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19912026
Showing 2012 · astro-ph.COShow all

134 papers · 2 filters

astro-ph.CO2012★ 58 cited

Testing Diagnostics of Nuclear Activity and Star Formation in Galaxies at z>1

Jonathan R. Trump, Nicholas P. Konidaris, Guillermo Barro +9

We present some of the first science data with the new Keck/MOSFIRE instrument to test the effectiveness of different AGN/SF diagnostics at z~1.5. MOSFIRE spectra were obtained in…

astro-ph.CO2012★ 26 cited

Multi-Wavelength Study of a Complete IRAC 3.6micron-Selected Galaxy Sample: a Fair Census of Red and Blue Populations at Redshifts 0.4-1

J. -S. Huang, S. M. Faber, C. N. A. Willmer +14

We present a multi-wavelength study of a 3.6 m-selected galaxy sample in the Extended Groth strip. The sample is complete for galaxies with stellar mass \Msun and re…

astro-ph.CO2012★ 371 cited

The COS-Halos Survey: An Empirical Description of the Metal-Line Absorption in the Low-Redshift Circumgalactic Medium

Jessica Werk, J. Xavier Prochaska, Christopher Thom +4

We present the equivalent width and column density measurements for low and intermediate ionization states of the circumgalactic medium (CGM) surrounding 44 low-z, L ~ L* galaxies…

astro-ph.CO2012★ 39 cited

A Census of Broad-Line Active Galactic Nuclei in Nearby Galaxies: Coeval Star Formation and Rapid Black Hole Growth

Jonathan R. Trump, Alexander D. Hsu, Jerome J. Fang +3

We present the first quantified, statistical map of broad-line active galactic nucleus (AGN) frequency with host galaxy color and stellar mass in nearby (0.01 < z < 0.11) galaxies.…

astro-ph.CO2012★ 6 cited

Testing the dark matter origin of the WMAP-Planck Haze with radio observations of Spiral Galaxies

Eric Carlson, Dan Hooper, Tim Linden +1

If the Galactic WMAP radio haze, as recently confirmed by Planck, is produced by dark matter annihilation or decay, similar diffuse radio halos should exist around other galaxies w…

astro-ph.CO2012★ 18 cited

An Independent Measurement of the Incidence of MgII Absorbers along Gamma-Ray Burst Sightlines: the End of the Mystery?

A. Cucchiara, J. X. Prochaska, G. Zhu +15

In 2006, Prochter et al. reported a statistically significant enhancement of very strong Mg II absorption systems intervening the sightlines to gamma-ray bursts (GRBs) relative to…

astro-ph.CO2012★ 96 cited

A Substantial Mass of Cool, Metal-Enriched Gas Surrounding the Progenitors of Modern-Day Ellipticals

J. Xavier Prochaska, Joseph F. Hennawi, Robert A. Simcoe

The hosts of luminous z~2 quasars evolve into today's massive elliptical galaxies. Current theories predict that the circum-galactic medium (CGM) of these massive, dark-matter halo…

astro-ph.CO2012★ 39 cited

Shape Evolution of Massive Early-Type Galaxies: Confirmation of Increased Disk Prevalence at z>1

Yu-Yen Chang, Arjen van der Wel, Hans-Walter Rix +4

We use high-resolution K-band VLT/HAWK-I imaging over 0.25 square degrees to study the structural evolution of massive early-type galaxies since z~1. Mass-selected samples, complet…

astro-ph.CO2012★ 85 cited

Pseudobulge Formation as a Dynamical Rather than a Secular Process

Javiera Guedes, Lucio Mayer, Marcella Carollo +1

We investigate the formation and evolution of the pseudobulge in "Eris", a high-resolution N-body + smoothed particle hydrodynamics (SPH) cosmological simulation that successfully…

astro-ph.CO2012★ 273 cited

The Imprint of The Extragalactic Background Light in the Gamma-Ray Spectra of Blazars

LAT Collaboration

The light emitted by stars and accreting compact objects through the history of the Universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of t…

astro-ph.CO2012★ 16 cited

Characterizing the satellites of massive galaxies up to z~2: young populations to build the outskirts of nearby massive galaxies

Esther Marmol-Queralto, Ignacio Trujillo, Victor Villar +2

The accretion of minor satellites is currently proposed as the most likely mechanism to explain the significant size evolution of the massive galaxies during the last ~10 Gyr. In t…

astro-ph.CO2012★ 62 cited

A Rest-frame Optical View on z~4 Galaxies I: Color and Age Distributions from Deep IRAC Photometry of the IUDF10 and GOODS Surveys

