A DIRECT MEASUREMENT OF THE INTERGALACTIC MEDIUM OPACITY TO H I IONIZING PHOTONS
- Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States)
- Department of Chemistry and Physics, Saint Michael's College, One Winooski Park, Colchester, VT 05439 (United States)
We present a new method to directly measure the opacity from H I Lyman limit (LL) absorption kappa{sub LL} along quasar sight lines by the intergalactic medium (IGM). The approach analyzes the average ('stacked') spectrum of an ensemble of quasars at a common redshift to infer the mean free path lambda{sup 912}{sub mfp} to ionizing radiation. We apply this technique to 1800 quasars at z = 3.50-4.34 drawn from the Sloan Digital Sky Survey (SDSS), giving the most precise measurements on kappa{sub LL} at any redshift. From z = 3.6 to 4.3, the opacity increases steadily as expected and is well parameterized by lambda{sup 912}{sub mfp} = lambda{sub 0} - b {sub l}ambda(z - 3.6) with lambda{sub 0} = (48.4 +- 2.1) h{sup -1}{sub 72} Mpc and b{sub l}ambda = (38.0 +- 5.3) h {sup -1}{sub 72} Mpc (proper distance). The relatively high lambda{sup 912} {sub mfp} values indicate that the incidence of systems which dominate kappa{sub LL} evolves less strongly at z > 3 than that of the Lyalpha forest. We infer a mean free path three times higher than some previous estimates, a result which has important implications for the photoionization rate derived from the emissivity of star-forming galaxies and quasars. Finally, our analysis reveals a previously unreported, systematic bias in the SDSS quasar sample related to the survey's color targeting criteria. This bias potentially affects all z approx 3 IGM studies using the SDSS database.
- OSTI ID:
- 21378339
- Journal Information:
- Astrophysical Journal (Online), Vol. 705, Issue 2; Other Information: DOI: 10.1088/0004-637X/705/2/L113; ISSN 1538-4357
- Country of Publication:
- United States
- Language:
- English
Similar Records
DISSECTING THE PROPERTIES OF OPTICALLY THICK HYDROGEN AT THE PEAK OF COSMIC STAR FORMATION HISTORY
A DEFINITIVE SURVEY FOR LYMAN LIMIT SYSTEMS AT z {approx} 3.5 WITH THE SLOAN DIGITAL SKY SURVEY
Related Subjects
COSMOLOGY AND ASTRONOMY
ABSORPTION
COLOR
EMISSIVITY
GALAXIES
IONIZING RADIATIONS
MEAN FREE PATH
PHOTOIONIZATION
PHOTONS
QUASARS
RED SHIFT
STARS
UNIVERSE
BOSONS
COSMIC RADIO SOURCES
ELEMENTARY PARTICLES
IONIZATION
MASSLESS PARTICLES
OPTICAL PROPERTIES
ORGANOLEPTIC PROPERTIES
PHYSICAL PROPERTIES
RADIATIONS
SORPTION
SURFACE PROPERTIES