allWISE W3ivo://CDS/P/allWISE/W310.26093/cds/aladin/na1n-03CDSBoch T.2014-04-15T09:25:00Z2019-05-20T08:23:00ZCDS Helpdeskcds-question@unistra.frSky surveyInfrared astronomyNear infrared astronomyNASA's Wide-field Infrared Survey Explorer (WISE; Wright et al.2010) mapped the sky at 3.4, 4.6, 12, and 22 um (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the four bands. WISE achieved 5 sigma point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.The All-Sky Release includes all data taken during the WISE full cryogenic mission phase, 7 January 2010 to 6 August 2010, that were processed with improved calibrations and reduction algorithms.Original acknowledgement for data: This Progressive Survey distribution makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, and NEOWISE, which is a project of the Jet Propulsion Laboratory/California Institute of Technology.WISE and NEOWISE are funded by the National Aeronautics and Space Administration.2010AJ....140.1868Whttps://alasky.cds.unistra.fr/AllWISE/W3SurveyResearchIsDerivedFromIPAC/NASAThis HiPS is distributed under ODbL license by Unistra/CNRShttps://alasky.cds.unistra.fr/AllWISE/W3https://alaskybis.cds.unistra.fr/AllWISE/W3https://irsa.ipac.caltech.edu/data/hips/CDS/AllWISE/W355378 554141.1508089524826803e-20 2.6688779486079922e-20https://alasky.cds.unistra.fr/AllWISE/W3/Moc.fitsInfrared