P. A. Oesch, I. Labbe, R. J. Bouwens +7

We present a study of rest-frame UV-to-optical color distributions for z~4 galaxies based on the combination of deep HST/ACS+WFC3/IR data with Spitzer/IRAC imaging. In particular,…

astro-ph.CO2012★ 545 cited

Structural Parameters of Galaxies in CANDELS

A. van der Wel, E. F. Bell, B. Haussler +19

We present global structural parameter measurements of 109,533 unique, H_F160W-selected objects from the CANDELS multi-cycle treasury program. Sersic model fits for these objects a…

astro-ph.CO2012★ 117 cited

Widespread and Hidden Active Galactic Nuclei in Star-Forming Galaxies at Redshift > 0.3

Stéphanie Juneau, Mark Dickinson, Frédéric Bournaud +23

We characterize the incidence of active galactic nuclei (AGNs) is 0.3 < z < 1 star-forming galaxies by applying multi-wavelength AGN diagnostics (X-ray, optical, mid-infrared, radi…

astro-ph.CO2012★ 100 cited

Finding the First Cosmic Explosions I: Pair-Instability Supernovae

Daniel J. Whalen, Wesley Even, Lucille H. Frey +9

The first stars are the key to the formation of primitive galaxies, early cosmological reionization and chemical enrichment, and the origin of supermassive black holes. Unfortunate…

astro-ph.CO2012★ 62 cited

Photometric Constraints on the Redshift of z~10 candidate UDFj-39546284 from deeper WFC3/IR+ACS+IRAC observations over the HUDF

R. J. Bouwens, P. A. Oesch, G. D. Illingworth +10

Ultra-deep WFC3/IR observations on the HUDF from the HUDF09 program revealed just one plausible z~10 candidate UDFj-39546284. UDFj-39546284 had all the properties expected of a gal…

astro-ph.CO2012★ 16 cited

The explosion energy of early stellar populations: The Fe-peak element ratios in low metallicity damped Lyman-alpha systems

Ryan Cooke, Max Pettini, Regina A. Jorgenson +3

The relative abundances of the Fe-peak elements (Ti-Zn) at the lowest metallicities are intimately linked to the physics of core-collapse supernova explosions. With a sample of 25…

astro-ph.CO2012★ 192 cited

A Census of Star-Forming Galaxies in the z~9-10 Universe based on HST+Spitzer Observations Over 19 CLASH clusters: Three Candidate z~9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at z~9

R. Bouwens, L. Bradley, A. Zitrin +34

We utilise a two-color Lyman-Break selection criterion to search for z~9-10 galaxies over the first 19 clusters in the CLASH program. A systematic search yields three z~9-10 candid…

astro-ph.CO2012★ 55 cited

The effect of models of the interstellar media on the central mass distribution of galaxies

Charlotte Christensen, Fabio Governato, Thomas Quinn +5

We compare the central mass distribution of galaxies simulated with three different models of the interstellar medium (ISM) with increasing complexity: primordial (H+He) cooling do…

astro-ph.CO2012★ 1 cited

Addressing Decadal Survey Science through Community Access to Highly Multiplexed Spectroscopy with BigBOSS on the KPNO Mayall Telescope

Caty Pilachowski, Carles Badenes, Stephen Bailey +87

This document summarizes the results of a community-based discussion of the potential science impact of the Mayall+BigBOSS highly multiplexed multi-object spectroscopic capability.…

astro-ph.CO2012★ 49 cited

Formation and evolution of dwarf early-type galaxies in the Virgo cluster II. Kinematic Scaling Relations

E. Toloba, A. Boselli, R. Peletier +3

We place our sample of 18 Virgo dwarf early-type galaxies (dEs) on the V-K - velocity dispersion, Faber-Jackson, and Fundamental Plane (FP) scaling relations for massive early-type…

astro-ph.CO2012★ 73 cited

The Slow Death (or Rebirth?) of Extended Star Formation in z~0.1 Green Valley Early-Type Galaxies

Jerome J. Fang, S. M. Faber, Samir Salim +2

UV observations in the local universe have uncovered a population of early-type galaxies with UV flux consistent with low-level recent or ongoing star formation. We present resolve…

astro-ph.CO2012★ 106 cited

The X-ray Star Formation Story as Told by Lyman Break Galaxies in the 4 Ms CDF-S

Antara R. Basu-Zych, Bret D. Lehmer, Ann E. Hornschemeier +12

We present results from deep X-ray stacking of >4000 high redshift galaxies from z~1 to 8 using the 4 Ms Chandra Deep Field South (CDF-S) data, the deepest X-ray survey of the extr…

astro-ph.CO2012★ 51 cited

Constraints on Dark Matter Annihilation in Clusters of Galaxies from Diffuse Radio Emission

Emma Storm, Tesla E. Jeltema, Stefano Profumo +1

Annihilation of dark matter can result in the production of stable Standard Model particles including electrons and positrons that, in the presence of magnetic fields, lose energy…