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The CatWISE2020 Catalog

Marocco, Federico and Eisenhardt, Peter R. M. and Fowler, John W. and Kirkpatrick, J. Davy and Meisner, Aaron M. and Schlafly, Edward F. and Stanford, S. A. and Garcia, Nelson and Caselden, Dan and Cushing, Michael C. and Cutri, Roc M. and Faherty, Jacqueline K. and Gelino, Christopher R. and Gonzalez, Anthony H. and Jarrett, Thomas H. and Koontz, Renata and Mainzer, Amanda and Marchese, Elijah J. and Mobasher, Bahram and Schlegel, David J. and Stern, Daniel and Teplitz, Harry I. and Wright, Edward L. (2021) The CatWISE2020 Catalog. Astrophysical Journal Supplement Series, 253 (1). Art. No. 8. ISSN 1538-4365. doi:10.3847/1538-4365/abd805. https://resolver.caltech.edu/CaltechAUTHORS:20210204-092658386

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Abstract

The CatWISE2020 Catalog consists of 1,890,715,640 sources over the entire sky selected from Wide-field Infrared Survey Explorer (WISE) and NEOWISE survey data at 3.4 and 4.6 μm (W1 and W2) collected from 2010 January 7 to 2018 December 13. This data set adds two years to that used for the CatWISE Preliminary Catalog, bringing the total to six times as many exposures spanning over 16 times as large a time baseline as the AllWISE catalog. The other major change from the CatWISE Preliminary Catalog is that the detection list for the CatWISE2020 Catalog was generated using crowdsource from Schlafly et al., while the CatWISE Preliminary Catalog used the detection software used for AllWISE. These two factors result in roughly twice as many sources in the CatWISE2020 Catalog. The scatter with respect to Spitzer photometry at faint magnitudes in the COSMOS field, which is out of the Galactic Plane and at low ecliptic latitude (corresponding to lower WISE coverage depth) is similar to that for the CatWISE Preliminary Catalog. The 90% completeness depth for the CatWISE2020 Catalog is at W1 = 17.7 mag and W2 = 17.5 mag, 1.7 mag deeper than in the CatWISE Preliminary Catalog. In comparison to Gaia, CatWISE2020 motions are accurate at the 20 mas yr⁻¹ level for W1~15 mag sources and at the ~100 mas yr⁻¹ level for W1~17 mag sources. This level of accuracy represents a 12× improvement over AllWISE. The CatWISE catalogs are available in the WISE/NEOWISE Enhanced and Contributed Products area of the NASA/IPAC Infrared Science Archive.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4365/abd805DOIArticle
https://arxiv.org/abs/2012.13084arXivDiscussion Paper
https://catwise.github.ioRelated ItemCatWISE website
ORCID:
AuthorORCID
Marocco, Federico0000-0001-7519-1700
Fowler, John W.0000-0002-7564-9643
Kirkpatrick, J. Davy0000-0003-4269-260X
Meisner, Aaron M.0000-0002-1125-7384
Schlafly, Edward F.0000-0002-3569-7421
Caselden, Dan0000-0001-7896-5791
Cushing, Michael C.0000-0001-7780-3352
Cutri, Roc M.0000-0002-0077-2305
Faherty, Jacqueline K.0000-0001-6251-0573
Gonzalez, Anthony H.0000-0002-0933-8601
Jarrett, Thomas H.0000-0002-4939-734X
Schlegel, David J.0000-0002-5042-5088
Stern, Daniel0000-0003-2686-9241
Teplitz, Harry I.0000-0002-7064-5424
Wright, Edward L.0000-0001-5058-1593
Additional Information:© 2021. The American Astronomical Society. Received 2020 July 18; revised 2020 December 17; accepted 2020 December 23; published 2021 February 23. We thank the anonymous referee for their careful review and thoughtful suggestions. CatWISE uses data products from WISE, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory (JPL)/California Institute of Technology (Caltech), funded by the National Aeronautics and Space Administration (NASA), and from NEOWISE, which is a joint project of JPL/Caltech and the University of Arizona funded by NASA. Characterization of CatWISE performance uses data from Gaia and from Spitzer. CatWISE is led by JPL/Caltech, with funding from NASA's Astrophysics Data Analysis Program (ADAP), and is also supported in part by ADAP grant NNH17AE75I at Lawrence Berkeley Laboratory. F.M. acknowledges support from the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Universities Space Research Association under a contract with NASA. F.M. also acknowledges support from grant 80NSSC20K0452 under the NASA Astrophysics Data Analysis Program. F.M. would like to thank Dongwei Fan for help with accessing the GPS1+ data via the China-VO.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
UCLAUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
NASANNH17AE75I
NASA Postdoctoral ProgramUNSPECIFIED
NASA80NSSC20K0452
Subject Keywords:Astronomy databases; Infrared astronomy; Infrared photometry; Catalogs
Issue or Number:1
Classification Code:Unified Astronomy Thesaurus concepts: Astronomy databases (83); Infrared astronomy (786); Infrared photometry (792); Catalogs (205)
DOI:10.3847/1538-4365/abd805
Record Number:CaltechAUTHORS:20210204-092658386
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210204-092658386
Official Citation:Federico Marocco et al 2021 ApJS 253 8
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:107901
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:04 Feb 2021 22:04
Last Modified:13 Apr 2021 17:37

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