magnetic domains of iron garnet, all-optical magnetization switching, and the creation of magnetic skyrmions.</p>
                <p> </p>
                <p> 6. In the Hardware design section, a more thorough description of the polarization optics should be done as it is the key for a proper functioning of a Kerr Microscope. It would be great if comparison with in-plane magnetization sensitive microscopes would be done, as there are plenty of systems where in-plane magnetization is the main actor.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We chose 
                    <ext-link ext-link-type="uri" xlink:href="https://www.thorlabs.co.jp/thorproduct.cfm?partnumber=LPVISE2X2">THORLABS LPVISE2X2</ext-link> with an extinction ratio of 100:1 or more in the visible light range. We also tried 
                    <ext-link ext-link-type="uri" xlink:href="https://www.edmundoptics.jp/p/85-x-5-linear-polarizing-film/46702/">EDMUNDS 8.5" x 5" Linear Polarizing Film</ext-link> but did not succeed due to the lower polarization efficiency of 88%. We agree that there are a number of materials exhibiting in-plane magnetization. However, observations of magnetic domains of in-plane magnetism are beyond the scope of the present study, although this is indeed an interesting research direction in the future.</p>
                <p> </p>
                <p> 7. As a comment, in figure 1 caption, maybe it is not necessary to include the citation for the OpenFlexure Project as it is already in the main text. The caption should focus on the figure itself.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We agree that the caption should explain a figure itself. We therefore replaced the detailed information of the original literature and &#x201c;The Openflexture Project&#x201d; with Ref. 5. in the figure caption.</p>
                <p> </p>
                <p> 8. There is a typo in the description in the main text of Figure 1(a): &#x201c;by a red rectangular&#x201d; should be &#x201c;by a red rectangle&#x201d;.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We would like to thank the referee for pointing this out. We accordingly changed this part from &#x201c;by a red rectangular&#x201d; to &#x201c;by a red rectangle.&#x201d;</p>
                <p> </p>
                <p> 9. The maximum rotation of the analyser should be indicated in the description of panel b of figure 1 as this is important for the tuning of the microscope. Could it be possible to include a retarder waveplate in the design in addition to the analyser too as it exists in other KM for signal optimization? A comment about this would be helpful as this would indicate that the authors have reviewed current Kerr Microscope setups in detail.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>To be confirmed, the analyzer, which we call the polarizer 2 in the text, is not rotatable in the first place. We have added the following sentence in the caption for panel b of Figure 1: &#x201c;Note that the angle of the rod for the polarizer 1 shown in panel b can vary from -75 to 75 degrees in the microscope.&#x201d;</p>
                <p> </p>
                <p> 10. We find the discussion about the electromagnet design very obscure. As it is a very important part of the microscope, it should be described with more detail indicating core material, remanent field, possible heating problems such as 3D printed plastic deformation? Also, stability of the microscope while utilization with the magnetic field on. Interference of the magnetic field with magnetic parts of the objective?</p>
                <p> Just a minor comment, probably, the price of the power supply for the electromagnet should be included in the total price of the microscope.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>
                </p>
                <p> We included the information on the core material (iron) in Table 1. The relationship between the magnetic field (mT) and the current (A) is shown below, indicating no remnant field. So far, we have not observed any plastic deformations of the 3D printed objects due to thermal heating of the coil.</p>
                <p> </p>
                <p> 
                    <ext-link ext-link-type="uri" xlink:href="https://f1000research.s3.amazonaws.com/linked/654324.Figure_R1.pdf">Figure R1: Current evolution of the magnetic field of the coil we employed in the present study.</ext-link>
                </p>
                <p> (Please find the updated figure file in above hyperlink Figure R1)</p>
                <p> </p>
                <p> We included the information on the power supply as</p>
                <p> &#x201c;DC power supply 6,000&#x00a0;&#x00a0;&#x00a0;&#x00a0;&#x00a0; 
                    <ext-link ext-link-type="uri" xlink:href="https://www.amazon.co.jp/dp/B0923KKYTG">Kungber stabilized power supply</ext-link>&#x00a0;&#x00a0;&#x00a0;&#x00a0;&#x00a0; 0-30V, 0-5A&#x201d;</p>
                <p> in Table 1. The total cost was changed from 20000 to 30000 yen.</p>
                <p> </p>
                <p> 11. First of all, why the authors binarize the data for its processing? The intensity of the signal recorded by the camera if it works in a linear manner is very important and can give useful information about the orientation of the magnetization within the system (vector sensitivity inherent to the MO effect). Here it is important also to indicate the dynamic range of the camera used as well as its relation with the smallest signal that the microscope can measure. A thorough discussion about this is mandatory as this work is describing a characterization technique.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>
