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<ri:Resource created="2025-11-18T13:25:06Z" status="active" updated="2026-08-03T07:32:05Z" 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>JWST NIRCam photometry of M 92 stars</title><shortName>J/MNRAS/517/484</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/517/484</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-g5-f4</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nardiello D.</name></creator><creator><name>Bedin L.R.</name></creator><creator><name>Burgasser A.</name></creator><creator><name>Salaris M.</name></creator><creator><name>Cassisi S.</name></creator><creator><name>Griggio M.,Scalco M.</name></creator><date role="Updated">2026-08-03T07:32:05Z</date><date role="Created">2025-11-18T13:25:06Z</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>globular-star-clusters</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><description>As the James Webb Space Telescope (JWST) has become fully operational, early release data are now available to begin building the tools and calibrations for precision point-source photometry and astrometry in crowded cluster environments. Here, we present our independent reduction of NIRCam imaging of the metal-poor globular cluster M 92, which were collected under Director's Discretionary Early Release Science programme ERS-1334. We derived empirical models of the point spread function (PSF) for filters F090W, F150W, F277W, and F444W, and find that these PSFs: (i) are generally undersampled (FWHM ~ 2 pixel) in F150W and F444W and severely undersampled (FWHM ~ 1 pixel) in F090W and F277W; (ii) have significant variation across the field of view, up to ~15-20 per cent; and (iii) have temporal variations of ~ 3-4 per cent across multi-epoch exposures. We deployed our PSFs to determine the photometric precision of NIRCam for stars in the crowded, central regions of M 92, measured to be at the ~0.01 mag level. We use these data to construct the first JWST colour-magnitude diagrams of a globular cluster. Employing existing stellar models, we find that the data reach almost the bottom of the M 92 main sequence (~0.1 M_{sun}_), and reveal 24 white dwarf candidate members of M 92 in the brightest portion of the white dwarf cooling sequence. The latter are confirmed through a cross-match with archival HST UV and optical data. We also detect the presence of multiple stellar populations along the low-mass main sequence of M 92.</description><source format="bibcode">2022MNRAS.517..484N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/517/484</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/AJ/149/153">J/AJ/149/153 : Abundances of red giants in 10 globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/15">J/ApJ/797/15 : HST/WFC3 observations in 4 metal-poor GCs of Fornax</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1658">J/AJ/133/1658 : ACS survey of galactic globular clusters (Sarajedini+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1780">J/MNRAS/463/1780 : Exoplanet candidates in Praesepe (M 44) (Libralato+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1831">J/MNRAS/463/1831 : M67 Kepler/K2 variable stars (Nardiello+, 2016)</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/MNRAS/517/484</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/517/484</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/517/484</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/517/484</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/517/484</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/517/484</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>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/517/484/f090wa1</name><description>Star sources NIRCam PSF photometry in F090W, SW module A and channel 1 of the detector</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f150wb2</name><description>Star sources NIRCam PSF photometry in F150W, SW module B and channel 2 of the detector</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f150wb3</name><description>Star sources NIRCam PSF photometry in F150W, SW module B and channel 3 of the detector</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f150wb4</name><description>Star sources NIRCam PSF photometry in F150W, SW module B and channel 4 of the detector</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f277wa</name><description>Star sources NIRCam PSF photometry in F277W, LW module A</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f277wb</name><description>Star sources NIRCam PSF photometry in F277W, LW module B</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f444wa</name><description>Star sources NIRCam PSF photometry in F444W, LW module A</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/f444wb</name><description>Star sources NIRCam PSF photometry in F444W, LW module B</description><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>X</name><description>X stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y stellar position in the reference system of the detector</description><unit>pix</unit><ucd>meta.ref.url;pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Xmag</name><description>Calibrated Vega magnitude of NIRCam JWST in filter as the file's names indicate F090W, F150W, F277W and F444W (MAG)</description><unit>mag</unit><ucd>phot.mag;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Xmag</name><description>Photometric error of Xmag (SIGMA_MAG)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qfit</name><description>The quality of a PSF model fit to an individual star where the smaller is the qfit the better the PSF fit is (QFIT)</description><ucd>stat.fit.goodness;instr.det.psf;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/517/484/list</name><description>List of fits images</description><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>Nx</name><description>Number of pixels along X-axis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ny</name><description>Number of pixels along Y-axis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>size</name><description>Size of FITS file</description><unit>Kibyte</unit><ucd>phys.size;meta.fits</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FileName</name><description>Name of FITS file, in subdirectory fits</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Title</name><description>Title of the FITS file</description><ucd>meta.title;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="32*">char</dataType></column></table></schema></tableset></ri:Resource>