output
19952026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing astro-ph.GAShow all

24 papers · 1 filter

astro-ph.GA2024★ 9 cited

Revealing ringed galaxies in group environments

Julia Fernandez, . Sol Alonso, Valeria Mesa +1

Aims. We explore galaxies with ringed structures inhabiting poor and rich groups with the aim of assessing the effects of local density environments on ringed galaxy properties. Me…

astro-ph.GA2023★ 59 cited

The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning

Bingjie Wang, Joel Leja, Ivo Labbé +41

The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster Abell 2744 to create the deepest view of our universe to date by leveraging strong…

astro-ph.GA2023★ 32 cited

JWST-TST Proper Motions: I. High-Precision NIRISS Calibration and Large Magellanic Cloud Kinematics

M. Libralato, A. Bellini, R. P. van der Marel +27

We develop and disseminate effective point-spread functions and geometric-distortion solutions for high-precision astrometry and photometry with the JWST NIRISS instrument. We corr…

astro-ph.GA2022★ 19 cited

Webb's PEARLS: Bright 1.5--2.0 micron Dropouts in the Spitzer/IRAC Dark Field

Haojing Yan, Seth H. Cohen, Rogier A. Windhorst +35

Using the first epoch of four-band NIRCam observations obtained by the James Webb Space Telescope (JWST) Prime Extragalactic Areas for Reionization and Lensing Science Program in t…

astro-ph.GA2019★ 15 cited

Hyper Wide Field Imaging of the Local Group Dwarf Irregular Galaxy IC 1613: An Extended Component of Metal-poor Stars

Ragadeepika Pucha, Jeffrey L. Carlin, Beth Willman +10

Stellar halos offer fossil evidence for hierarchical structure formation. Since halo assembly is predicted to be scale-free, stellar halos around low-mass galaxies constrain proper…

astro-ph.GA2019★ 123 cited

The Lazy Giants: APOGEE Abundances Reveal Low Star Formation Efficiencies in the Magellanic Clouds

David L. Nidever, Sten Hasselquist, Christian R. Hayes +28

We report the first APOGEE metallicities and alpha-element abundances measured for 3600 red giant stars spanning a large radial range of both the Large (LMC) and Small Magellanic C…

astro-ph.GA2017★ 26 cited

The not so simple globular cluster Cen. I. Spatial distribution of the multiple stellar populations

A. Calamida, G. Strampelli, A. Rest +8

We present a multi-band photometric catalog of 1.7 million cluster members for a field of view of 2x2 degree across Cen. Photometry is based on images colle…

astro-ph.GA2015★ 26 cited

Oxygen Abundance Measurements of SHIELD Galaxies

Nathalie C. Haurberg, John J. Salzer, John M. Cannon +1

We have derived oxygen abundances for 8 galaxies from the Survey of HI in Extremely Low-mass Dwarfs (SHIELD). The SHIELD survey is an ongoing study of very low-mass galaxies, with…

astro-ph.GA2014★ 39 cited

Two Local Volume Dwarf Galaxies Discovered in 21 cm Emission: Pisces A and B

Erik J. Tollerud, Marla C. Geha, Jana Grcevich +2

We report the discovery of two dwarf galaxies, Pisces A and B, from a blind 21 cm HI search. These were the only two galaxies found via optical imaging and spectroscopy of 22 HI cl…

astro-ph.GA2014★ 30 cited

Evidence from the Very Long Baseline Array that J1502SE/SW are Double Hotspots, not a Supermassive Binary Black Hole

J. M. Wrobel, R. C. Walker, H. Fu

SDSS J150243.09+111557.3 is a merging system at z = 0.39 that hosts two confirmed AGN, one unobscured and one dust-obscured, offset by several kiloparsecs. Deane et al. recently re…

astro-ph.GA2014★ 109 cited

The Sloan Digital Sky Survey Stripe 82 Imaging Data: Depth-Optimized Co-adds Over 300 Deg^2 in Five Filters

