Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992)

Details Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992) Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992)

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat.2177....0f&link_type=abstract

VizieR On-line Data Catalog: II/177. Originally published in: 1992A&AS...93..151F

Physics

Mass Loss, Photometry: Classification, Stars: Carbon

Scientific paper

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. (1 data file).

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