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Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

Pérez-González, P. G. and Blain, A. W. and Bock, J. J. and Bridge, C. R. and Dowell, C. D. and Fadda, D. and Zemcov, M. (2010) Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts. Astronomy and Astrophysics, 518 . L15. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20101201-100758912

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Abstract

We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the Herschel Lensing Survey (HLS) Program. We describe in detail a photometric procedure designed to recover robust fluxes and deblend faint Herschel sources near the confusion noise. The method is based on the use of the positions of Spitzer/MIPS 24 μm sources as priors. Our catalogs are able to reliably (5σ) recover galaxies with fluxes above 6 and 10 mJy in the PACS 100 and 160 μm channels, respectively, and 12 to 18 mJy in the SPIRE bands. We also obtain spectral energy distributions covering the optical through the far-infrared/millimeter spectral ranges of all the Herschel detected sources, and analyze them to obtain independent estimations of the photometric redshift based on either stellar population or dust emission models. We exemplify the potential of the combined use of Spitzer position priors plus independent optical and IR photometric redshifts to robustly assign optical/NIR counterparts to the sources detected by Herschel and other (sub-)mm instruments.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201014593DOIUNSPECIFIED
http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201014593&Itemid=129PublisherUNSPECIFIED
ORCID:
AuthorORCID
Pérez-González, P. G.0000-0003-4528-5639
Blain, A. W.0000-0001-7489-5167
Bock, J. J.0000-0002-5710-5212
Fadda, D.0000-0002-3698-7076
Zemcov, M.0000-0001-8253-1451
Additional Information:© 2010 ESO. Received 31 March 2010; Accepted 6 May 2010; Published online 16 July 2010. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. This work is based in part on observations made with Spitzer, operated by JPL/Caltech. We thank the AzTEC Team for letting us use their data. P.G.P.-G. acknowledges support from grants AYA 2006–02358, AYA 2006–15698–C02–02, and CSD2006-00070, and the Ramón y Cajal Program, all financed by the Spanish Government and/or the European Union.
Funders:
Funding AgencyGrant Number
Spanish GovernmentAYA 2006–02358
Spanish GovernmentAYA 2006–15698–C02–02
Spanish GovernmentCSD2006-00070
European UnionUNSPECIFIED
Subject Keywords:infrared: galaxies; submillimeter: galaxies; galaxies: evolution; galaxies: high-redshift; gravitational lensing: strong; galaxies: photometry
Record Number:CaltechAUTHORS:20101201-100758912
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20101201-100758912
Official Citation:Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts P. G. Pérez-González, E. Egami, M. Rex, T. D. Rawle, J.-P. Kneib, J. Richard, D. Johansson, B. Altieri, A. W. Blain, J. J. Bock, F. Boone, C. R. Bridge, S. M. Chung, B. Clément, D. Clowe, F. Combes, J.-G. Cuby, M. Dessauges-Zavadsky, C. D. Dowell, N. Espino-Briones, D. Fadda, A. K. Fiedler, A. Gonzalez, C. Horellou, O. Ilbert, R. J. Ivison, M. Jauzac, D. Lutz, R. Pelló, M. J. Pereira, G. H. Rieke, G. Rodighiero, D. Schaerer, G. P. Smith, I. Valtchanov, G. L. Walth, P. van der Werf, M. W. Werner and M. Zemcov A&A 518 L15 (2010) DOI: 10.1051/0004-6361/201014593
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21089
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:01 Dec 2010 21:20
Last Modified:09 Mar 2020 13:19

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