J/ApJS/78/239 J/ApJS/78/239 Orion stars CO-added IRAS fluxes catalog W B Weaver G Jones Astrophys. J. Suppl. Ser. 78 239 1992 1992ApJS...78..239W catalogs infrared: stars stars: emission-line, Be stars: pre-main sequence A catalog of co-added IRAS fluxes for the pre-main-sequence objects in the Herbig-Bell catalog (HBC) is presented. This catalog doubles the number of HBC stars with detected IRAS fluxes and provides improved flux values for the previously known sources. Noise levels are given for all HBC fields in each band, permitting upper limits to be estimated for all undetected sources.

HBC Herbig-Bell Catalog Number --- Name Primary name, taken from the HBC number=1 If the name is too long to fit, it is included in the comments or notes. --- e_f12 rms uncertainty on f12 number=2 rms deviation of the residuals after the baseline fit by SCANPI. mJy f12 12 micron flux estimate Jy e_f25 rms uncertainty on f25 number=2 rms deviation of the residuals after the baseline fit by SCANPI. mJy f25 25 micron flux estimate Jy e_f60 rms uncertainty on f60 number=2 rms deviation of the residuals after the baseline fit by SCANPI. mJy f60 60 micron flux estimate Jy e_f100 rms uncertainty on f100 number=2 rms deviation of the residuals after the baseline fit by SCANPI. mJy f100 100 micron flux estimate Jy PSC(f12) 12 micron flux estimate from the IRAS Point Source Catalog (PSC) Jy n_PSC(f12) PSC(f12) note --- PSC(f25) 25 micron PSC estimate Jy n_PSC(f25) PSC(f25) note --- PSC(f60) 60 micron PSC estimate Jy n_PSC(f60) PSC(f60) note --- PSC(f100) 100 micron PSC estimate Jy n_PSC(f100) PSC(f100) note --- IRAS IRAS PSC number --- Qual Quality estimates number=3 a: high quality, est. errors < 10% b: intermediate quality, est. errors 10-25% c: low quality, est. errors > 25% or minimum detection x: no signal detected y: no measurement possible, usually because of a strong, nearby source --- Notes Processing notes number=4 dxx: deconvolution was performed at xx microns exx: extended source detected of xx width (arcmin) (): offset in arcmin, positive in northerly direction *: object has comments in table5.dat For example, HBC 17 lists d12e2.5(-0.7) as the first part of the processing notes. This means that the default 12 micron flux was changed after it was examined with DECON, a deconvolution program described in the published paper. The point response function of the IRAS beam was convoluted with a rectangular source of 2.5arcmin full width to provide the best fit to the scan. The resulting integrated flux was 24.00Jy (fourth data field) and this extended source was offset 0.7arcmin in a southerly direction with respect to the HBC coordinates. --- HBC Herbig-Bell Catalog Number, if blank, the text continues the previous record --- Name Text of the note --- Lee Brotzman ADS 1994, Patricia Bauer [CDS] 26-Oct-1994May11Addresses: Weaver W.B. and Jones G. Monterey Institute for Research in Astronomy, 900 Major Sherman Lane, Monterey, CA 93940 AAS CD-ROM series, Volume 2, 1994 J_ApJS_78_239.xml