Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012)

Details Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012) Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012)

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..21980001f&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/198/1. Originally published in: 2012ApJS..198....1F

Computer Science

Active Gal. Nuclei, Galaxy Catalogs, Redshifts, Surveys, Photometry: Ugriz, Photometry: Ultraviolet, Photometry: Infrared

Scientific paper

The field has been observed with XMM-Newton in the time period between 2000 April and 2002 December. In the far-ultraviolet (FUV) and the near-ultraviolet (NUV) the Lockman Hole area was observed by the Galaxy Evolution Explorer (GALEX). Here, we consider the magnitude in 3" diameter aperture available in the General Release 4/5 (GR4/5). In the optical wavelengths, our data set consists of a compilation of observations from Large Binocular Telescope (LBT; between 2007 February and 2009 March in 5 bands (U, B, V, Y, and z')), Subaru (between 2001 November and 2002 April in the Rc, Ic, and z' filters), and Sloan Digital Sky Survey (SDSS-DR7). The near-infrared view of our sources is provided by the data release 7 of the UKIRT Infrared Deep Sky Survey (UKIDSS). For the near- to mid-infrared wavelengths we are using observations at 3.6um, 4.5um, 5.8um, and 8.0um from the IRAC.
(3 data files).

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