<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Article on Natanael.net</title><link>https://natanael.net/pubtype/article/</link><description>Recent content in Article on Natanael.net</description><generator>Hugo</generator><language>en</language><lastBuildDate>Mon, 06 Jul 2026 00:00:00 +0000</lastBuildDate><atom:link href="https://natanael.net/pubtype/article/index.xml" rel="self" type="application/rss+xml"/><item><title>The S-PLUS Fifth Data-Release: Over 4500 square degrees of the Southern Sky and a multicolor view of the Hydra and Antlia galaxy clusters</title><link>https://natanael.net/publications/2026/lima/</link><pubDate>Mon, 06 Jul 2026 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2026/lima/</guid><description/></item><item><title>S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known systems in DR5 and a pilot study of Abell 4038</title><link>https://natanael.net/publications/2026/mendes-de-oliveira/</link><pubDate>Mon, 29 Jun 2026 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2026/mendes-de-oliveira/</guid><description>&lt;h2 id="table-1" class="group scroll-mt-24"&gt;&#10; Table 1&#10; &lt;a&#10; class="ms-2 align-middle text-[0.6em] text-ink-faint no-underline opacity-0 transition-opacity group-hover:opacity-100 focus:opacity-100"&#10; href="#table-1"&#10; aria-label="Link to this section"&gt;#&lt;/a&gt;&#10;&lt;/h2&gt;&#10;&lt;p&gt;A digital version of Table 1 from the published article is provided to facilitate data analysis. Table 1 presents a summary of the 83 SCALE systems, with each row corresponding to an individual cluster and reporting aggregated cluster properties. The table includes the principal quantities derived in this work, such as &lt;/p&gt;&#10;$$R_{200}$$&lt;p&gt;, &lt;/p&gt;&#10;$$M_{200}$$&lt;p&gt;, and &lt;/p&gt;</description></item><item><title>AstroInspect: a web-based system to organize, assess, and visually inspect astronomical objects</title><link>https://natanael.net/publications/2026/cardoso/</link><pubDate>Tue, 14 Apr 2026 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2026/cardoso/</guid><description>&lt;p&gt;&lt;figure class="m-card m-figure "&gt;&lt;img&#10; src="https://natanael.net/publications/2026/cardoso/astroinspect_ui_hu_d712d2a5b2470d84.webp"&#10; srcset="https://natanael.net/publications/2026/cardoso/astroinspect_ui_hu_2741bb5835d371c1.webp 600w, https://natanael.net/publications/2026/cardoso/astroinspect_ui_hu_331f44680abb1c10.webp 1000w, https://natanael.net/publications/2026/cardoso/astroinspect_ui_hu_d712d2a5b2470d84.webp 1600w"&#10; sizes="(min-width: 720px) 720px, 100vw"&#10; width="1600"&#10; height="1041"&#10; alt=""&#10; loading="lazy"&#10; decoding="async"&gt;&#10;&lt;/figure&gt;&#10;&lt;/p&gt;&#10;&lt;h2 id="table-1" class="group scroll-mt-24"&gt;&#10; Table 1&#10; &lt;a&#10; class="ms-2 align-middle text-[0.6em] text-ink-faint no-underline opacity-0 transition-opacity group-hover:opacity-100 focus:opacity-100"&#10; href="#table-1"&#10; aria-label="Link to this section"&gt;#&lt;/a&gt;&#10;&lt;/h2&gt;&#10;&lt;p&gt;The Table 1 of the AstroInspect paper contains all H&lt;/p&gt;&#10;$$\alpha$$&lt;p&gt; emission-line galaxies within 5&lt;/p&gt;&#10;$$R_{200}$$&lt;p&gt; (&lt;/p&gt;&#10;$$\approx 7$$&lt;p&gt; deg) of the Hydra I cluster (also known as Abell 1060)&lt;sup id="fnref:1"&gt;&lt;a href="#fn:1" class="footnote-ref" role="doc-noteref"&gt;1&lt;/a&gt;&lt;/sup&gt; found by visual inspection using AstroInspect.&lt;/p&gt;&#10;&lt;h3 id="columns-description" class="group scroll-mt-24"&gt;&#10; Columns description&#10; &lt;a&#10; class="ms-2 align-middle text-[0.6em] text-ink-faint no-underline opacity-0 transition-opacity group-hover:opacity-100 focus:opacity-100"&#10; href="#columns-description"&#10; aria-label="Link to this section"&gt;#&lt;/a&gt;&#10;&lt;/h3&gt;&#10;&lt;table&gt;&#10; &lt;thead&gt;&#10; &lt;tr&gt;&#10; &lt;th&gt;#&lt;/th&gt;&#10; &lt;th&gt;Unit&lt;/th&gt;&#10; &lt;th&gt;Column name&lt;/th&gt;&#10; &lt;th&gt;Description&lt;/th&gt;&#10; &lt;/tr&gt;&#10; &lt;/thead&gt;&#10; &lt;tbody&gt;&#10; &lt;tr&gt;&lt;td&gt;1&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;id&lt;/td&gt;&lt;td&gt;Catalog unique identifier&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;2&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;ra&lt;/td&gt;&lt;td&gt;Right Ascension in decimal degrees (J2000)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;3&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;dec&lt;/td&gt;&lt;td&gt;Declination in decimal degrees (J2000)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;4&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_u&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the u band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;5&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_g&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the g band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;6&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_r&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the r band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;7&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_i&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the i band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;8&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_z&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the z band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;9&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F378&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F378 band (Balmer jump / [O\(_{\rm II}\)])&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;10&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F395&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F395 band (Ca H + K)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;11&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F410&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F410 band (H\(\delta\))&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;12&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F430&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F430 band (G band)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;13&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F515&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F515 band (Mg b triplet)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;14&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F660&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F660 band (H\(\alpha\))&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;15&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;sp_mag_F861&lt;/td&gt;&lt;td&gt;S-PLUS DR5 magnitude in the F861 band (Ca triplet)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;16-27&lt;/td&gt;&#10; &lt;td&gt;mag&lt;/td&gt;&#10; &lt;td&gt;sp_mag_err_&lt;tt&gt;[band]&lt;/tt&gt;&lt;/td&gt;&#10; &lt;td&gt;&#10; S-PLUS DR5 magnitude error, where &lt;tt&gt;[band]&lt;/tt&gt; is one of:&#10; u, g, r, i, z, F378, F395, F410, F430, F515, F660, F861&#10; &lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;28&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_A&lt;/td&gt;&lt;td&gt;S-PLUS DR5 profile RMS along the major axis&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;29&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_B&lt;/td&gt;&lt;td&gt;S-PLUS DR5 profile RMS along the minor axis&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;30&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_PA&lt;/td&gt;&lt;td&gt;S-PLUS DR5 position angle (CCW/World-x)&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;31&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_radius_petro&lt;/td&gt;&lt;td&gt;S-PLUS DR5 Petrosian aperture radius&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;32&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_radius_50&lt;/td&gt;&lt;td&gt;S-PLUS DR5 radius enclosing 50% of the total flux&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;33&lt;/td&gt;&lt;td&gt;deg&lt;/td&gt;&lt;td&gt;sp_radius_90&lt;/td&gt;&lt;td&gt;S-PLUS DR5 radius enclosing 90% of the total flux&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;34&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;sp_photoz&lt;/td&gt;&lt;td&gt;S-PLUS DR5 photometric redshift&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;35&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;sp_photoz_odds&lt;/td&gt;&lt;td&gt;S-PLUS DR5 photometric redshift odds&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;36&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;ls_mag_g&lt;/td&gt;&lt;td&gt;LS DR10 magnitude in the g