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Paper detail

Deep Herschel view of obscured star formation in the Bullet cluster

We use deep, five band (100-500um) data from the Herschel Lensing Survey (HLS) to fully constrain the obscured star formation rate, SFR_FIR, of galaxies in the Bullet cluster (z=0.296), and a smaller background system (z=0.35) in the same field. Herschel detects 23 Bullet cluster members with a total SFR_FIR = 144 +/- 14 M_sun yr^-1. On average, the background system contains brighter far-infrared (FIR) galaxies, with ~50% higher SFR_FIR (21 galaxies; 207 +/- 9 M_sun yr^-1). SFRs extrapolated from 24um flux via recent templates (SFR_24) agree well with SFR_FIR for ~60% of the cluster galaxies. In the remaining ~40%, SFR_24 underestimates SFR_FIR due to a significant excess in observed S_100/S_24 (rest frame S_75/S_18) compared to templates of the same FIR luminosity.

preprint2010arXivOpen access
T. D. RawleS. M. ChungD. FaddaM. RexE. EgamiP. G. Pérez-GonzálezB. AltieriA. W. BlainC. R. BridgeA. K. FiedlerA. H. GonzalezM. J. PereiraJ. RichardI. SmailI. ValtchanovM. ZemcovP. N. AppletonJ. J. BockF. BooneB. ClementF. CombesC. D. DowellM. Dessauges-ZavadskyO. IlbertR. J. IvisonM. JauzacJ. -P. KneibD. LutzR. PellóG. H. RiekeG. RodighieroD. SchaererG. P. SmithG. L. WalthP. van der WerfM. W. Werner
astro-ph.CO
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T. D. RawleS. M. ChungD. FaddaM. RexE. EgamiP. G. Pérez-GonzálezB. AltieriA. W. BlainC. R. BridgeA. K. FiedlerA. H. GonzalezM. J. PereiraJ. RichardI. SmailI. ValtchanovM. ZemcovP. N. AppletonJ. J. BockF. BooneB. ClementF. CombesC. D. DowellM. Dessauges-ZavadskyO. IlbertR. J. IvisonM. JauzacJ. -P. KneibD. LutzR. PellóG. H. RiekeG. RodighieroD. SchaererG. P. SmithG. L. WalthP. van der WerfM. W. Werner

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