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AN ULTRA-FAINT GALAXY CANDIDATE DISCOVERED in EARLY DATA from the MAGELLANIC SATELLITES SURVEY

dc.contributor.authorDrlica-Wagner, Alex
dc.contributor.authorBechtol, Keith C.
dc.contributor.authorAllam, Sahar
dc.contributor.authorTucker, D
dc.contributor.authorGruendl, R.A
dc.contributor.authorJohnson, Michael D.
dc.contributor.authorWalker, Alistair R
dc.contributor.authorJames, David
dc.contributor.authorNidever, David L.
dc.contributor.authorOlsen, Knut A. G.
dc.contributor.authorConn, Blair
dc.date.accessioned2018-11-29T22:56:36Z
dc.date.available2018-11-29T22:56:36Z
dc.date.issued2016
dc.date.updated2018-11-29T08:13:26Z
dc.description.abstractWe report a new ultra-faint stellar system found in Dark Energy Camera data from the first observing run of the Magellanic Satellites Survey (MagLiteS). MagLiteS J0644-5953 (Pictor II or Pic II) is a low surface brightness (μ = 28.5+1 -1 mag arcsec-2 within its half-light radius) resolved overdensity of old and metal-poor stars located at a heliocentric distance of 45+5 -4 kpc. The physical size (r1/2 = 46+15 -11) and low luminosity (Mv = -3.2+0.4 -0.5 mag) of this satellite are consistent with the locus of spectroscopically confirmed ultra-faint galaxies. MagLiteS J0644-5953 (Pic II) is located 11.3+3.1 -0.9 kpc from the Large Magellanic Cloud (LMC), and comparisons with simulation results in the literature suggest that this satellite was likely accreted with the LMC. The close proximity of MagLiteS J0644-5953 (Pic II) to the LMC also makes it the most likely ultra-faint galaxy candidate to still be gravitationally bound to the LMC
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/1885/153579
dc.publisherInstitute of Physics Publishing Ltd.
dc.sourceAstrophysical Journal Letters
dc.titleAN ULTRA-FAINT GALAXY CANDIDATE DISCOVERED in EARLY DATA from the MAGELLANIC SATELLITES SURVEY
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.contributor.affiliationDrlica-Wagner, Alex, Fermi National Accelerator Laboratory
local.contributor.affiliationBechtol, Keith C., University of Chicago
local.contributor.affiliationAllam, Sahar, Fermi National Accelerator Laboratory
local.contributor.affiliationTucker, D, Fermi National Accelerator Laboratory
local.contributor.affiliationGruendl, R.A, University of Illinois
local.contributor.affiliationJohnson, Michael D., University of Illinois at Urbana-Champaign
local.contributor.affiliationWalker, Alistair R, Cerro Tololo Inter-American Obervatory
local.contributor.affiliationJames, David, Cerro Tololo Inter-American Observatory
local.contributor.affiliationNidever, David L., University Michigan Ann Arbor
local.contributor.affiliationOlsen, Knut A. G., National Optical Astronomy Observatory
local.contributor.affiliationConn, Blair, College of Science, ANU
local.contributor.authoruidConn, Blair, u2525160
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationa383154xPUB8438
local.identifier.citationvolume833
local.identifier.doi10.3847/2041-8205/833/1/L5
local.identifier.scopusID2-s2.0-85006365124
local.identifier.thomsonID000401603900005
local.type.statusPublished Version

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