SIMBAD references

2015ApJ...813..109D - Astrophys. J., 813, 109 (2015/November-2)

Eight ultra-faint galaxy candidates discovered in year two of the dark energy survey.

DRLICA-WAGNER A., BECHTOL K., RYKOFF E.S., LUQUE E., QUEIROZ A., MAO Y.-Y., WECHSLER R.H., SIMON J.D., SANTIAGO B., YANNY B., BALBINOT E., DODELSON S., NETO A.F., JAMES D.J., LI T.S., MAIA M.A.G., MARSHALL J.L., PIERES A., STRINGER K., WALKER A.R., ABBOTT T.M.C., ABDALLA F.B., ALLAM S., BENOIT-LEVY A., BERNSTEIN G.M., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CROCCE M., DA COSTA L.N., DESAI S., DIEHL H.T., DIETRICH J.P., DOEL P., EIFLER T.F., EVRARD A.E., FINLEY D.A., FLAUGHER B., FOSALBA P., FRIEMAN J., GAZTANAGA E., GERDES D.W., GRUEN D., GRUENDL R.A., GUTIERREZ G., HONSCHEID K., KUEHN K., KUROPATKIN N., LAHAV O., MARTINI P., MIQUEL R., NORD B., OGANDO R., PLAZAS A.A., REIL K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SEVILLA-NOARBE I., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., TUCKER D., VIKRAM V., WESTER W., ZHANG Y., ZUNTZ J. (The DES Collaboration)

Abstract (from CDS):

We report the discovery of eight new ultra-faint dwarf galaxy candidates in the second year of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are detected at high confidence, while two lower-confidence candidates are identified in regions of non-uniform survey coverage. The new stellar systems are found by three independent automated search techniques and are identified as overdensities of stars, consistent with the isochrone and luminosity function of an old and metal-poor simple stellar population. The new systems are faint (MV> -4.7) and span a range of physical sizes (17 < r1/2< 181) and heliocentric distances (25 kpc < D< 214 kpc). All of the new systems have central surface brightnesses consistent with known ultra-faint dwarf galaxies (µ ≳ 27.5–2). Roughly half of the DES candidates are more distant, less luminous, and/or have lower surface brightnesses than previously known Milky Way satellite galaxies. Most of the candidates are found in the southern part of the DES footprint close to the Magellanic Clouds. We find that the DES data alone exclude (p < 10–3) a spatially isotropic distribution of Milky Way satellites and that the observed distribution can be well, though not uniquely, described by an association between several of the DES satellites and the Magellanic system. Our model predicts that the full sky may hold ∼100 ultra-faint galaxies with physical properties comparable to the DES satellites and that 20%-30% of these would be spatially associated with the Magellanic Clouds.

Abstract Copyright:

Journal keyword(s): galaxies: dwarf - Local Group

Nomenclature: Tables 1-2: DES JHHMM+DDMM N=8. NAME Grus II = NAME Gru II. NAME Tucana R = NAME Tuc R (Nos III-V) added. NAME Columba I = NAME Col I. NAME Reticulum III = NAME Ret III. NAME Indus II = NAME Ind II. NAME Cetus II = NAME Cet II.

Simbad objects: 50

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2019.09.15-23:01:55

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