output
19952026
most citedThe Demography of Massive Dark Objects in Galaxy Centres

4k citations

Showing 2013Show all

68 papers · 1 filter

astro-ph.GA2013★ 176 cited

Evolution of Broad-line Emission from Active Galactic Nuclei

Moshe Elitzur, Luis C. Ho, Jonathan R. Trump

Apart from viewing-dependent obscuration, intrinsic broad-line emission from active galactic nuclei (AGNs) follows an evolutionary sequence: Type …

astro-ph.CO2013★ 112 cited

A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey

Yu Lu, Risa H. Wechsler, Rachel S. Somerville +13

We compare the predictions of three independently developed semi-analytic galaxy formation models that are being used to aid in the interpretation of results from the CANDELS surve…

astro-ph.CO2013★ 69 cited

AGN X-ray variability in the XMM-COSMOS survey

G. Lanzuisi, G. Ponti, M. Salvato +18

We took advantage of the observations carried out by XMM in the COSMOS field during 3.5 years, to study the long term variability of a large sample of AGN (638 sources), in a wide…

astro-ph.CO2013★ 63 cited

Constraints on the merging channel of massive galaxies since z~1

I. Ferreras, I. Trujillo, E. Mármol-Queraltó +8

(Abridged) We probe the merging channel of massive galaxies over the z=0.3-1.3 redshift window by studying close pairs in a sample of 238 galaxies with stellar mass >1E11Msun, from…

astro-ph.CO2013★ 77 cited

The colour distribution of galaxies at redshift five

A. B. Rogers, R. J. McLure, J. S. Dunlop +11

We present the results of a study investigating the rest-frame ultra-violet (UV) spectral slopes of redshift z~5 Lyman-break galaxies (LBGs). By combining deep Hubble Space Telesco…

astro-ph.CO2013★ 29 cited

MOND and IMF variations in early-type galaxies from

C. Tortora, A. J. Romanowsky, V. F. Cardone +2

MOdified Newtonian dynamics (MOND) represents a phenomenological alternative to dark matter (DM) for the missing mass problem in galaxies and clusters of galaxies. We analyze the c…

astro-ph.IM2013★ 18 cited

FIRST, a fibered aperture masking instrument II. Spectroscopy of the Capella binary system at the diffraction limit

E. Huby, G. Duchêne, F. Marchis +7

FIRST is a prototype instrument built to demonstrate the capabilities of the pupil remapping technique, using single-mode fibers and working at visible wavelengths. We report on ob…

astro-ph.CO2013★ 60 cited

Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2

Michael V. Maseda, Arjen van der Wel, Elisabete da Cunha +21

Spectroscopic observations from the Large Binocular Telescope and the Very Large Telescope reveal kinematically narrow lines (~50 km/s) for a sample of 14 Extreme Emission Line Gal…

astro-ph.CO2013★ 255 cited

A CANDELS - 3D-HST Synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5

Stijn Wuyts, Natascha M. Forster Schreiber, Erica J. Nelson +20

We analyze the resolved stellar populations of 473 massive star-forming galaxies at 0.7 < z < 1.5, with multi-wavelength broad-band imaging from CANDELS and Halpha surface brightne…

astro-ph.GA2013★ 19 cited

The Pattern of CN, O, and Na Inhomogeneities on the Red Giant Branch of Messier 5

Graeme H. Smith, Payal N. Modi, Katherine M. Hamren

Data from the literature are used to explore the relation between 3883 CN band strength and the sodium and oxygen abundances of red giants in the globular cluster Messier 5. Alt…

astro-ph.GA2013★ 57 cited

A New Approach to Detailed Structural Decomposition from the SPLASH and PHAT Surveys: Kicked-up Disk Stars in the Andromeda Galaxy?

Claire E. Dorman, Lawrence M. Widrow, Puragra Guhathakurta +7

We characterize the bulge, disk, and halo subcomponents in the Andromeda galaxy (M31) over the radial range 4 < R_proj < 225 kpc. The cospatial nature of these subcomponents render…

astro-ph.CO2013★ 132 cited

The Progenitors of the Compact Early-Type Galaxies at High-Redshift

Christina C. Williams, Mauro Giavalisco, Paolo Cassata +19

We use GOODS and CANDELS images to identify progenitors of massive (log M > 10 Msun) compact "early-type" galaxies (ETGs) at z~1.6. Since merging and accretion increase the size of…

astro-ph.SR2013★ 166 cited

Carbon-enhanced Metal-poor Stars in SDSS/SEGUE. I. Carbon Abundance Estimation and Frequency of CEMP Stars

