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THE DISAPPEARANCE OF Ly{alpha} BLOBS: A GALEX SEARCH AT z = 0.8

Journal Article · · Astronomical Journal (New York, N.Y. Online)
;  [1];  [2]
  1. Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487 (United States)
  2. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom)
Ly{alpha} blobs-luminous, spatially extended emission-line nebulae, often lacking bright continuum counterparts-are common in dense environments at high redshift. Until recently, atmospheric absorption and filter technology have limited our knowledge of any similar objects at z {<=} 2. We use Galaxy Evolution Explorer slitless spectroscopy to search for similar objects in the rich environments of two known cluster and supercluster fields at z = 0.8, where the instrumental sensitivity peaks. The regions around Cl 1054-0321 and Cl 0023+0423 were each observed in slitless-spectrum mode for 10-19 ks, with accompanying direct images of 3-6 ks to assist in recognizing continuum sources. Using several detection techniques, we find no resolved Ly{alpha} emitters to a flux limit of (1.5-9) x 10{sup -15} erg cm{sup -2} s{sup -1}, on size scales of 5-30 arcsec. This corresponds to line luminosities of (0.5-3) x 10{sup 43} erg s{sup -1} for linear scales 35-200 kpc. Comparison with both blind and targeted surveys at higher redshifts indicates that the population must have evolved in comoving density at least as strongly as (1 + z){sup 3}. These results suggest that the population of Ly{alpha} blobs is specific to the high-redshift universe.
OSTI ID:
21301623
Journal Information:
Astronomical Journal (New York, N.Y. Online), Journal Name: Astronomical Journal (New York, N.Y. Online) Journal Issue: 3 Vol. 138; ISSN 1538-3881
Country of Publication:
United States
Language:
English

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