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On the Significance of Absorption Features in HST/COS Data
Danforth, Charles W.; France, Kevin; Stocke, John T. +2 more
We present empirical scaling relations for the significance of absorption features detected in medium-resolution, far-UV spectra obtained with the Cosmic Origins Spectrograph (COS). These relations properly account for both the extended wings of the COS line-spread function and the non-Poissonian noise properties of the data, which we characterize…
Warm Gas in the Virgo Cluster. I. Distribution of Lyα Absorbers
Chen, Hsiao-Wen; Yoon, Joo Heon; Putman, Mary E. +2 more
The first systematic study of the warm gas (T = 104 - 5 K) distribution across a galaxy cluster is presented using multiple background QSOs in and around the Virgo Cluster. We detect 25 Lyα absorbers (NH I = 1013.1-15.4 cm-2) in the Virgo velocity range toward 9 of 12 QSO sightlines observed with the Co…
The Star Formation History of M32
Monachesi, Antonela; Lauer, Tod R.; Dressler, Alan +5 more
We use deep Hubble Space Telescope Advanced Camera for Surveys/High Resolution Channel observations of a field within M32 (F1) and an M31 background field (F2) to determine the star formation history (SFH) of M32 from its resolved stellar population. We find that 2-5 Gyr old stars contribute ~40% ± 17% of M32's mass, while ~55% ± 21% of M32's mass…
CLASH: Discovery of a Bright z ~= 6.2 Dwarf Galaxy Quadruply Lensed by MACS J0329.6-0211
Shu, X.; Zheng, W.; Molino, A. +22 more
We report the discovery of a z phot = 6.18+0.05 - 0.07 (95% confidence level) dwarf galaxy, lensed into four images by the galaxy cluster MACS J0329.6-0211 (zl = 0.45). The galaxy is observed as a high-redshift dropout in HST/ACS/WFC3 CLASH and Spitzer/IRAC imaging. Its redshift is securely determined du…
Weak-lensing Results for the Merging Cluster A1758
Bradač, M.; Markevitch, M.; Gonzalez, A. H. +2 more
Here we present the weak-lensing results for A1758, which is known to consist of four subclusters undergoing two separate mergers, A1758N and A1758S. Weak-lensing results for A1758N agree with previous weak-lensing results for clusters 1E0657-558 (Bullet cluster) and MACS J0025.4-1222, whose X-ray gas components were found to be largely separated …
Discovery of VHE emission towards the Carina arm region with the H.E.S.S. telescope array: HESS J1018-589
Klochkov, D.; Santangelo, A.; Quirrenbach, A. +191 more
The Carina arm region, containing the supernova remnant SNR G284.3-1.8, the high-energy (HE; E > 100 MeV) binary 1FGL J1018.6-5856 and the energetic pulsar PSR J1016-5857 and its nebula, has been observed with the H.E.S.S. telescope array. The observational coverage of the region in very-high-energy (VHE; E > 0.1 TeV) γ-rays benefits from de…
Sizing up Partially Depleted Galaxy Cores
Graham, Alister W.; Dullo, Bililign T.
We have modeled the inner surface brightness profiles of 39 alleged "core" galaxies with the core-Sérsic model, and provide new physical parameters for the largest ever sample of "core" galaxies fit with this model. When present, additional nuclear components were simultaneously modeled and the typical root-mean-square scatter of the fits (out to …
The Stellar and Gas Kinematics of the LITTLE THINGS Dwarf Irregular Galaxy NGC 1569
Brinks, Elias; Hunter, Deidre A.; Johnson, Megan +5 more
In order to understand the formation and evolution of Magellanic-type dwarf irregular (dIm) galaxies, one needs to understand their three-dimensional structure. We present measurements of the stellar velocity dispersion in NGC 1569, a nearby post-starburst dIm galaxy. The stellar vertical velocity dispersion, σz, coupled with the maximu…
A unique isolated dwarf spheroidal galaxy at D = 1.9 Mpc
Makarova, Lidia; Guhathakurta, Puragra; Makarov, Dmitry +5 more
We present a photometric and spectroscopic study of the unique isolated nearby dwarf spheroidal (dSph) galaxy KKR 25. The galaxy was resolved into stars with Hubble Space Telescope/Wide Field Planetary Camera 2 including old red giant branch and red clump. We have constructed a model of the resolved stellar populations and measured the star format…
Dust-to-gas Ratio in the Extremely Metal-poor Galaxy I Zw 18
Cannon, John M.; Bolatto, Alberto D.; Leroy, Adam K. +7 more
The blue compact dwarf galaxy I Zw 18 is one of the most metal-poor systems known in the local universe (12+log(O/H) = 7.17). In this work we study I Zw 18 using data from Spitzer, Herschel Space Telescope, and IRAM Plateau de Bure Interferometer. Our data set includes the most sensitive maps of I Zw 18, to date, in both the far-infrared and the C…