band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;37&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;ls_mag_r&lt;/td&gt;&lt;td&gt;LS DR10 magnitude in the r band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;38&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;ls_mag_i&lt;/td&gt;&lt;td&gt;LS DR10 magnitude in the i band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;39&lt;/td&gt;&lt;td&gt;mag&lt;/td&gt;&lt;td&gt;ls_mag_z&lt;/td&gt;&lt;td&gt;LS DR10 magnitude in the z band&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;40&lt;/td&gt;&#10; &lt;td&gt;&lt;/td&gt;&#10; &lt;td&gt;ls_type&lt;/td&gt;&#10; &lt;td&gt;&#10; LS DR10 morphological type (for details, see&#10; &lt;a href="https://www.legacysurvey.org/dr10/description"&gt;&#10; https://www.legacysurvey.org/dr10/description&#10; &lt;/a&gt;)&#10; &lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;41&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;lit_redshift&lt;/td&gt;&lt;td&gt;Spectroscopic redshift&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;42&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;lit_redshift_err&lt;/td&gt;&lt;td&gt;Spectroscopic redshift error&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;43&lt;/td&gt;&lt;td&gt;&lt;/td&gt;&lt;td&gt;lit_source&lt;/td&gt;&lt;td&gt;Spectroscopic redshift source from literature&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;44&lt;/td&gt;&lt;td&gt;km/s&lt;/td&gt;&lt;td&gt;velocity&lt;/td&gt;&lt;td&gt;Velocity derived from spectroscopic redshift&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&lt;td&gt;45&lt;/td&gt;&lt;td&gt;km/s&lt;/td&gt;&lt;td&gt;velocity_err&lt;/td&gt;&lt;td&gt;Velocity error&lt;/td&gt;&lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;46&lt;/td&gt;&#10; &lt;td&gt;km/s&lt;/td&gt;&#10; &lt;td&gt;velocity_offset&lt;/td&gt;&#10; &lt;td&gt;&#10; Velocity difference between the object and the Hydra I cluster,&#10; available only for objects with known spectroscopic redshift&#10; &lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;47&lt;/td&gt;&#10; &lt;td&gt;deg&lt;/td&gt;&#10; &lt;td&gt;dist_proj&lt;/td&gt;&#10; &lt;td&gt;&#10; Sky-projected angular distance between the object and the Hydra I cluster center&#10; &lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;48&lt;/td&gt;&#10; &lt;td&gt;Mpc&lt;/td&gt;&#10; &lt;td&gt;dist&lt;/td&gt;&#10; &lt;td&gt;&#10; Distance between the object and the Hydra I cluster center,&#10; available only for objects with known spectroscopic redshift&#10; &lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;/tbody&gt;&#10; &lt;caption&gt;Columns prefixed with &lt;tt&gt;sp&lt;/tt&gt; are drawn from S-PLUS DR5 (E. V. Lima et al. 2026, in preparation), while those prefixed with &lt;tt&gt;ls&lt;/tt&gt; originate from Legacy Survey DR10[^legacy]. Columns prefixed with &lt;tt&gt;lit&lt;/tt&gt; originate from redshift compilation from the literature[^erik-redshifts]. Columns without these prefixes were derived in this work. All magnitudes are reported in the AB system, and the S-SPLUS magnitudes included in the catalog are only the auto-aperture values.&lt;/caption&gt;&#10;&lt;/table&gt;&#10;&lt;div class="footnotes" role="doc-endnotes"&gt;&#10;&lt;hr&gt;&#10;&lt;ol&gt;&#10;&lt;li id="fn:1"&gt;&#10;&lt;p&gt;Abell, G. O., Corwin, H. G., Jr., &amp;amp; Olowin, R. P. (1989). A catalog of rich clusters of galaxies. &lt;em&gt;The Astrophysical Journal Supplement Series&lt;/em&gt;, 70, 1. doi:10.1086/191333&amp;#160;&lt;a href="#fnref:1" class="footnote-backref" role="doc-backlink"&gt;&amp;#x21a9;&amp;#xfe0e;&lt;/a&gt;&lt;/p&gt;</description></item><item><title>The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering ∼ 5 virial radii around NGC 1399 with galaxy properties</title><link>https://natanael.net/publications/2026/haack/</link><pubDate>Wed, 08 Apr 2026 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2026/haack/</guid><description/></item><item><title>MAR: A Multiband Astronomical Reduction package</title><link>https://natanael.net/publications/2025/oliveira-schwarz/</link><pubDate>Tue, 01 Apr 2025 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2025/oliveira-schwarz/</guid><description/></item><item><title>The S-PLUS Fornax Project (S+FP): A first 12-band glimpse of the Fornax galaxy cluster</title><link>https://natanael.net/publications/2024/smith-castelli/</link><pubDate>Tue, 23 Apr 