                </p>
                <p> For the following reasons, analyses by binarization are well justified.</p>
                <p> (a) This thin film has high perpendicular magnetic anisotropy, so the magnetic domains of up and downward spins are distinct.</p>
                <p> (b) The width of the domain wall is much smaller than the spatial resolution of the optical microscope.</p>
                <p> </p>
                <p> Figure R2 shows the effect of binarization available with Zenodo of Ref.14. This operation makes the up and down magnetic domains created by strong perpendicular magnetic anisotropy more clearly visible. Domain walls are too small to be observed.</p>
                <p> </p>
                <p> 
                    <ext-link ext-link-type="uri" xlink:href="https://f1000research.s3.amazonaws.com/linked/654325.Figure_R2.pdf">Figure R2</ext-link>: (Left) Original data of magnetic domains in the MO sensor collected with 
                    <italic>B</italic> = -1.1 mT (Ref. 11). (Right) Binalized data, a part of which is shown in panel 2 of Figure 3 in the main text. Note that the black/white is inverted compared with the left figure for clarity.</p>
                <p> ((Please find the updated figure file in above hyperlink 
                    <ext-link ext-link-type="uri" xlink:href="https://f1000research.s3.amazonaws.com/linked/654325.Figure_R2.pdf">Figure R2</ext-link>)</p>
                <p> </p>
                <p> 12. Another important point here is the fact that the sample used for demonstrating the proof of concept does not really use the Kerr effect, but the Faraday effect which gives a huge signal when compared with polar Kerr for instance. The rotation indicated in figure 3 by the manufacturer of the sensor indicates a rotation of +/-8 degrees between saturations. This is very easy to measure and is adequate for an initial demonstration, but real samples measured using Kerr configuration will most probably show way smaller rotations of the polarization. In this regard, how are the low extinction ratio polarizers going to work? At this point we think that in order to demonstrate real capabilities of the proposed microscope, a real sample where Kerr effect is used for its characterization is mandatory, as is in this configuration where the microscope should work.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>
                </p>
                <p> The right side of Figure 3 is the Faraday effect (obtained by transmission) provided by the company Matesy GmbH to obtain the reference M-H curve. We are conducting microscopy measurements on this sample by using the reflective Kerr effect and have already observed magnetic domain images using this MO sensor as a real sample. Measurements on other samples are currently underway, and we would like to report on them in future publications.</p>
                <p> </p>
                <p> 13. Finally, two comments about figure 3. The external field units of the two loops (half-loops) presented should be the same, and the normalization protocol used for removing background and getting magnetic signal should be better clarified. As it is now, I understand that image 1 (-3.8 mT) is the one used for normalization, which shows stripes. If this is the image taken for normalization, why aren&#x2019;t these stripes present always in all the images? A fully flat image should be taken to work as reference and then the microscope would be working in differential mode. Have the authors observed strong Faraday effects due to the objective optics in combination with the external field from the electromagnet? Please clarify this point.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>
                </p>
                <p> We apologize that the original statement was different from our analysis procedure and thereby misleading. We used the darkest image without stripes collected at -7.6 mT&#x00a0; (not shown)&#x00a0; as a background. This is certainly why these stripes are not present in normalized images. To make this point clearer, we wrote, &#x201c;the darkest image at -7.6 mT is used as a representing background signal.&#x201d;</p>
                <p> We changed the external field unit of the right loop from kAm-1 to mT by using the relationship of 1 mT = 0.7958 kAm-1.</p>
                <p> We confirmed that there are no Faraday effects of the objective lens. By considering the Verdet constant, this is much below 0.1 deg, much smaller than the Kerr rotation of the thin film.</p>
            </body>
        </sub-article>
    </sub-article>
    <sub-article article-type="reviewer-report" id="report189385">
        <front-stub>
            <article-id pub-id-type="doi">10.5256/f1000research.146271.r189385</article-id>
            <title-group>
                <article-title>Reviewer response for version 1</article-title>
            </title-group>
            <contrib-group>
                <contrib contrib-type="author">
                    <name>
                        <surname>Matsui</surname>
                        <given-names>Tatsunosuke</given-names>
                    </name>
                    <xref ref-type="aff" rid="r189385a1">1</xref>
                    <role>Referee</role>
                    <uri content-type="orcid">https://orcid.org/0000-0003-2179-9432</uri>
                </contrib>
                <aff id="r189385a1">
                    <label>1</label>Department of Electrical and Electronic Engineering, Mie University, Tsu, Mie Prefecture, Japan</aff>
            </contrib-group>
            <author-notes>
