TY - JOUR KW - galaxy: formation KW - galaxy: halo KW - galaxy: structure KW - local group KW - DIGITAL SKY SURVEY KW - EXPLORING HALO SUBSTRUCTURE KW - TRACING GALAXY FORMATION KW - HERCULES-AQUILA CLOUD KW - WAY GLOBULAR-CLUSTERS KW - MILKY-WAY KW - PISCES OVERDENSITY KW - DWARF GALAXY KW - TRIANGULUM-ANDROMEDA KW - SATELLITE GALAXIES N1 - This version is the version of record. For information on re-use, please refer to the publisher?s terms and conditions. IS - 2 EP - 11 SN - 1538-4357 TI - Discovery of a stellar overdensity in eridanus?phoenix in the dark energy survey AV - public A1 - Li, TS A1 - Balbinot, E A1 - Mondrik, N A1 - Marshall, JL A1 - Yanny, B A1 - Bechtol, K A1 - Drlica-Wagner, A A1 - Oscar, D A1 - Santiago, B A1 - Simon, JD A1 - Vivas, AK A1 - Walker, AR A1 - Wang, MY A1 - Abbott, TMC A1 - Abdalla, FB A1 - Benorr-Levy, A A1 - Bernstein, GM A1 - Bertin, E A1 - Brooks, D A1 - Burke, DL A1 - Carnero Rosell, A A1 - Kind, MC A1 - Carretero, J A1 - da Costa, LN A1 - DePoy, DL A1 - Desai, S A1 - Diehl, HT A1 - Doel, P A1 - Estrada, J A1 - Finley, DA A1 - Flaugher, B A1 - Frieman, J A1 - Gruen, D A1 - Gruendl, RA A1 - Gutierrez, G A1 - Honscheid, K A1 - James, DJ A1 - Kuehn, K A1 - Kuropatkin, N A1 - Lahav, O A1 - Maia, MAG A1 - March, M A1 - Martini, P A1 - Ogando, R A1 - Plazas, AA A1 - Reil, K A1 - Romer, AK A1 - Roodman, A A1 - Sanchez, E A1 - Scarpine, V A1 - Schubnell, M A1 - Sevilla-Noarbe, I A1 - Smith, RC A1 - Soares-Santos, M A1 - Sobreira, F A1 - Suchyta, E A1 - Swanson, MEC A1 - Tarle, G A1 - Tucker, D A1 - Zhang, Y PB - IOP PUBLISHING LTD JF - The Astrophysical Journal VL - 817 N2 - We report the discovery of an excess of main sequence turn-off stars in the direction of the constellations of Eridanus and Phoenix from the first year data of the Dark Energy Survey (DES). The Eridanus-Phoenix (EriPhe) overdensity is centered around l ? 285? and b ? ?60? and spans at least 30? in longitude and 10? in latitude. The Poisson significance of the detection is at least 9?. The stellar population in the overdense region is similar in brightness and color to that of the nearby globular cluster NGC 1261, indicating that the heliocentric distance of EriPhe is about d ? 16 kpc. The extent of EriPhe in projection is therefore at least ? 4 kpc by ? 3 kpc. On the sky, this overdensity is located between NGC 1261 and a new stellar stream discovered by DES at a similar heliocentric distance, the so-called Phoenix Stream. Given their similar distance and proximity to each other, it is possible that these three structures may be kinematically associated. Alternatively, the EriPhe overdensity is morphologically similar to the Virgo overdensity and the Hercules-Aquila cloud, which also lie at a similar Galactocentric distance. These three overdensities lie along a polar plane separated by ? 120? and may share a common origin. Spectroscopic follow-up observations of the stars in EriPhe are required to fully understand the nature of this overdensity ID - discovery10055816 UR - http://dx.doi.org/10.3847/0004-637X/817/2/135 Y1 - 2016/01/27/ ER -