submm point sources from the Archeops experiment (Desert+, 2008)

Details submm point sources from the Archeops experiment (Desert+, 2008) submm point sources from the Archeops experiment (Desert+, 2008)

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34810411d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/481/411. Originally published in: 2008A&A...481..411D

Other

Interstellar Medium, Millimetric/Submm Sources

Scientific paper

Table 3 gives coordinates and basic photometric properties. The name of the source gives the galactic coordinates in degrees. Fluxes and 1-sigma errors are in Jy, assuming a Rayleigh-Jeans color and for the 4 frequencies of 143, 217, 353 and 545GHz. No available measurements are quoted as (sigma=-1). Upper limits are quoted at the 2-sigma level. The bright sources with an asterisk have positional uncertainties larger than the nominal 4arcmin (1-sigma).
Table 4 gives the model fit parameters and associations. For each point source, the emissivity exponent beta and temperature T are given along with the reduced chi^2 value. When the fit is unsatisfactory, beta11 (assuming a fixed temperature of 11K), or T2 (assuming a fixed exponent index of 2) are provided instead. The associated Iras source is given along with the far infrared fluxes. A star by the name of the Iras counterpart indicates that the Iras source has the Iras colors of an ultra-compact HII region. Then associations with a commonly used name are given with Lynds Dark Nebulae, Bright Nebulae, Sharpless and other common catalogs. Associations with HII regions (with angular size le 10arcmin) from the catalogue by Paladini et al. (2003, Cat. ) are also given.
(2 data files).

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