/ftp/cats/2/330



==========================================================================
II/330    Northern sky photometric catalog of 44 million sources (Madsen+ 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat table3.dat
==========================================================================

drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 3 cats archive 267 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 325 Dec 4 2015 .message -r--r--r-- 1 cats archive 12212 Dec 4 2015 ReadMe -r--r--r-- 1 cats archive 47180859 Mar 10 2014 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 44243863 Mar 7 2014 table1.fits.gz [Uncompressed] -r--r--r-- 1 cats archive 3417143889 Mar 12 2014 table3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4003635015 Mar 7 2014 table3.fits.gz [Uncompressed]
Beginning of ReadMe : II/330 Northern sky photometric catalog of 44 million sources (Madsen+ 2013) ================================================================================ A precision multi-band two-epoch photometric catalog of 44 million sources in the northern sky from a combination of the USNO-B and Sloan Digital Sky Survey catalogs. Madsen G.J., Gaensler B.M. <Astrophys. J. Suppl. Ser., 209, 33 (2013)> =2013ApJS..209...33M =2014yCat.2330....0M ================================================================================ ADC_Keywords: Surveys; Photometry, SDSS Keywords: catalogs - methods: data analysis - quasars: general - stars: variables: general - techniques: photometric Abstract: A key science driver for the next generation of wide-field optical and radio surveys is the exploration of the time variable sky. These surveys will have unprecedented sensitivity and areal coverage, but will be limited in their ability to detect variability on time scales longer than the lifetime of the surveys. We present a new precision, multi-epoch photometric catalog that spans 60 yr by combining the US Naval Observatory-B (USNO-B) and Sloan Digital Sky Survey (SDSS) Data Release 9 (DR9) catalogs. We recalibrate the photometry of the original USNO-B catalog and create a catalog with two epochs of photometry in up to five different bands for 43,647,887 optical point sources that lie in the DR9 footprint of the northern sky. The recalibrated objects span a magnitude range 14< m< 20 and are accurate to  0.1mag. We minimize the presence of spurious objects and those with inaccurate magnitudes by identifying and removing several sources of systematic errors in the two originating catalogs, with a focus on spurious objects that exhibit large apparent magnitude variations. After accounting for these effects, we find  250,000 stars and quasars that show significant (>=4sigma) changes in brightness between the USNO-B and SDSS DR9 epochs. We discuss the historical value of the catalog and its application to the study of long time scale, large amplitude variable stars and quasars.