Linhua Jiang, Xiaohui Fan, Fuyan Bian +9

We present and release co-added images of the Sloan Digital Sky Survey (SDSS) Stripe 82. Stripe 82 covers an area of 300 deg^2 on the Celestial Equator, and has been repeatedly sca…

astro-ph.GA2014★ 17 cited

The Ultraviolet Attenuation Law in Backlit Spiral Galaxies

William C. Keel, Anna M. Manning, Benne W. Holwerda +2

(Abridged) The effective extinction law (attenuation behavior) in galaxies in the emitted ultraviolet is well known only for actively star-forming objects and combines effects of t…

astro-ph.GA2013★ 80 cited

Kinematics of Outer Halo Globular Clusters in M31

J. Veljanoski, A. M. N. Ferguson, A. D. Mackey +12

We present the first kinematic analysis of the far outer halo globular cluster (GC) population in the Local Group galaxy M31. Our sample contains 53 objects with projected radii of…

astro-ph.GA2012★ 41 cited

The Remarkable High Pressure of the Local Leo Cold Cloud

David M. Meyer, J. T. Lauroesch, J. E. G. Peek +1

Using the Space Telescope Imaging Spectrograph (STIS) onboard the Hubble Space Telescope, we have obtained high-resolution ultraviolet spectra of the C I absorption toward two star…

astro-ph.GA2011★ 61 cited

Kinematics and Chemistry of Stars Along the Sagittarius Trailing Tidal Tail and Constraints on the Milky Way Mass Distribution

Jeffrey L. Carlin, Steven R. Majewski, Dana I. Casetti-Dinescu +3

We present three-dimensional kinematics of Sagittarius (Sgr) trailing tidal debris in six fields located 70-130 degrees along the stream from the Sgr dwarf galaxy core. The data ar…

astro-ph.GA2011★ 31 cited

The Carina Project. IV. radial velocity distribution

M. Fabrizio, M. Nonino, G. Bono +16

We present new and accurate radial velocity (RV) measurements of luminous stars of all ages (old horizontal branch, intermediate--age red clump, and young blue plume, as well as re…

astro-ph.GA2010★ 10 cited

Mapping the Asymmetric Thick Disk: III. The Kinematics and Interaction with the Galactic Bar

Roberta M. Humphreys, Timothy C. Beers, Juan E. Cabanela +4

In the first two papers of this series, Larsen et al (2010a,b) describe our faint CCD survey in the inner Galaxy and map the over-density of Thick Disk stars in Quadrant I (Q1) to…

astro-ph.GA2010★ 9 cited

Near-infrared counterparts of Chandra X-ray sources toward the Galactic Center

Curtis DeWitt, Reba M. Bandyopadhyay, Stephen S. Eikenberry +4

The Chandra X-ray Observatory has now discovered nearly 10,000 X-ray point sources in the 2 x 0.8 degree region around the Galactic Center (Muno 2009). The sources are likely to be…

astro-ph.GA2010★ 10 cited

The Membership and Distance of the Open Cluster Collinder 419

Lewis C. Roberts, Douglas R. Gies, J. Robert Parks +6

The young open cluster Collinder 419 surrounds the massive O star, HD 193322, that is itself a remarkable multiple star system containing at least four components. Here we present…

astro-ph.GA2010★ 123 cited

A Hidden Population of Massive Stars with Circumstellar Shells Discovered with the Spitzer Space Telescope

S. Wachter, J. C. Mauerhan, S. D. Van Dyk +3

We have discovered a large number of circular and elliptical shells at 24 microns around luminous central sources with the MIPS instrument on-board the Spitzer Space Telescope. Our…

astro-ph.GA2010★ 87 cited

SDSS J1254+0846: A Binary Quasar Caught in the Act of Merging

Paul J. Green, Adam D. Myers, Wayne A. Barkhouse +5

We present the first luminous, spatially resolved binary quasar that clearly inhabits an ongoing galaxy merger. SDSS J125455.09+084653.9 and SDSS J125454.87+084652.1 (SDSS J1254+08…

astro-ph.GA2010★ 7 cited

Red Clump Stars in the Sagittarius Tidal Streams

Kenneth Carrell, Ronald Wilhelm, Yuqin Chen

We have probed a section (l ~ 150, b ~ -60) of the trailing tidal arm of the Sagittarius dwarf spheroidal galaxy by identifying a sample of Red Clump stream stars. Red Clump stars…

astro-ph.GA2009★ 20 cited

HST/NICMOS observations of the GLIMPSE9 stellar cluster

Maria Messineo, Donald F. Figer, Ben Davies +4

We present HST/NICMOS photometry, and low-resolution K-band spectra of the GLIMPSE9 stellar cluster. The newly obtained color-magnitude diagram shows a cluster sequence with H-Ks =…

astro-ph.GA2009★ 12 cited

Fabry-Perot Absorption Line Spectroscopy of the Galactic Bar. II. Stellar Metallicities

Naseem Rangwala, T. B. Williams

We measure the Ca II 8542 line strength in 3360 stars along three lines-of-sight in the Galactic bar: (l,b) ~ (+/-5.0,-3.5) and Baade's Window, using Fabry-Perot (FP) absorption li…