/ftp/cats/2/177



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II/177      Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	main
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=II/177
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 2 cats archive 254 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 456 Dec 19 2022 .message -r--r--r-- 1 cats archive 3503 Nov 15 1995 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 3043 Jul 28 1992 intro.tex -r--r--r-- 1 cats archive 33974 Jul 28 1992 main
Beginning of ReadMe : II/177 Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992) ================================================================================ Near Infrared Photometry of a Sample of IRAS Point Sources Fouque P., Le Bertre T., Epchtein N., Guglielmo F., Kerschbaum F. <Astron. Astrophys. Suppl. Ser. 93, 151 (1992)> =1992A&AS...93..151F ================================================================================ ADC_Keywords: Mass loss ; Photometry, classification ; Stars, carbon Description: The results are given for the 516 sources that we have observed from La Silla (452 in the southern hemisphere, plus 64 in the range 0 to 20deg). For each source, the IRAS name is given followed by the epoch of observation (with the convention given in Table 1), the J, H, K, L', M magnitudes that we have obtained, then three classifications based on IRAS Low Resolution Spectra (LRS), IRAS broad-band photometry (VH) and the combination of IRAS broad-band photometry with our near-infrared photometry (Val), and, finally, one association.