Young Sun Lee, Timothy C. Beers, Thomas Masseron +8

We describe a method for the determination of stellar [C/Fe] abundance ratios using low-resolution (R = 2000) stellar spectra from the SDSS and SEGUE. By means of a star-by-star co…

astro-ph.CO2013★ 75 cited

The SLUGGS Survey: The globular cluster systems of three early-type galaxies using wide-field imaging

Sreeja S. Kartha, Duncan A. Forbes, Lee R. Spitler +3

We present the results from a wide-field imaging study of globular cluster (GC) systems in three early-type galaxies. Combinations of Subaru/Suprime-Cam, CFHT/MegaCam and HST/WFPC2…

astro-ph.CO2013★ 121 cited

The SLUGGS Survey: Wide-field Stellar Kinematics of Early-type Galaxies

Jacob A. Arnold, Aaron J. Romanowsky, Jean P. Brodie +10

We present stellar kinematics of 22 nearby early-type galaxies (ETGs), based on two-dimensional (2D) absorption line stellar spectroscopy out to ~2-4 R_e (effective radii), as part…

astro-ph.CO2013★ 340 cited

A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey

Molly S. Peeples, Jessica K. Werk, Jason Tumlinson +4

We present a budget and accounting of metals in and around star-forming galaxies at . We combine empirically derived star formation histories with updated supernova and AG…

astro-ph.CO2013★ 67 cited

Towards a Unified Description of the Intergalactic Medium at Redshift z~2.5

J. Xavier Prochaska, Piero Madau, John M. O'Meara +1

We examine recent measurements of the z~2.5 intergalactic medium (IGM) which constrain the HI frequency distribution f(N) and the mean free path MFP to ionizing radiation. We argue…

astro-ph.SR2013★ 323 cited

The Neutron Star Mass Distribution

Bulent Kiziltan, Athanasios Kottas, Maria De Yoreo +1

In recent years, the number of pulsars with secure mass measurements has increased to a level that allows us to probe the underlying neutron star (NS) mass distribution in detail.…

astro-ph.CO2013★ 379 cited

The COS-Halos Survey: Rationale, Design, and A Census of Circumgalactic Neutral Hydrogen

Jason Tumlinson, Christopher Thom, Jessica Werk +11

We present the design and methods of the COS-Halos survey, a systematic investigation of the gaseous halos of 44 z = 0.15-0.35 galaxies using background QSOs observed with the Cosm…

astro-ph.CO2013★ 34 cited

Discovery of a Quadruple Lens in CANDELS with a Record Lens Redshift z=1.53

A. van der Wel, G. van de Ven, M. Maseda +10

Using spectroscopy from the Large Binocular Telescope and imaging from the Hubble Space Telescope we discovered the first strong galaxy lens at z(lens)>1. The lens has a secure pho…

astro-ph.CO2013★ 71 cited

Do We Expect Most AGN to Live in Disks?

Philip F. Hopkins, Dale D. Kocevski, Kevin Bundy

Recent observations have indicated that a large fraction of the low to intermediate luminosity AGN population lives in disk-dominated hosts, while the more luminous quasars live in…

astro-ph.SR2013★ 160 cited

The Role of Stellar Feedback in the Dynamics of HII Regions

Laura A. Lopez, Mark R. Krumholz, Alberto D. Bolatto +3

Stellar feedback is often cited as the biggest uncertainty in galaxy formation models today. This uncertainty stems from a dearth of observational constraints as well as the great…

astro-ph.CO2013★ 51 cited

The SLUGGS Survey: Wide Field Imaging of the Globular Cluster System of NGC 4278

Christopher Usher, Duncan A. Forbes, Lee R. Spitler +4

We use multi-pointing HST ACS and wide field Subaru Suprime-Cam imaging to study the globular cluster system of the L* elliptical galaxy NGC 4278. We have also obtained a handful o…

astro-ph.CO2013★ 84 cited

A near-infrared census of the multi-component stellar structure of early-type dwarf galaxies in the Virgo cluster

J. Janz, E. Laurikainen, T. Lisker +12

The fraction of star-forming to quiescent dwarf galaxies varies from almost infinity in the field to zero in the centers of rich galaxy clusters. What is causing this pronounced mo…