Explanatory Supplement to the WISE All-Sky Data Release Products

By R. Cutri, E. L. Wright, T. Conrow, J. Bauer, Dominic J. Benford, H. Brandenburg, J. Dailey, Peter Eisenhardt, T. Evans, S. Fajardo-Acosta and 32 more. WISE, 2012

372 citations recorded by the source corpus.

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Citations in the corpus

GALAXY AND MASS ASSEMBLY (GAMA): MID-INFRARED PROPERTIES AND EMPIRICAL RELATIONS FROM WISE (2014, methodology): “The work of Donoso et al. (2012) showed the power of combining WISE with a large-area survey (SDSS); they investigated the effect of star formation- and AGN-activity on the WISE properties of >95,000 galaxies, including calibrations using the 12 μm and 22 μm luminosities.”
THE TENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT (2013, methodology): “Given the use of WISE photometry in target selection, we have imported the WISE All-Sky Release catalog (Cutri et al. 2012) into the SDSS CAS, and performed an astrometric cross-match with 4′′ matching radius with the SDSS catalog objects.”
Overview of the DESI Legacy Imaging Surveys (2018, unknown): “During its primary 7-month mission from 2010 January through 2010 August, WISE conducted an all-sky survey in four bands centered at 3.4, 4.6, 12 and 22µm (known as W1, W2, W3 and W4; Wright et al. 2010; Cutri et al. 2012).”
THE DISK POPULATION OF THE UPPER SCORPIUS ASSOCIATION (2012, methodology): “Since the W2 fluxes for saturated stars are significantly overestimated (0.2–1 mag at W2< 6, Cutri et al. 2012), we have omitted these measurements from our tabulation.”
THE RED MSX SOURCE SURVEY: THE MASSIVE YOUNG STELLAR POPULATION OF OUR GALAXY (2013, background): “WISE suffers from saturation for bright sources and the fact that the published catalog is described as a source finding catalog rather than a point source catalog (Cutri et al. 2012).”
The CatWISE2020 Catalog (2020, methodology): “Most of the columns have the same names as in the AllWISE Catalog, and are described in §II.1.a of the AllWISE Explanatory Supplement (Cutri et al. 2013).”
The ATLASGAL survey: a catalog of dust condensations in the Galactic plane (2013, methodology): “…-RMS associ- 11 We convert the magnitudes given in the WISE catalog using the zero-level fluxes from Wright et al. (2010), a color correction factor of 1.0 and a correction factor of 0.9 from Cutri et al. (2012). ations from Urquhart et al. (2013a) and Urquhart et al. (2013b) respectively.”
Unveiling the gas-and-dust disk structure in HD 163296 using ALMA observations (2013, methodology): “The model contains an exponentially tapered-edge and provided an adequate fit to the broadband spectral energy distribution ( SED), the Herschel PACS lines observed by the Key program GASPS (Gas in Protoplanetary Systems; Dent et al. 2013), as well as sub-millimeter interferometry (continuum and CO ”