IRS observations of X-ray Background Sources

Details IRS observations of X-ray Background Sources IRS observations of X-ray Background Sources

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...16h&link_type=abstract

Spitzer Proposal ID #16

Physics

Scientific paper

Optically faint or unidentifiable sources from Chandra deep surveys in SSA13, AXAF-South, Lockman Hole, Groth NE, and from XMM-Deep will be selected for IRS lo res observations with the objective of determining spectroscopic redshifts for optically obscured X-ray sources. IRS observations will be obtained only for sources found to have MIPS 24 micron fluxes above about 0.7 mJy.

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