========================================================================== J/MNRAS/401/1587 Far-infrared survey at North Galactic Pole (Vaisanen+, 2010) The following files can be converted to FITS (extension .fit or fit.gz) tablea2.dat notes.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/401/1587 ==========================================================================
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Beginning of ReadMe : J/MNRAS/401/1587 RIK photometry of far-IR sources in NGP (Vaisanen+, 2010) ================================================================================ A far-infrared survey at the North Galactic Pole. I. Nearby star-forming galaxies and effect of confused sources on source counts. Vaisanen P., Kotilainen J.K., Juvela M., Mattila K., Efstathiou A., Kahanpaa J. <Mon. Not. R. Astron. Soc., 401, 1587-1601 (2010)> =2010MNRAS.401.1587V ================================================================================ ADC_Keywords: Surveys ; Galaxies, IR ; Galactic pole, north ; Photometry, SDSS ; Photometry, infrared Keywords: galaxies: evolution - galaxies: starburst - infrared: galaxies Abstract: We present follow-up observations of the far-infrared (FIR) sources at 90, 150 and 180um detected as part of the ISOPHOT EBL project, which has recently measured the absolute surface brightness of the cosmic infrared background (CIRB) radiation for the first time independently from COBE data. We have observed the fields at the North Galactic Pole region in the optical and near-IR, and complement these data with Sloan Digital Sky Survey photometry, and spectroscopy where available, and present identifications of the 25 FIR sources which reach down to 150mJy in all three ISOPHOT bands. Identifications are done by means of full spectral energy density fitting to all sources in the FIR error circle areas. Description: Table A.2 lists the full photometric catalog of the ISOPHOT EBL project North Galactic Pole fields acquired with the Nordic Optical Telescope, using the ALFOSC (in R and I band) and NOTCAM (in K band) instruments. The photometry is performed with SExtractor and both "total" and aperture magnitudes are given using the AUTO and APER (with 2.7" diameter) magnitudes, as well as the star/galaxy CLASS parameter. The photometry is matched with the SDSS and the ugriz magnitudes are also given. All objects falling within 60" of a given ISOPHOT far-IR source are indicated - these areas are analysed in the Paper.
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