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<ri:Resource created="2023-11-17T06:59:32Z" status="active" updated="2025-06-13T15:25:00Z" 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>Absolute Calibration. III. Sirius &amp; Sun IR spectra</title><shortName>J/AJ/165/99</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/99</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rieke G.H.</name></creator><creator><name>Engelke C.</name></creator><creator><name>Su K.</name></creator><creator><name>Casagrande L.</name></creator><date role="Updated">2023-12-20T08:42:40Z</date><date role="Created">2023-11-17T06:59:32Z</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>the-sun</subject><subject>standard-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>We propose Sirius as an improved zero-point-defining star and calibrate its spectrum to an accuracy of ~0.6% in both the visible and infrared. This result is based on a newly derived independent calibration in the visible of similar accuracy to the previous standard one, with which it is combined. We use a large variety of approaches in the infrared to reach about three times smaller error than for previous absolute calibrations. The results in the two wavelength regimes are in agreement, providing a consistent link from the visible throughout the near- and mid-infrared. The Sirius-based zero-point at 5557.5{AA} (in vacuum) is 13.436{+/-}0.081x10^-12^W/cm^2^/{mu}m, based on the improved value for Vega of 3.473{+/-}0.018x10^-12^W/cm^2^/{mu}m and the measured magnitude difference between the two stars. At 2.1603{mu}m, the zero-point is 4.225{+/-}0.025x10^-14^W/cm^2^/{mu}m taking Sirius at a magnitude of -1.395. A jackknife analysis indicates that there are no serious systematic errors in these results. We consider selection of secondary standards that can extend the calibration over the sky. Despite more than a century in this role, normal A-stars are not suitable, although Am and Ap stars may be. G-stars older than ~1Gyr are good candidates if accurate temperatures can be measured. White dwarfs are suitable from the visible through the near-infrared, but their properties are unexplored at the necessary level at the longer infrared wavelengths, and for most facilities they are too faint there. Finally, as a further test of the calibration, we demonstrate an upgraded infrared flux method to determine accurate stellar diameters from K-band photometry.</description><source format="bibcode">2023AJ....165...99R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/99</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/II/5">II/5 : UBV Photometry of Bright Stars (Johnson+ 1966)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/135">J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/110/275">J/AJ/110/275 : IR spectra of standard stars (Cohen+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/2274">J/AJ/112/2274 : Spectral irradiance calibration. 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