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<ri:Resource created="2022-02-23T10:03:53Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>NIR obs. of the Gal. magnetar SGR 1935+215 with PGIR</title><shortName>J/ApJ/901/L7</shortName><identifier>ivo://CDS.VizieR/J/ApJ/901/L7</identifier><altIdentifier>doi:10.26093/cds/vizier.19019007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De K.</name></creator><creator><name>Ashley M.C.B.</name></creator><creator><name>Andreoni I.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Soria R.,Srinivasaragavan G.P.</name></creator><creator><name>Cai Ce</name></creator><creator><name>Delacroix A.</name></creator><creator><name>Greffe T.</name></creator><creator><name>Hale D.,Hankins M.J.</name></creator><creator><name>Li C.</name></creator><creator><name>McKenna D.</name></creator><creator><name>Moore A.M.</name></creator><creator><name>Ofek E.O.</name></creator><creator><name>Smith R.M.</name></creator><creator><name>Soon J.,Travouillon T.</name></creator><creator><name>Zhang S.</name></creator><date role="Updated">2022-08-25T11:44:19Z</date><date role="Created">2022-02-23T10:03:53Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>pulsars</subject><subject>infrared-photometry</subject><description>The Galactic magnetar SGR 1935+2154 has been reported to produce the first example of a bright millisecond-duration radio burst (FRB200428) similar to the cosmological population of fast radio bursts (FRBs). The detection of a coincident bright X-ray burst represents the first observed multiwavelength counterpart of an FRB. However, the search for similar emission at optical wavelengths has been hampered by the high inferred extinction on the line of sight. Here, we present results from the first search for second-timescale emission from the source at near-infrared (NIR) wavelengths using the Palomar Gattini-IR observing system in the J band, enabled by a novel detector readout mode that allows short exposure times of ~0.84s with 99.9% observing efficiency. With a total observing time of ~12hr (~47728 images) during its 2020 outburst, we place median 3{sigma} limits on the second-timescale NIR fluence of &lt;~18Jy.ms (13.1 AB mag). The corresponding extinction-corrected limit is &lt;~125Jy.ms for an estimated extinction of A_J_=2.0mag. Our observations were sensitive enough to easily detect an NIR counterpart of FRB 200428 if the NIR emission falls on the same power law as observed across its radio to X-ray spectrum. We report nondetection limits from epochs of four simultaneous X-ray bursts detected by the Insight-HXMT and NuSTAR telescopes during our observations. These limits provide the most stringent constraints to date on fluence of flares at ~10^14^Hz, and constrain the fluence ratio of the NIR emission to coincident X-ray bursts to R_NIR_&lt;~0.025 (fluence index &gt;~0.35).</description><source format="bibcode">2020ApJ...901L...7D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/901/L7</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/6">J/ApJS/212/6 : The McGill magnetar catalog (Olausen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/11">J/ApJS/218/11 : 5yr Fermi/GBM magnetar burst catalog (Collazzi+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/33.45">J/other/PASA/33.45 : FRBCAT: Fast Radio Burst (FRB) Catalog (Petroff+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/232/17">J/ApJS/232/17 : Spectral data of magnetar bursts (Kirmizibayrak+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/469/2313">J/MNRAS/469/2313 : Radio pulsars post-glitchs (Gugercinoglu, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/896/L2">J/ApJ/896/L2 : ZTF obs. of FRB 180916.J0158+65 (Andreoni+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/901/L7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/901/L7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/901/L7</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/901/L7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/901/L7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/901/L7</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/901/L7/fig2</name><description>Measured standard deviation in fluxes</description><column><name>JD</name><description>Julian date converted from UT date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Obs</name><description>Year of the observation start; UTC</description><ucd>time.epoch</ucd><flag>indexed</flag></column><column><name>Exp</name><description>[0.84/1.65] Exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fluence</name><description>[-6.1e-10/3.1e-10] Measured fluence in erg/cm^2^ units</description><unit>mJ.m**-2</unit><ucd>phot.fluence;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Fluence</name><description>[3.3e-11/2.3e-10] The 3{sigma} limit on Fluence</description><unit>mJ.m**-2</unit><ucd>stat.error;phot.fluence</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>