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We present the first V, B-V color-magnitude diagram of the Leo IV dwarf spheroidal galaxy, a faint Milky Way satellite recently discovered by the Sloan Digital Sky Survey. We have obtained B,V time-series photometry reaching about half a…

Solar and Stellar Astrophysics · Physics 2009-07-22 M. I. Moretti , M. Dall'Ora , V. Ripepi , G. Clementini , L. Di Fabrizio , H. Smith , N. De Lee , C. Kuehn , M. Catelan , M. Marconi , I. Musella , T. Beers , K. Kinemuchi

We present HST photometry of the resolved stellar population in the dwarf irregular galaxy NGC 1705. The galaxy has been observed with both WFPC2 and NICMOS, and successful images have been obtained in the F555W, F814W, F110W and F160W…

Astrophysics · Physics 2009-11-06 M. Tosi , E. Sabbi , M. Bellazzini , A. Aloisi , L. Greggio , C. Leitherer , P. Montegriffo

An optical monitoring survey in the nearby dwarf galaxies was carried out with the 2.5-m Isaac Newton Telescope (INT). 55 dwarf galaxies and four isolated globular clusters in the Local Group (LG) were observed with the Wide Field Camera…

Aims: We explore the wealth of high quality photometric data provided by data release 2 of the Gaia mission for long period variables (LPVs) in the Large Magellanic Cloud. Our goal is to identify stars of various types and masses along the…

Solar and Stellar Astrophysics · Physics 2018-08-29 T. Lebzelter , N. Mowlavi , P. Marigo , G. Pastorelli , M. Trabucchi , P. R. Wood , I. Lecoeur-Taibi

We have discovered two new high redshift (z=2.38) galaxies, near the previously known z=2.38 galaxy 2139-4434 B1 (Francis et al. 1996). All three galaxies are strong Ly-alpha emitters, and have much redder continuum colors (I-K about 5)…

Astrophysics · Physics 2009-10-30 Paul J. Francis , Bruce E. Woodgate , Anthony C. Danks

Leo P is a low-luminosity dwarf galaxy discovered through the blind HI Arecibo Legacy Fast ALFA (ALFALFA) survey. The HI and follow-up optical observations have shown that Leo P is a gas-rich dwarf galaxy with both active star formation and…

Currently only a small number of Milky Way (MW) stars are known to exist beyond 100 kpc from the Galactic center. Though the distribution of these stars in the outer halo is believed to be sparse, they can provide evidence of more recent…

Astrophysics of Galaxies · Physics 2017-08-02 Robyn E. Sanderson , Amy Secunda , Kathryn V. Johnston , John J. Bochanski

Using the Hubble Space Telescope, we have resolved individual red-giant branch stars in the halos of eight nearby spiral galaxies. The fields lie at projected distances between 2 and 13 kpc along the galaxies' minor axes. The data set…

Astrophysics · Physics 2009-11-13 M. Mouhcine , H. C. Ferguson , R. M. Rich , T. M. Brown , T. E. Smith

Context: Recent near-infrared data have contributed to unveil massive and obscured stellar populations in both new and previously known clusters in our Galaxy. These discoveries lead us to view the Milky Way as an active star-forming…

Solar and Stellar Astrophysics · Physics 2018-06-27 Sebastián Ramírez Alegría , Artemio Herrero , Klaus Rübke , Antonio Marín-Franch , Miriam García , Jura Borissova

The known host galaxies of short-hard gamma-ray bursts (GRBs) to date are characterized by low to moderate star-formation rates and a broad range of stellar masses. In this paper, we positionally associate the recent unambiguously…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Daniel A. Perley , M. Modjaz , A. N. Morgan , S. B. Cenko , J. S. Bloom , N. R. Butler , A. V. Filippenko , A. A. Miller

We have combined optical and near-infrared data of known RR Lyrae (RRL) stars in the bulge in order to study the spatial distribution of its metal-poor component by measuring precise reddening values and distances of 7663 fundamental-mode…

Astrophysics of Galaxies · Physics 2015-01-21 I. Dékány , D. Minniti , M. Catelan , M. Zoccali , R. K. Saito , M. Hempel , O. A. Gonzalez

Recent observations suggest the existence of a white dwarf population in the Galactic halo, while others suggest that deuterium has been astrated in systems at high redshift and low metallicity. We propose that these observations could be…

We use star counts from 13 deep HST fields imaged with the {\it Wide Field Camera - 2} in order to constrain the amount of dark matter in the Galaxy that can be in the form of low-mass main sequence stars or white-dwarfs. Based on the…

Astrophysics · Physics 2015-06-24 Basilio X. Santiago , Gerard Gilmore , Rebecca A. W. Elson

We present a color-based method for identifying red giants based on Pan-STARRS grz and WISE W1 and W2 photometry. We utilize a subsample of bright stars with precise parallaxes from Gaia DR2 to verify that the color-based selection reliably…

We present V and I photometry of the resolved stars in the cometary dwarf irregular galaxy NGC 2366, using Wide Field Planetary Camera 2 images obtained with the Hubble Space Telescope. The resulting color-magnitude diagram reaches down to…

Astrophysics · Physics 2009-11-10 T. X. Thuan , Y. I. Izotov

We report the discovery of two ultra-faint dwarf galaxies, Leo M and Leo K, that lie outside the halo of the Milky Way. Using Hubble Space Telescope imaging of the resolved stars, we create color-magnitude diagrams reaching the old main…

We present a CCD survey of variable stars in the Draco dwarf spheroidal galaxy. This survey, which has the largest areal coverage since the original variable star survey by Baade & Swope, includes photometry for 270 RR Lyrae stars, 9…

(abridged) We studied a large sample of ~14000 dwarf star-forming galaxies with strong emission lines selected from the Sloan Digital Sky Survey (SDSS) and distributed in the redshift range of z~0-0.6. We modelled spectral energy…

Cosmology and Nongalactic Astrophysics · Physics 2023-05-03 Y. I. Izotov , N. G. Guseva , K. J. Fricke , C. Henkel

We present the results of a new search for variable stars in the Local Group dwarf galaxy Leo A, based on deep photometry from the Advanced Camera for Surveys onboard the Hubble Space Telescope. We detected 166 bona fide variables in our…

We report on our analysis of HST/NICMOS snapshot high resolution images of 255 stars in 201 systems within ~10 parsecs of the Sun. Photometry was obtained through filters F110W, F180M, F207M, and F222M using NICMOS Camera 2. These filters…

Solar and Stellar Astrophysics · Physics 2015-06-05 Sergio B. Dieterich , Todd J. Henry , David A. Golimowski , John E. Krist , Angelle M. Tanner
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