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- W2015304642 abstract "Tracking the star formation rate to high redshifts requires knowledge of the contribution from both optically visible and obscured sources. The dusty, optically obscured galaxies can be located by X-ray and infrared surveys. To establish criteria for selecting such sources based only on X-ray and infrared surveys, we determine the ratio of infrared to X-ray brightness that would be observed by SIRTF and Chandra for objects with the same spectral shapes as nearby starbursts if seen at high redshift. The parameter infrared/X-ray (IR/X) is defined as IR/X = (flux density observed in the SIRTF Multiband Imaging Photometer 24 μm filter in mJy)/(total flux observed within 0.5-2.0 keV in units of 10-16 ergs s-1 cm-2). Based on observations of NGC 4038/39 (The Antennae), NGC 3690+IC 694 (Arp 299 or Mrk 171), M82, and Arp 220, nine starburst regions are compared using mid-infrared spectra taken by the Infrared Space Observatory and X-ray spectra obtained with Chandra. The IR/X are determined as they would appear for 1 4 would not match any of the objects considered." @default.
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- W2015304642 date "2004-01-01" @default.
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- W2015304642 title "ComparingChandraandSIRTFObservations for Obscured Starbursts and Active Galactic Nuclei at High Redshift" @default.
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- W2015304642 doi "https://doi.org/10.1086/379785" @default.
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