Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)

Details Spitzer quasar and ULIRG evolution study (Veilleux+, 2009) Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21820628v&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/182/628. Originally published in: 2009ApJS..182..628V

Computer Science

Galaxies: Ir, Qsos, Spectroscopy, Redshifts

Scientific paper

Galaxies from our own program (#3187; P.I. Veilleux) were observed in the IRS modules SL, SH, and LH, using staring mode. Together, these modules cover observed wavelengths of 5-35um. The high resolution data at observed wavelengths of 10-35um (SH and LH modules, with resolution R~600) allow sensitive measurements of important atomic and molecular emission lines.
The ULIRG component of our program focuses on the 1Jy sample, a complete flux-limited sample of 118 ULIRGs selected at 60um from a redshift survey of the IRAS faint source catalog (Kim & Sanders, 1998ApJS..119...41K).
(9 data files).

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