<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2022-11-30T05:49:00Z" status="active" updated="2026-03-04T11:08:16Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/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/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>DECaPS DR2 r survey collection</title><shortName>DECaPS DR2 r</shortName><identifier>ivo://CDS/P/DECaPS/DR2/r</identifier><altIdentifier>10.26093/cds/aladin/35gc-wzp</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Buga M.</name></creator><date role="Created">2022-11-30T05:49:00Z</date><date role="Updated">2022-12-01T10:05:00Z</date><contact><name>CDS Helpdesk</name><email>cds-question@unistra.fr</email></contact></curation><content><subject>Sky survey</subject><subject>Optical astronomy</subject><subject>Milky Way disk</subject><description>DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | %3C 10 deg , 6 deg &gt; l &gt; - 124 deg (essentially the low latitude Galactic plane south of delta %3C - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium.</description><source format="bibcode">2022arXiv220611909S</source><referenceURL>https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r</referenceURL><type>Survey</type><contentLevel>Research</contentLevel></content><rights rightsURI="https://cds.unistra.fr/aladin-org/licences_aladin.html">This HiPS is distributed under ODbL license by Unistra/CNRS</rights><capability standardID="ivo://ivoa.net/std/hips#hips-1.0"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r</accessURL><mirrorURL>https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r</mirrorURL></interface></capability><coverage><temporal>57460 58606</temporal><spectral>2.7704963140152424e-19 3.5158333754848296e-19</spectral><footprint ivo-id="ivo://mocivod">https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r/Moc.fits</footprint><waveband>Optical</waveband></coverage></ri:Resource>