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Related papers: ESO540-032: a Transition-Type Dwarf in the Sculpto…

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We have employed FORS1/2+VLT to acquire deep B and R CCD images of 16 dwarf elliptical galaxies in the direction of the Virgo cluster. For each dwarf we measure the R-band surface brightness fluctuation (SBF) magnitude \bar{m}_R and the…

Astrophysics · Physics 2009-11-10 H. Jerjen , Bruno Binggeli , Fabio D. Barazza

This third paper in a series about the dwarf galaxy populations in groups within the Local Supercluster concerns the intermediate mass (2.1 x 10^13 solar) NGC 5353/4 Group with a core dominated by S0 systems and a periphery of mostly spiral…

Astrophysics · Physics 2009-11-13 R. Brent Tully , Neil Trentham

We present ground-based and HST WFPC2 imaging of the nearby low surface brightness dwarf spheroidal galaxy DDO 44. For the first time DDO 44 was resolved into stars. The resulting color-magnitude diagram for about 1290 stars shows the red…

We present 4-micron ISAAC imaging and spectroscopy of the extremely metal-poor dwarf galaxy SBS 0335-052, aimed at a better understanding of the dust in this low-metallicity galaxy. The 4-micron emission turns out to be very compact,…

Astrophysics · Physics 2009-11-07 L. K. Hunt , L. Vanzi , T. X. Thuan

We present Multiple Mirror Telescope (MMT) and Keck II telescope spectrophotometry and 3.5m Calar Alto telescope R, I photometry of the western component of the extremely low-metallicity blue compact galaxy SBS 0335-052. The components,…

Astrophysics · Physics 2014-10-13 V. A. Lipovetsky , F. H. Chaffee , Y. I. Izotov , C. B. Foltz , A. Y. Kniazev , U. Hopp

We have determined the distance and star formation history of the Local Group dwarf galaxy LGS 3 from deep Hubble Space Telescope WFPC2 observations. LGS 3 is intriguing because ground-based observations showed that, while its stellar…

Astrophysics · Physics 2009-11-07 B. W. Miller , A. E. Dolphin , M. G. Lee , S. C. Kim , P. Hodge

The stellar population of the Pegasus dwarf irregular galaxy is investigated in images taken in the F439W (B), F555W (V), and F814W (I) bands with WFPC2. These and ground-based data are combined to produce color-magnitude diagrams which…

We present the photometric sample of a faint galaxy survey carried out in the southern hemisphere, using CCDs on the 3.60m and NTT-3.5m telescopes at La Silla (ESO). The survey area is a continuous strip of 0.2 deg x 1.53 deg located at…

Astrophysics · Physics 2009-10-30 S. Arnouts , V. de Lapparent , G. Mathez , A. Mazure , Y. Mellier , E. Bertin , A. Kruszewski

We have used the ACS camera on HST to obtain (V,I) photometry for 5300 red-giant stars in the halo of the dominant Leo-group member NGC 3379, a galaxy usually regarded as a classic normal giant elliptical. We use this sample of stars to…

Astrophysics · Physics 2011-02-11 W. E. Harris , G. L. H. Harris , A. C. Layden , E. H. Wehner

We present V and I photometry of a 9.4' X 9.4' field centered on the dwarf spheroidal galaxy Leo II. The Tip of the Red Giant Branch is identified at I^{TRGB}=17.83 +/- 0.03 and adopting <[M/H]> = -1.53 +/- 0.2 from the comparison of RGB…

Astrophysics · Physics 2009-11-10 M. Bellazzini , N. Gennari , F. R. Ferraro

Observations of the highly isolated dwarf spheroidal galaxy KKs 3 = [KK2000] 03 with the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) are presented. We measured the galaxy distance of $2.12\pm0.07$ Mpc using the Tip of Red…

Astrophysics of Galaxies · Physics 2015-06-23 I. D. Karachentsev , L. N. Makarova , D. I. Makarov , R. B. Tully , L. Rizzi

[ABRIDGED] We present the first statistical analysis of the complete ESO-Sculptor redshift survey (ESS). The flux-calibrated sample of 617 galaxy spectra with R_c<20.5 is separated into 3 spectral classes (early, intermediate, and late). We…

Astrophysics · Physics 2008-11-26 Valerie de Lapparent , Gaspar Galaz , Sandro Bardelli , Stephane Arnouts

We present the results of our analysis of the RR Lyrae (RRL) variable stars detected in two transition-type dwarf galaxies (dTrans), ESO294-G010 and ESO410-G005 in the Sculptor group, which is known to be one of the closest neighboring…

Astrophysics of Galaxies · Physics 2015-06-18 Soung-Chul Yang , Rachel Wagner-Kaiser , Ata Sarajedini , Sang Chul Kim , Jaemann Kyeong

We analyze three-band HST/ACS imaging data of the giant elliptical galaxy ESO325-G004. This is the nearest known strongly lensing galaxy, and it resides in the center of the poor cluster Abell S0740 at redshift z=0.034. Based on magnitude,…

Astrophysics · Physics 2009-11-13 John P. Blakeslee , Regina Barber DeGraaff

We describe the current status of the ESO-Sculptor Survey. The observational goal has been to produce a new multi-color photometric catalogue of galaxies in a region located near the southern galactic pole, complemented by a spectroscopic…

Astrophysics · Physics 2007-05-23 V. de Lapparent , G. Galaz , S. Arnouts , S. Bardelli , M. Ramella

Here we present observations with the Advanced Camera for Surveys on the Hubble Space Telescope of the nearby, transition-type dwarf galaxy KK258 = ESO468-020. We measure a distance of 2.23$\pm$0.05 Mpc using the Tip of Red Giant Branch…

Astrophysics of Galaxies · Physics 2015-06-22 I. D. Karachentsev , L. N. Makarova , R. B. Tully , Po-Feng Wu , A. Y. Kniazev

We briefly show results on the redshift and space distribution of field galaxies with different spectral types in the ESO-Sculptor survey (ESS). We also show results on the ESS galaxy luminosity function.

Astrophysics · Physics 2007-05-23 Gaspar Galaz , Valerie de Lapparent

We present wide-field photometry of resolved stars in the nearby Sculptor dwarf spheroidal galaxy using CTIO/MOSAIC, going down to the oldest Main Sequence Turn-Off. The accurately flux calibrated wide field Colour-Magnitude Diagrams can be…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 T. J. L. de Boer , E. Tolstoy , A. Saha , K. Olsen , M. J. Irwin , G. Battaglia , V. Hill , M. D. Shetrone , G. Fiorentino , A. Cole

We present new deep $VI$ ground-based photometry of the Local Group dwarf galaxy Phoenix. Our results confirm that this galaxy is mainly dominated by red stars, with some blue plume stars indicating recent (100 Myr old) star formation in…

Astrophysics · Physics 2009-10-31 D. Martinez-Delgado , C. Gallart , A. Aparicio

We present abundances for seven stars in the (extremely) low-metallicity tail of the Sculptor dwarf spheroidal galaxy, from spectra taken with X-shooter on the ESO VLT. Targets were selected from the Ca II triplet (CaT) survey of the Dwarf…