========================================================================== J/ApJS/73/359 1.49 GHz atlas of the IRAS bright galaxies (Condon+, 1990) The following files can be converted to FITS (extension .fit .fgz or .fiZ) iras1490.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJS/73/359 ==========================================================================
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Beginning of ReadMe : J/ApJS/73/359 1.49 GHz atlas of the IRAS bright galaxies (Condon+, 1990) ================================================================================ A 1.49 GHz atlas of the IRAS bright galaxy sample. Condon J.J., Helou G., Sanders D.B., Soifer B.T. <Astrophys. J. Suppl. Ser. 73, 359 (1990)> =1990ApJS...73..359C ================================================================================ ADC_Keywords: Radio continuum ; Infrared sources ; Galaxies, IR ; Galaxies, radio Keywords: galaxies: structure - infrared: sources - radio sources: galaxies Description: This catalog contains 1.49 GHz VLA observations of sources from the IRAS Bright Galaxy Sample. The original IRAS Bright Galaxy Sample (Soifer et al., 1987ApJ...320..238S) comprises 324 extragalactic objects with 60 micron flux densities above 5.4 Jy. It is the infrared analog of the radio 3CR or optical Shapley-Ames samples. Recalibration of the IRAS flux densities led to a revised Bright Galaxy Sample (Soifer et al., 1989AJ.....98..766S) containing 313 sources stronger than 5.24 Jy at 60 microns. Only one source from these samples was not detected (NGC1377) at 1.49 GHz. For most sources, multiple observations were conducted with different synthesized beam areas. Thus, for a given galaxy there may be several rows in the table reporting data at different angular resolution or reporting different radio components of the object. A low-resolution observation was used to yield an accurate total flux density and a high-resolution observation was used to resolve the brightest components clearly. These observations were originally presented in Condon, et al., (1990ApJS...73..359C).
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