                <fn fn-type="conflict">
                    <p>
                        <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                </fn>
            </author-notes>
            <pub-date pub-type="epub">
                <day>18</day>
                <month>8</month>
                <year>2023</year>
            </pub-date>
            <permissions>
                <copyright-statement>Copyright: &#x00a9; 2023 Matsui T</copyright-statement>
                <copyright-year>2023</copyright-year>
                <license xlink:href="https://creativecommons.org/licenses/by/4.0/">
                    <license-p>This is an open access peer review report distributed under the terms of the Creative Commons Attribution Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
                </license>
            </permissions>
            <related-article ext-link-type="doi" id="relatedArticleReport189385" related-article-type="peer-reviewed-article" xlink:href="10.12688/f1000research.133292.1"/>
            <custom-meta-group>
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                    <meta-value>approve</meta-value>
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            </custom-meta-group>
        </front-stub>
        <body>
            <p>This manuscript shows development of an open-source, low-cost and compact 3D printed microscope for the observation of magnetic domains in magnetic materials by the magneto-optical Kerr effect (MOKE). Developments of such open-source and low-cost microscope are actively studied in recent years
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-1">1</xref>
                </sup>. A lot of design files are freely available and the authors of the current manuscript utilized one of these 3D printable design developed by the OpenFlexure Project&#x00a0;
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-2">2</xref>
                </sup>. In MOKE observation, polarizers have to be introduced to detect rotation of the polarization of the linearly polarized light reflected from a magnetic material under applied magnetic field. Therefore, they redesigned several components of the OpenFlexure microscope to attach electromagnet and polarizers, and they also made the data for the reproduction of them freely available. They also showed experimental results of the MOKE observation using commercially available magneto-optical (MO) sensor as a sample, which is sufficient to guaranty feasibility of their system.</p>
            <p> </p>
            <p> The OpenFlexure microscope families are superior for their extremely high positioning precision with tens of nanometers based on flexure mechanism of the flexible plastics and low-cost stepper motors&#x00a0;
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-3">3</xref>
                </sup>. Several groups have made contribution to the improvement of such OpenFlexure microscope for advanced scientific applications such as, the optical projection tomography (OPT)
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-4">4</xref>
                </sup>, computational super-resolution imaging system based on the super-resolution radial fluctuation (SRRF) algorism
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-5">5</xref>
                </sup>, and so on. The studies presented in the current manuscript successfully added new function to the OpenFlexure microscope, which may be useful for the researchers working in the field of materials science, especially in magnetic materials.</p>
            <p> </p>
            <p> We are also one of such contributor and reported about a low-cost fabrication of the structured illumination microscope (SIM) for the optical sectioning based on the OpenFlexure stages
                <sup>
                    <xref ref-type="bibr" rid="rep-ref-189385-6">6</xref>
                </sup>. I am confident that we are familiar with the basic working principle of the OpenFlexure microscope and are experienced in building 3D-printable microscopes, but I have poor experience on magnetic measurements. I can say that the authors present appropriate procedures for the reproduction of their work, but I think it will be more informative and helpful if they can provide detailed information about polarizer holder. The polarizers are key components in the MOKE observation and have to be rotated depending on the direction of axes of the magnetic material. The authors simply describe that the polarizers can be rotated in the current manuscript, but do not give detailed explanation how it can be done. My other concern is about uniformity of the LED illumination and the applied magnetic field in the field of view. I think it will be better if the authors can provide descriptions on these points.</p>
            <p>Is the work clearly and accurately presented and does it cite the current literature?</p>
            <p>Yes</p>
            <p>If applicable, is the statistical analysis and its interpretation appropriate?</p>
            <p>I cannot comment. A qualified statistician is required.</p>
            <p>Are all the source data underlying the results available to ensure full reproducibility?</p>
            <p>Yes</p>
            <p>Is the study design appropriate and is the work technically sound?</p>
            <p>Yes</p>
            <p>Are the conclusions drawn adequately supported by the results?</p>
            <p>Yes</p>
            <p>Are sufficient details of methods and analysis provided to allow replication by others?</p>
            <p>Yes</p>
            <p>Reviewer Expertise:</p>
