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dc.contributor.authorBurchett, Joseph N.
dc.contributor.authorTripp, Todd M.
dc.contributor.authorBordoloi, Rongmon
dc.contributor.authorWerk, Jessica K.
dc.contributor.authorProchaska, J. Xavier
dc.contributor.authorTumlinson, Jason
dc.contributor.authorWillmer, C. N. A.
dc.contributor.authorO’Meara, John
dc.contributor.authorKatz, Neal
dc.date.accessioned2017-04-14T16:30:32Z
dc.date.available2017-04-14T16:30:32Z
dc.date.issued2016-11
dc.date.submitted2016-09
dc.identifier.issn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1721.1/108168
dc.description.abstractUsing Hubble Space Telescope Cosmic Origins Spectrograph observations of 89 QSO sightlines through the Sloan Digital Sky Survey footprint, we study the relationships between C iv absorption systems and the properties of nearby galaxies, as well as the large-scale environment. To maintain sensitivity to very faint galaxies, we restrict our sample to 0.0015 < z < 0.015, which defines a complete galaxy survey to L ≳ 0.01 L* or stellar mass M*≳ 10⁸M [subscript ⊙]. We report two principal findings. First, for galaxies with impact parameter ρ < 1r[subscript vir], C IV detection strongly depends on the luminosity/stellar mass of the nearby galaxy. C IV is preferentially associated with galaxies with M[subscript *] > 10 [superscript 9.5] M [subscript ⊙] lower-mass galaxies rarely exhibit significant C IV absorption (covering fraction f [subscript C = 9 [ subscript-6] [subscript +12] % for 11 galaxies with M[subscript *] < 10 [superscript 9.5]M [subscript ⊙]. Second, C IV detection within the M* > 10 [superscript 9.5]M [subscript ⊙] population depends on environment. Using a fixed-aperture environmental density metric for galaxies with ρ < 160 kpc at z < 0.055, we find that 57 [ subscript -13] [superscript +12]% (8/14) of galaxies in low-density regions (regions with fewer than seven L > 0.15L* galaxies within 1.5 Mpc) have affiliated C IV absorption; however, none (0/7) of the galaxies in denser regions show C IV. Similarly, the C IV detection rate is lower for galaxies residing in groups with dark matter halo masses of M [subscript halo] > 10[superscript12.5]M [subscript ⊙]. In contrast to C IV, H i is pervasive in the circumgalactic medium without regard to mass or environment. These results indicate that C IV absorbers with logN(C IV) ≳13.5 [superscript -2 cm] trace the halos of M* > 10 [superscript 9.5]M[subscript ⊙] galaxies but also reflect larger-scale environmental conditions.en_US
dc.description.sponsorshipSpace Telescope Science Institute (U.S.) (HST-AR-1389)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (HST-GO-11741)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (HST-GO-1159)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (HST-GO-1224)en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.3847/0004-637x/832/2/124en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceIOP Publishingen_US
dc.titleA DEEP SEARCH FOR FAINT GALAXIES ASSOCIATED WITH VERY LOW REDSHIFT C iv ABSORBERS. III. THE MASS- AND ENVIRONMENT-DEPENDENT CIRCUMGALACTIC MEDIUMen_US
dc.typeArticleen_US
dc.identifier.citationBurchett, Joseph N., Todd M. Tripp, Rongmon Bordoloi, Jessica K. Werk, J. Xavier Prochaska, Jason Tumlinson, C. N. A. Willmer, John O’Meara, and Neal Katz. “A DEEP SEARCH FOR FAINT GALAXIES ASSOCIATED WITH VERY LOW REDSHIFT C Iv ABSORBERS. III. THE MASS- AND ENVIRONMENT-DEPENDENT CIRCUMGALACTIC MEDIUM.” The Astrophysical Journal 832, no. 2 (November 22, 2016): 124. © 2016 The American Astronomical Societyen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorBordoloi, Rongmon
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsBurchett, Joseph N.; Tripp, Todd M.; Bordoloi, Rongmon; Werk, Jessica K.; Prochaska, J. Xavier; Tumlinson, Jason; Willmer, C. N. A.; O’Meara, John; Katz, Nealen_US
dspace.embargo.termsNen_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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