2024 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2024/smith-castelli/</guid><description/></item><item><title>Diagnostic diagrams for ram pressure stripped candidates</title><link>https://natanael.net/publications/2024/krabbe/</link><pubDate>Thu, 01 Feb 2024 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2024/krabbe/</guid><description/></item><item><title>Morphological Classification of Galaxies in S-PLUS using an Ensemble of Convolutional Networks</title><link>https://natanael.net/publications/2021/cardoso/</link><pubDate>Wed, 10 Nov 2021 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2021/cardoso/</guid><description>&lt;p&gt;&lt;figure class="m-card m-figure "&gt;&lt;img&#10; src="https://natanael.net/publications/2021/cardoso/nt-splus-morpho_hu_9fe68930d67dcaae.webp"&#10; srcset="https://natanael.net/publications/2021/cardoso/nt-splus-morpho_hu_a8b0facf2d4c6d87.webp 600w, https://natanael.net/publications/2021/cardoso/nt-splus-morpho_hu_9fe68930d67dcaae.webp 1000w"&#10; sizes="(min-width: 720px) 720px, 100vw"&#10; width="1000"&#10; height="265"&#10; alt=""&#10; loading="lazy"&#10; decoding="async"&gt;&#10;&lt;/figure&gt;&#10;&lt;/p&gt;&#10;&lt;h3 id="classifications-of-blind-sample" class="group scroll-mt-24"&gt;&#10; Classifications of blind sample&#10; &lt;a&#10; class="ms-2 align-middle text-[0.6em] text-ink-faint no-underline opacity-0 transition-opacity group-hover:opacity-100 focus:opacity-100"&#10; href="#classifications-of-blind-sample"&#10; aria-label="Link to this section"&gt;#&lt;/a&gt;&#10;&lt;/h3&gt;&#10;&lt;table class="table table-hover"&gt;&#10; &lt;thead&gt;&#10; &lt;tr&gt;&#10; &lt;th&gt;Column&lt;/th&gt;&#10; &lt;th&gt;Description&lt;/th&gt;&#10; &lt;/tr&gt;&#10; &lt;/thead&gt;&#10; &lt;tbody&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;ra&lt;/td&gt;&#10; &lt;td&gt;right ascension in decimal degrees (J2000)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;dec&lt;/td&gt;&#10; &lt;td&gt;declination in decimal degrees (J2000)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;r_auto&lt;/td&gt;&#10; &lt;td&gt;S-PLUS DR1 r-band magnitude (SDSS-like r)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;mn170_pE&lt;/td&gt;&#10; &lt;td&gt;probability of the object being elliptical given by the classification of the trained model with objects with magnitude \(r_{auto} &lt; 17\) (mn stands for "MorphoNet")&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;mn170_pS&lt;/td&gt;&#10; &lt;td&gt;probability of the object being spiral given by the classification of the trained model with objects with magnitude \(r_{auto} &lt; 17\)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;mn175_pE&lt;/td&gt;&#10; &lt;td&gt;probability of the object being elliptical given by the classification of the trained model with objects with magnitude \(r_{auto} &lt; 17.5\)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;tr&gt;&#10; &lt;td&gt;mn175_pS&lt;/td&gt;&#10; &lt;td&gt;probability of the object being spiral given by the classification of the trained model with objects with magnitude \(r_{auto} &lt; 17.5\)&lt;/td&gt;&#10; &lt;/tr&gt;&#10; &lt;/tbody&gt;&#10;&lt;/table&gt;&#10;&lt;p&gt;Downloads:&lt;/p&gt;</description></item><item><title>Deep Learning Assessment of galaxy morphology in S-PLUS Data Release 1</title><link>https://natanael.net/publications/2021/bom/</link><pubDate>Mon, 26 Jul 2021 00:00:00 +0000</pubDate><guid>https://natanael.net/publications/2021/bom/</guid><description>&lt;p&gt;&lt;figure class="m-card m-figure "&gt;&lt;img&#10; src="https://natanael.net/publications/2021/bom/paper-clecio_hu_e892dcd34a2da1bd.webp"&#10; srcset="https://natanael.net/publications/2021/bom/paper-clecio_hu_52261b3470ba4e32.webp 600w, https://natanael.net/publications/2021/bom/paper-clecio_hu_e892dcd34a2da1bd.webp 1000w"&#10; sizes="(min-width: 720px) 720px, 100vw"&#10; width="1000"&#10; height="513"&#10; alt=""&#10; loading="lazy"&#10; decoding="async"&gt;&#10;&lt;/figure&gt;&#10;&lt;/p&gt;&#10;&lt;p&gt;Materials and data related with this paper are available at &lt;a href="http://clearnightsrthebest.com" rel="noopener" data-external&gt;http://clearnightsrthebest.com&lt;/a&gt; and &lt;a href="https://github.com/cdebom/splus_morph" rel="noopener" data-external&gt;https://github.com/cdebom/splus_morph&lt;/a&gt;.&lt;/p&gt;</description></item></channel></rss>