            <p>My expertise is in development of novel optical materials and devices based on organic functional materials such as pi-conjugated materials and liquid crystals. I am also working on metamaterials, plasmonics, photonic crystals, terahertz spectroscopy, and optics in general.</p>
            <p>I confirm that I have read this submission and believe that I have an appropriate level of expertise to confirm that it is of an acceptable scientific standard.</p>
        </body>
        <back>
            <ref-list>
                <title>References</title>
                <ref id="rep-ref-189385-1">
                    <label>1</label>
                    <mixed-citation publication-type="journal">
                        <person-group person-group-type="author"/>:
                        <article-title>The Field Guide to 3D Printing in Optical Microscopy for Life Sciences.</article-title>
                        <source>
                            <italic>Adv Biol (Weinh)</italic>
                        </source>.<year>2022</year>;<volume>6</volume>(<issue>4</issue>) :
                        <elocation-id>10.1002/adbi.202100994</elocation-id>
                        <fpage>e2100994</fpage>
                        <pub-id pub-id-type="pmid">34693666</pub-id>
                        <pub-id pub-id-type="doi">10.1002/adbi.202100994</pub-id>
                    </mixed-citation>
                </ref>
                <ref id="rep-ref-189385-2">
                    <label>2</label>
                    <mixed-citation>
                        <article-title>The OpenFlexure Project</article-title>.
                        <ext-link ext-link-type="uri" xlink:href="https://openflexure.org/">Reference source</ext-link>
                    </mixed-citation>
                </ref>
                <ref id="rep-ref-189385-3">
                    <label>3</label>
                    <mixed-citation publication-type="journal">
                        <person-group person-group-type="author"/>:
                        <article-title>A one-piece 3D printed flexure translation stage for open-source microscopy.</article-title>
                        <source>
                            <italic>Rev Sci Instrum</italic>
                        </source>.<year>2016</year>;<volume>87</volume>(<issue>2</issue>) :
                        <elocation-id>10.1063/1.4941068</elocation-id>
                        <fpage>025104</fpage>
                        <pub-id pub-id-type="pmid">26931888</pub-id>
                        <pub-id pub-id-type="doi">10.1063/1.4941068</pub-id>
                    </mixed-citation>
                </ref>
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                    <mixed-citation publication-type="journal">
                        <person-group person-group-type="author"/>:
                        <article-title>OptiJ: Open-source optical projection tomography of large organ samples.</article-title>
                        <source>
                            <italic>Sci Rep</italic>
                        </source>.<year>2019</year>;<volume>9</volume>(<issue>1</issue>) :
                        <elocation-id>10.1038/s41598-019-52065-0</elocation-id>
                        <fpage>15693</fpage>
                        <pub-id pub-id-type="pmid">31666606</pub-id>
                        <pub-id pub-id-type="doi">10.1038/s41598-019-52065-0</pub-id>
                    </mixed-citation>
                </ref>
                <ref id="rep-ref-189385-5">
                    <label>5</label>
                    <mixed-citation publication-type="journal">
                        <person-group person-group-type="author"/>:
                        <article-title>Adapting the 3D-printed Openflexure microscope enables computational super-resolution imaging.</article-title>
                        <source>
                            <italic>F1000Res</italic>
                        </source>.<year>2019</year>;<volume>8</volume>:
                        <elocation-id>10.12688/f1000research.21294.1</elocation-id>
                        <fpage>2003</fpage>
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                    </mixed-citation>
                </ref>
                <ref id="rep-ref-189385-6">
                    <label>6</label>
                    <mixed-citation publication-type="journal">
                        <person-group person-group-type="author"/>:
                        <article-title>Optical sectioning robotic microscopy for everyone: the structured illumination microscope with the OpenFlexure stages.</article-title>
                        <source>
                            <italic>Opt Express</italic>
                        </source>.<year>2022</year>;<volume>30</volume>(<issue>13</issue>) :
                        <elocation-id>10.1364/OE.461910</elocation-id>
                        <fpage>23208</fpage>-<lpage>23216</lpage>
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                    </mixed-citation>
                </ref>
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        </back>
        <sub-article article-type="response" id="comment10787-189385">
            <front-stub>
                <contrib-group>
                    <contrib contrib-type="author">
                        <name>
                            <surname>Wadati</surname>
                            <given-names>Hiroki</given-names>
                        </name>
                        <aff>University of Hyogo, Japan</aff>
                    </contrib>
                </contrib-group>
                <author-notes>
                    <fn fn-type="conflict">
