The CatWISE Preliminary Catalog: Motions from WISE and NEOWISE Data

April 2020 • 2020ApJS..247...69E

Authors • Eisenhardt, Peter R. M. • Marocco, Federico • Fowler, John W. • Meisner, Aaron M. • Kirkpatrick, J. Davy • Garcia, Nelson • Jarrett, Thomas H. • Koontz, Renata • Marchese, Elijah J. • Stanford, S. Adam • Caselden, Dan • Cushing, Michael C. • Cutri, Roc M. • Faherty, Jacqueline K. • Gelino, Christopher R. • Gonzalez, Anthony H. • Mainzer, Amanda • Mobasher, Bahram • Schlegel, David J. • Stern, Daniel • Teplitz, Harry I. • Wright, Edward L.

Abstract • CatWISE is a program to catalog sources selected from combined WISE and NEOWISE all-sky survey data at 3.4 and 4.6 &mgrm (W1 and W2). The CatWISE Preliminary Catalog consists of 900,849,014 sources measured in data collected from 2010 to 2016. This data set represents four times as many exposures and spans over 10 times as large a time baseline as that used for the AllWISE Catalog. CatWISE adapts AllWISE software to measure the sources in coadded images created from six-month subsets of these data, each representing one coverage of the inertial sky, or epoch. The catalog includes the measured motion of sources in eight epochs over the 6.5 yr span of the data. From comparison to Spitzer, signal-to-noise ratio = 5 limits in magnitudes in the Vega system are W1 &equals 17.67 and W2 = 16.47, compared to W1 &equals 16.96 and W2 = 16.02 for AllWISE. From comparison to Gaia, CatWISE positions have typical accuracies of 50 mas for stars at W1 &equals 10 mag and 275 mas for stars at W1 = 15.5 mag. Proper motions have typical accuracies of 10 mas yr^-1 and 30 mas yr^-1 for stars with these brightnesses, an order of magnitude better than from AllWISE. The catalog is available in the WISE/NEOWISE Enhanced and Contributed Products area of the NASA/IPAC Infrared Science Archive.

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