Extragalactic submillimetric surveys with BLAST

E. Pascale; P. A.R. Ade; J. J. Bock; E. L. Chapin; M. J. Devlin; M. Griffin; J. O. Gundersen; M. Halpern; P. C. Hargrave; D. H. Hughes; J. Klein; G. Marsden; P. G. Martin; P. Mauskopf; L. Moncelsi; C. B. Netterfield; H. Ngo; L. Olmi; G. Patanchon; M. Rex; D. Scott; C. Semisch; N. Thomas; M. D.P. Truch; C. Tucker; G. S. Tucker; M. P. Viero; D. V. Wiebe

doi:10.1051/eas/1040057

Extragalactic submillimetric surveys with BLAST

E. Pascale, P. A.R. Ade, J. J. Bock, E. L. Chapin, M. J. Devlin, M. Griffin, J. O. Gundersen, M. Halpern, P. C. Hargrave, D. H. Hughes, J. Klein, G. Marsden, P. G. Martin, P. Mauskopf, L. Moncelsi, C. B. Netterfield, H. Ngo, L. Olmi, G. Patanchon, M. RexD. Scott, C. Semisch, N. Thomas, M. D.P. Truch, C. Tucker, G. S. Tucker, M. P. Viero, D. V. Wiebe

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2 Scopus citations

Abstract

The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) has recently conducted an extragalactic submillimetric survey of the Chandra Deep Field South region of unprecedented size, depth, and angular resolution in three wavebands centered at 250, 350, and 500μm. BLAST wavelengths are chosen to study the Cosmic Infrared Background near its peak at 200μm. We find that most of the CIB at these wavelengths is contributed by galaxies detected at 24μby the MIPS instrument on Spitzer, and that the source counts distribution shows a population with strongly evolving density and luminosity. These results anticipate what can be expected from the surveys that will be conducted with the SPIRE instrument on the Herschel space observatory.

Original language	English (US)
Pages (from-to)	411-415
Number of pages	5
Journal	EAS Publications Series
Volume	40
DOIs	https://doi.org/10.1051/eas/1040057
State	Published - 2010
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
General Engineering
Space and Planetary Science

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Pascale, E., Ade, P. A. R., Bock, J. J., Chapin, E. L., Devlin, M. J., Griffin, M., Gundersen, J. O., Halpern, M., Hargrave, P. C., Hughes, D. H., Klein, J., Marsden, G., Martin, P. G., Mauskopf, P., Moncelsi, L., Netterfield, C. B., Ngo, H., Olmi, L., Patanchon, G., ... Wiebe, D. V. (2010). Extragalactic submillimetric surveys with BLAST. EAS Publications Series, 40, 411-415. https://doi.org/10.1051/eas/1040057

Pascale, E, Ade, PAR, Bock, JJ, Chapin, EL, Devlin, MJ, Griffin, M, Gundersen, JO, Halpern, M, Hargrave, PC, Hughes, DH, Klein, J, Marsden, G, Martin, PG, Mauskopf, P, Moncelsi, L, Netterfield, CB, Ngo, H, Olmi, L, Patanchon, G, Rex, M, Scott, D, Semisch, C, Thomas, N, Truch, MDP, Tucker, C, Tucker, GS, Viero, MP & Wiebe, DV 2010, 'Extragalactic submillimetric surveys with BLAST', EAS Publications Series, vol. 40, pp. 411-415. https://doi.org/10.1051/eas/1040057

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title = "Extragalactic submillimetric surveys with BLAST",

abstract = "The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) has recently conducted an extragalactic submillimetric survey of the Chandra Deep Field South region of unprecedented size, depth, and angular resolution in three wavebands centered at 250, 350, and 500μm. BLAST wavelengths are chosen to study the Cosmic Infrared Background near its peak at 200μm. We find that most of the CIB at these wavelengths is contributed by galaxies detected at 24μby the MIPS instrument on Spitzer, and that the source counts distribution shows a population with strongly evolving density and luminosity. These results anticipate what can be expected from the surveys that will be conducted with the SPIRE instrument on the Herschel space observatory.",

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AU - Pascale, E.

AU - Ade, P. A.R.

AU - Bock, J. J.

AU - Chapin, E. L.

AU - Devlin, M. J.

AU - Griffin, M.

AU - Gundersen, J. O.

AU - Halpern, M.

AU - Hargrave, P. C.

AU - Hughes, D. H.

AU - Klein, J.

AU - Marsden, G.

AU - Martin, P. G.

AU - Mauskopf, P.

AU - Moncelsi, L.

AU - Netterfield, C. B.

AU - Ngo, H.

AU - Olmi, L.

AU - Patanchon, G.

AU - Rex, M.

AU - Scott, D.

AU - Semisch, C.

AU - Thomas, N.

AU - Truch, M. D.P.

AU - Tucker, C.

AU - Tucker, G. S.

AU - Viero, M. P.

AU - Wiebe, D. V.

PY - 2010

Y1 - 2010

N2 - The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) has recently conducted an extragalactic submillimetric survey of the Chandra Deep Field South region of unprecedented size, depth, and angular resolution in three wavebands centered at 250, 350, and 500μm. BLAST wavelengths are chosen to study the Cosmic Infrared Background near its peak at 200μm. We find that most of the CIB at these wavelengths is contributed by galaxies detected at 24μby the MIPS instrument on Spitzer, and that the source counts distribution shows a population with strongly evolving density and luminosity. These results anticipate what can be expected from the surveys that will be conducted with the SPIRE instrument on the Herschel space observatory.

AB - The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) has recently conducted an extragalactic submillimetric survey of the Chandra Deep Field South region of unprecedented size, depth, and angular resolution in three wavebands centered at 250, 350, and 500μm. BLAST wavelengths are chosen to study the Cosmic Infrared Background near its peak at 200μm. We find that most of the CIB at these wavelengths is contributed by galaxies detected at 24μby the MIPS instrument on Spitzer, and that the source counts distribution shows a population with strongly evolving density and luminosity. These results anticipate what can be expected from the surveys that will be conducted with the SPIRE instrument on the Herschel space observatory.

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DO - 10.1051/eas/1040057

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JO - EAS Publications Series

JF - EAS Publications Series

ER -

Extragalactic submillimetric surveys with BLAST

Abstract

ASJC Scopus subject areas

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