                        <p>
                            <bold>Competing interests: </bold>No competing interests were disclosed.</p>
                    </fn>
                </author-notes>
                <pub-date pub-type="epub">
                    <day>19</day>
                    <month>12</month>
                    <year>2023</year>
                </pub-date>
            </front-stub>
            <body>
                <p>1. This manuscript shows development of an open-source, low-cost and compact 3D printed microscope for the observation of magnetic domains in magnetic materials by the magneto-optical Kerr effect (MOKE). Developments of such open-source and low-cost microscope are actively studied in recent years
                    <sup>1</sup>. A lot of design files are freely available and the authors of the current manuscript utilized one of these 3D printable design developed by the OpenFlexure Project 
                    <sup>2</sup>. In MOKE observation, polarizers have to be introduced to detect rotation of the polarization of the linearly polarized light reflected from a magnetic material under applied magnetic field. Therefore, they redesigned several components of the OpenFlexure microscope to attach electromagnet and polarizers, and they also made the data for the reproduction of them freely available. They also showed experimental results of the MOKE observation using commercially available magneto-optical (MO) sensor as a sample, which is sufficient to guaranty feasibility of their system.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We thank the reviewer for his careful reading of our manuscript and for considering our work worthy of publication. In the following, we answer his concerns one by one, and we point out the changes made in the manuscript to improve both the discussion and the figures following his suggestions.</p>
                <p> </p>
                <p> 2. The OpenFlexure microscope families are superior for their extremely high positioning precision with tens of nanometers based on flexure mechanism of the flexible plastics and low-cost stepper motors
                    <sup>3</sup>. Several groups have made contribution to the improvement of such OpenFlexure microscope for advanced scientific applications such as, the optical projection tomography (OPT)
                    <sup>4</sup>, computational super-resolution imaging system based on the super-resolution radial fluctuation (SRRF) algorism
                    <sup>5</sup>, and so on. The studies presented in the current manuscript successfully added new function to the OpenFlexure microscope, which may be useful for the researchers working in the field of materials science, especially in magnetic materials.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>Thank you for highlighting the novelty of our present work in comparison with recent studies relevant to our study. Note that we found that Ref. 4 in the original manuscript was not properly cited and thus revised as follows: Opt. Express. 2022; 30 (13): 23208-23216.</p>
                <p> </p>
                <p> 3. We are also one of such contributor and reported about a low-cost fabrication of the structured illumination microscope (SIM) for the optical sectioning based on the OpenFlexure stages6. I am confident that we are familiar with the basic working principle of the OpenFlexure microscope and are experienced in building 3D-printable microscopes, but I have poor experience on magnetic measurements. I can say that the authors present appropriate procedures for the reproduction of their work, but I think it will be more informative and helpful if they can provide detailed information about polarizer holder. The polarizers are key components in the MOKE observation and have to be rotated depending on the direction of axes of the magnetic material. The authors simply describe that the polarizers can be rotated in the current manuscript, but do not give detailed explanation how it can be done.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>We totally agree that detailed information about the polarizer holder would be helpful for readers. To better understand our system, we have added the following sentence in the section on Hardware design: &#x201c;The rod can be mechanically rotated by hand. The angle of the holder can vary from -75 to 75 degrees in the current setup.&#x201d;</p>
                <p> </p>
                <p> 4. My other concern is about uniformity of the LED illumination and the applied magnetic field in the field of view. I think it will be better if the authors can provide descriptions on these points.</p>
                <p> </p>
                <p> 
                    <bold>Our Reply: </bold>&#x00a0;</p>
                <p> To clarify the uniformity of the LED illumination, we rewrote the sentence as</p>
                <p> &#x201c;This microscope employs the K&#x00f6;hler illumination method, where the illuminated light becomes collimated on the sample surface by using the three lenses. This ensures the uniformity of the LED illumination.&#x201d;</p>
                <p> The in-plane component of the magnetic field was 0.1 mT or less, measured by a Tesla meter. Small non-uniformity causes no problem due to the observed small area (~0.5 &#x00d7; 0.5 mm). Moreover, the coercive field estimated from our Kerr intensity in response to the magnetic field is nearly identical to the Faraday rotation data provided by Matesy GmbH (Fig. 3), implying that the magnetic field is essentially homogeneous in our apparatus.</p>
            </body>
        </sub-article>
    </sub-article>
</article>
