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Document Version Version Comment Date Status
559438.0 [No comment] 28.05.2018 16:41 Released

ID: 559438.0, MPI für Astronomie / Publikationen_mpia
The opacity of galactic disks at z ~ 0.7
Authors:Sargent, M. T.; Carollo, C. M.; Kampczyk, P.; Lilly, S. J.; Scarlata, C.; Capak, P.; Ilbert, O.; Koekemoer, A. M.; Kneib, J. P.; Leauthaud, A.; Massey, R.; Oesch, P. A.; Rhodes, J.; Schinnerer, E.; Scoville, N.; Taniguchi, Y.
Date of Publication (YYYY-MM-DD):2010
Title of Journal:The Astrophysical Journal
Journal Abbrev.:The Astrophysical Journal
Issue / Number:1
Start Page:L113
End Page:L117
Review Status:not specified
Audience:Experts Only
Abstract / Description:We compare the surface brightness-inclination relation for a sample of COSMOS pure disk galaxies at z ~ 0.7 with an artificially redshifted sample of Sloan Digital Sky Survey (SDSS) disks well matched to the COSMOS sample in terms of rest-frame photometry and morphology, as well as their selection and analysis. The offset between the average surface brightness of face-on and edge-on disks in the redshifted SDSS sample matches that predicted by measurements of the optical depth of galactic disks in the nearby universe. In contrast, large disks at z ~ 0.7 have a virtually flat surface brightness-inclination relation, suggesting that they are more opaque than their local counterparts. This could be explained by either an increased amount of optically thick material in disks at higher redshift or a different spatial distribution of the dust.
Free Keywords:cosmology: observations; dust; extinction; galaxies: spiral; surveys
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2010ApJ...714L.113S [ID No:1]