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Total galaxy magnitudes and effective radii from Petrosian magnitudes and radii

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dc.contributor.authorGraham, Alister
dc.contributor.authorDriver, Simon
dc.contributor.authorPetrosian, Vahe
dc.contributor.authorConselice, Christopher J
dc.contributor.authorBershady, Matthew
dc.contributor.authorCrawford, Steven M
dc.contributor.authorGoto, Tomotsugu
dc.date.accessioned2015-12-13T23:01:57Z
dc.date.issued2005
dc.date.updated2015-12-12T07:43:52Z
dc.description.abstractPetrosian magnitudes were designed to help with the difficult task of determining a galaxy's total light. Although these magnitudes [taken here as the flux within 2RP, with the inverted Petrosian index 1/η(RP) = 0.2] can represent most of an object's flu
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/84663
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxies: fundamental parameters; Galaxies: structure; Methods: analytical; Methods: data analysis
dc.titleTotal galaxy magnitudes and effective radii from Petrosian magnitudes and radii
dc.typeJournal article
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage1544
local.bibliographicCitation.startpage1535
local.contributor.affiliationGraham, Alister, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDriver, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPetrosian, Vahe, Stanford University
local.contributor.affiliationConselice, Christopher J, California Institute of Technology
local.contributor.affiliationBershady, Matthew, University of Wisconsin
local.contributor.affiliationCrawford, Steven M, University of Wisconsin
local.contributor.affiliationGoto, Tomotsugu, Japan Aerospace Exploration Agency
local.contributor.authoruidGraham, Alister, u3782099
local.contributor.authoruidDriver, Simon, u4041024
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub12930
local.identifier.citationvolume130
local.identifier.doi10.1086/444475
local.identifier.scopusID2-s2.0-27744543120
local.type.statusPublished Version

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