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|a (TOE)ost774338
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|a (TOE)774338
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|a E 1.99:la-ur-01-655
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|a E 1.99:la-ur-01-655
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|a la-ur-01-655
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|a HOST GALAXIES AS GAMMA-RAY BURST DISTANCE INDICATORS
|h [electronic resource]
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|a Washington, D.C. :
|b United States. Department of Energy ;
|a Oak Ridge, Tenn. :
|b distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
|c 2001.
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| 300 |
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|a 142 Kilobytes pages :
|b digital, PDF file.
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| 336 |
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|a text
|b txt
|2 rdacontent.
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| 337 |
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|a computer
|b c
|2 rdamedia.
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| 338 |
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|a online resource
|b cr
|2 rdacarrier.
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|a Published through SciTech Connect.
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|a 01/01/2001.
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|a "la-ur-01-655"
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|a Conference title not supplied, Conference location not supplied, Conference dates not supplied.
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| 500 |
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|a ET AL; D. BAND.
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|a We calculate the distributions of the total burst energy, the peak luminosity and the X-ray afterglow energy using burst observations and distances to the associated host galaxies. To expand the sample, we include redshift estimates for host galaxies without spectroscopic redshifts. The methodology requires a model of the host galaxy population; we find that in the best model the burst rate is proportional to the host galaxy luminosity at the time of the burst.
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|b W-7405-ENG-36.
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| 650 |
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|a Afterglow.
|2 local.
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| 650 |
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|a Galaxies.
|2 local.
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| 650 |
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|a Luminosity.
|2 local.
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| 650 |
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|a Distance.
|2 local.
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| 650 |
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|a Indicators.
|2 local.
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| 650 |
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|a Classical And Quantum Mechanics, General Physics.
|2 edbsc.
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| 710 |
2 |
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|a Los Alamos National Laboratory.
|4 res.
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| 710 |
1 |
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|a United States.
|b Department of Energy.
|4 spn.
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| 710 |
1 |
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information.
|4 dst.
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| 856 |
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|u http://www.osti.gov/scitech/biblio/774338
|z Online Access
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| 907 |
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|a .b69857714
|b 03-06-23
|c 03-31-12
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| 998 |
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|a web
|b 09-08-16
|c f
|d m
|e p
|f eng
|g
|h 0
|i 4
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|p Can circulate
|a University of Colorado Boulder
|b Online
|c Online
|d Online
|e E 1.99:la-ur-01-655
|h Superintendent of Documents classification
|i web
|n 1
|
