Discovery of hyperluminous infrared galaxies using spitzer and sharc-II

C. Borys; V. Barnard; C. Bian; A. W. Blain; M. J.I. Brown; A. Dey; C. D. Dowell; D. T. Frayer; J. Higdon; S. Higdon; B. Jannuzi; E. Le Fl'och; B. T. Soifer; T. G. Phillips

Discovery of hyperluminous infrared galaxies using spitzer and sharc-II

C. Borys
, V. Barnard
, C. Bian
, A. W. Blain
, M. J.I. Brown
, A. Dey
, C. D. Dowell
, D. T. Frayer
, J. Higdon
, S. Higdon
, B. Jannuzi
, E. Le Fl'och
, B. T. Soifer
, T. G. Phillips

Research output: Contribution to journal › Conference article › peer-review

Abstract

We have used observations taken as part of the Bootes Spitzer GTO program to pre-select high redshift luminous star-forming galaxy candidates. Subsequent ground-based sub-millimeter imaging using SHARC-II at the Caltech Submillimeter Observatory detected several objects, including one particularly exotic one: An extremely bright infrared galaxy with an apparent luminosity in excess of 10 ^13.5L _⊙. It has a spectral energy distribution similar to that of Arp 220, though appears to be at a much higher redshift. Although lensing is one possible explanation, this object has helped refine the selection method, and hints at a way to pre-select similar objects using Mid-IR silicate absorption features. galaxy evolution; galaxy formation; starburst galaxies.

Original language	English (US)
Pages (from-to)	275-276
Number of pages	2
Journal	European Space Agency, (Special Publication) ESA SP
Issue number	577
State	Published - 2005
Externally published	Yes
Event	The Dusty and Molecular Universe - A Prelude to Herschel and ALMA - Paris, France Duration: Oct 27 2004 → Oct 29 2004

ASJC Scopus subject areas

Aerospace Engineering
Space and Planetary Science

Cite this

@article{6d673916511e4b27ba5131216c5f808f,

title = "Discovery of hyperluminous infrared galaxies using spitzer and sharc-II",

abstract = "We have used observations taken as part of the Bootes Spitzer GTO program to pre-select high redshift luminous star-forming galaxy candidates. Subsequent ground-based sub-millimeter imaging using SHARC-II at the Caltech Submillimeter Observatory detected several objects, including one particularly exotic one: An extremely bright infrared galaxy with an apparent luminosity in excess of 10 13.5L ⊙. It has a spectral energy distribution similar to that of Arp 220, though appears to be at a much higher redshift. Although lensing is one possible explanation, this object has helped refine the selection method, and hints at a way to pre-select similar objects using Mid-IR silicate absorption features. galaxy evolution; galaxy formation; starburst galaxies.",

author = "C. Borys and V. Barnard and C. Bian and Blain, \{A. W.\} and Brown, \{M. J.I.\} and A. Dey and Dowell, \{C. D.\} and Frayer, \{D. T.\} and J. Higdon and S. Higdon and B. Jannuzi and \{Le Fl'och\}, E. and Soifer, \{B. T.\} and Phillips, \{T. G.\}",

year = "2005",

language = "English (US)",

pages = "275--276",

journal = "European Space Agency, (Special Publication) ESA SP",

issn = "0379-6566",

publisher = "European Space Agency",

number = "577",

note = "The Dusty and Molecular Universe - A Prelude to Herschel and ALMA ; Conference date: 27-10-2004 Through 29-10-2004",

}

TY - JOUR

T1 - Discovery of hyperluminous infrared galaxies using spitzer and sharc-II

AU - Borys, C.

AU - Barnard, V.

AU - Bian, C.

AU - Blain, A. W.

AU - Brown, M. J.I.

AU - Dey, A.

AU - Dowell, C. D.

AU - Frayer, D. T.

AU - Higdon, J.

AU - Higdon, S.

AU - Jannuzi, B.

AU - Le Fl'och, E.

AU - Soifer, B. T.

AU - Phillips, T. G.

PY - 2005

Y1 - 2005

N2 - We have used observations taken as part of the Bootes Spitzer GTO program to pre-select high redshift luminous star-forming galaxy candidates. Subsequent ground-based sub-millimeter imaging using SHARC-II at the Caltech Submillimeter Observatory detected several objects, including one particularly exotic one: An extremely bright infrared galaxy with an apparent luminosity in excess of 10 13.5L ⊙. It has a spectral energy distribution similar to that of Arp 220, though appears to be at a much higher redshift. Although lensing is one possible explanation, this object has helped refine the selection method, and hints at a way to pre-select similar objects using Mid-IR silicate absorption features. galaxy evolution; galaxy formation; starburst galaxies.

AB - We have used observations taken as part of the Bootes Spitzer GTO program to pre-select high redshift luminous star-forming galaxy candidates. Subsequent ground-based sub-millimeter imaging using SHARC-II at the Caltech Submillimeter Observatory detected several objects, including one particularly exotic one: An extremely bright infrared galaxy with an apparent luminosity in excess of 10 13.5L ⊙. It has a spectral energy distribution similar to that of Arp 220, though appears to be at a much higher redshift. Although lensing is one possible explanation, this object has helped refine the selection method, and hints at a way to pre-select similar objects using Mid-IR silicate absorption features. galaxy evolution; galaxy formation; starburst galaxies.

UR - https://www.scopus.com/pages/publications/23844519039

UR - https://www.scopus.com/pages/publications/23844519039#tab=citedBy

M3 - Conference article

AN - SCOPUS:23844519039

SN - 0379-6566

SP - 275

EP - 276

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

IS - 577

T2 - The Dusty and Molecular Universe - A Prelude to Herschel and ALMA

Y2 - 27 October 2004 through 29 October 2004

ER -

Discovery of hyperluminous infrared galaxies using spitzer and sharc-II

Abstract

ASJC Scopus subject areas

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