SIMBAD references

2016AJ....151...75G - Astron. J., 151, 75 (2016/March-0)

The CDF archive: Herschel PACS and SPIRE spectroscopic data pipeline and products for protostars and young stellar objects.

GREEN J.D., YANG Y.-L., EVANS II N.J., KARSKA A., HERCZEG G., VAN DISHOECK E.F., LEE J.-E., LARSON R.L. and BOUWMAN J.

Abstract (from CDS):

We present the COPS-DIGIT-FOOSH (CDF) Herschel spectroscopy data product archive, and related ancillary data products, along with data fidelity assessments, and a user-created archive in collaboration with the Herschel-PACS and SPIRE ICC groups. Our products include datacubes, contour maps, automated line fitting results, and best 1D spectra products for all protostellar and disk sources observed with PACS in RangeScan mode for two observing programs: the DIGIT Open Time Key Program (KPOTnevans1 and SDPnevans1; PI: N. Evans), and the FOOSH Open Time Program (OT1jgreen022; PI: J. Green). In addition, we provide our best SPIRE-FTS spectroscopic products for the COPS Open Time Program (OT2jgreen026; PI: J. Green) and FOOSH sources. We include details of data processing, descriptions of output products, and tests of their reliability for user applications. We identify the parts of the data set to be used with caution. The resulting absolute flux calibration has improved in almost all cases. Compared to previous reductions, the resulting rotational temperatures and numbers of CO molecules have changed substantially in some sources. On average, however, the rotational temperatures have not changed substantially (<2%), but the number of warm (Trot∼ 300 K) CO molecules has increased by about 18%.

Abstract Copyright:

Journal keyword(s): infrared: stars - stars: formation - submillimeter: ISM - submillimeter: stars - surveys - techniques: imaging spectroscopy

VizieR on-line data: <Available at CDS (J/AJ/151/75): table1.dat table8.dat>

CDS comments: IRAS 04362+2535 is a misprint for IRAS 04365+2535. [TS84] IRS 7C = [NWA2005] SMM 1C in Simbad.

Simbad objects: 87

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2019.10.19-23:12:54

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