output
19922026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2019 · astro-ph.GAShow all

22 papers · 2 filters

astro-ph.GA2019★ 13 cited

Substructure of visibility functions from scattered radio emission of pulsars through space VLBI

M. V. Popov, N. Bartel, M. S. Burgin +3

We report on the substructure of visibility functions in the delay domain of PSRs B0329+54, B0823+26, B0834+06, B1933+16 and B0833-45 (Vela) observed with earth-earth and RadioAstr…

astro-ph.GA2019★ 50 cited

The colors and sizes of recently quenched galaxies: a result of compact starburst before quenching

Po-Feng Wu, Arjen van der Wel, Rachel Bezanson +11

We analyze the colors and sizes of 32 quiescent (UVJ-selected) galaxies with strong Balmer absorption ($\mbox{EW}(Hδ) \geq 4$Å) at drawn from DR2 of the LEGA-C survey to…

astro-ph.GA2019★ 26 cited

HST/WFC3 grism observations of clusters: evidence for evolution in the mass-size relation of quiescent galaxies from poststarburst galaxies

Jasleen Matharu, Adam Muzzin, Gabriel B. Brammer +10

Minor mergers have been proposed as the driving mechanism for the size growth of quiescent galaxies with decreasing redshift. The process whereby large star-forming galaxies quench…

astro-ph.GA2019★ 102 cited

An Extremely Massive Quiescent Galaxy at : Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models

Ben Forrest, Marianna Annunziatella, Gillian Wilson +17

We present spectra of the most massive quiescent galaxy yet discovered at , spectroscopically confirmed via the detection of Balmer absorption features in the and ban…

astro-ph.GA2019★ 31 cited

The dark matter component of the Gaia radially anisotropic substructure

Nassim Bozorgnia, Azadeh Fattahi, Carlos S. Frenk +5

We study the properties of the dark matter component of the radially anisotropic stellar population recently identified in the Gaia data, using magneto-hydrodynamical simulations o…

astro-ph.GA2019★ 40 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Comparison of Lag Measurement Methods with Simulated Observations

Jennifer I-Hsiu Li, Yue Shen, W. N. Brandt +8

We investigate the performance of different methodologies that measure the time lag between broad-line and continuum variations in reverberation mapping data using simulated light…

astro-ph.GA2019★ 39 cited

Detection statistics of the RadioAstron AGN survey

Y. Y. Kovalev, N. S. Kardashev, K. V. Sokolovsky +57

The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightnes…

astro-ph.GA2019★ 31 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Improving Lag Detection with an Extended Multi-Year Baseline

Yue Shen, C. J. Grier, Keith Horne +32

We investigate the effects of extended multi-year light curves (9-year photometry and 5-year spectroscopy) on the detection of time lags between the continuum variability and broad…

astro-ph.GA2019★ 25 cited

Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry

Nicholas S. Martis, Danilo M. Marchesini, Adam Muzzin +5

We investigate the stellar and dust properties of massive (log) and dusty () galaxies at by modeling their spectral energy distri…

astro-ph.GA2019★ 48 cited

Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum

G. A. Kriss, G. De Rosa, J. Ely +164

We model the ultraviolet spectra of the Seyfert 1 galaxy NGC~5548 obtained with the Hubble Space Telescope during the 6-month reverberation-mapping campaign in 2014. Our model of t…

astro-ph.GA2019★ 13 cited

The Rest-frame -band Luminosity Function of Red Sequence Galaxies in Clusters at

Jeffrey C. C. Chan, Gillian Wilson, Gregory Rudnick +22

We present results on the rest-frame -band luminosity functions (LF) of red sequence galaxies in seven clusters at 1.0 < z < 1.3 from the Gemini Observations of Galaxies in Rich…

astro-ph.GA2019★ 46 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar

Jason Dexter, Shuo Xin, Yue Shen +18

We analyze extensive spectroscopic and photometric data of the hypervariable quasar SDSS J131424+530527 (RMID 017) at z=0.456, an optical "changing look" quasar from the Sloan Digi…

astro-ph.GA2019★ 111 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Initial CIV Lag Results from Four Years of Data

C. J. Grier, Yue Shen, Keith Horne +31

We present reverberation-mapping lags and black-hole mass measurements using the CIV 1549 broad emission line from a sample of 349 quasars monitored as a part of the Sloan Digital…

astro-ph.GA2019★ 60 cited

Rejuvenation in quiescent galaxies in LEGA-C

Priscilla Chauke, Arjen van der Wel, Camilla Pacifici +12

We use reconstructed star-formation histories (SFHs) of quiescent galaxies at in the LEGA-C survey to identify secondary star-formation episodes that, after an initial pe…

astro-ph.GA2019★ 14 cited

Multiwavelength radio observations of a Brightest Cluster Galaxy at z=1.71: Detection of a modest Active Galactic Nucleus and evidence for extended star formation

Ariane Trudeau, Tracy Webb, Julie Hlavacek-Larrondo +7

We present deep, multiwavelength radio observations of SpARCS104922.6+564032.5, a z = 1.71 galaxy cluster with a starbusting core. Observations were made with the Karl G. Jansky Ve…

astro-ph.GA2019★ 29 cited

The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS)

Jan-Torge Schindler, Xiaohui Fan, Yun-Hsin Huang +7

We present the results of the Extremely Luminous Quasar Survey in the survey of the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS; PS1). This effort applies…

astro-ph.GA2019★ 22 cited

Variability of Low-ionization Broad Absorption Line Quasars Based on Multi-epoch Spectra from The Sloan Digital Sky Survey

Weimin. Yi, W. N. Brandt, P. B. Hall +5

We present absorption variability results for 134 bona fide \mgii\ broad absorption line (BAL) quasars at 0.46~~2.3 covering days to 10 yr in the rest f…

astro-ph.GA2019★ 76 cited

The evolution of the quenching of star formation in cluster galaxies since z 1

I. Pintos-Castro, H. K. C. Yee, A. Muzzin +2

We study the star-forming (SF) population of galaxies within a sample of 209 IR-selected galaxy clusters at 0.31.1 in the ELAIS-N1 and XMM-LSS fields, exploiting…

astro-ph.GA2019★ 6 cited

Denuded Dwarfs Demystified: Gas Loss from dSph Progenitors and Implications for the Minimum Mass of Galaxies

Nina Ivkovich, Marshall L. McCall

The placement of early-type dwarf galaxies (dSphs and dEs) with respect to the Potential Plane defined by pressure-supported late-type dwarf galaxies (dIs and BCDs) has been determ…

astro-ph.GA2019★ 1 cited

Mapping the Inner Structure of Quasars with Time-Domain Spectroscopy

Yue Shen, Scott Anderson, Edo Berger +40

The ubiquitous variability of quasars across a wide range of wavelengths and timescales encodes critical information about the structure and dynamics of the circumnuclear emitting…

astro-ph.GA2019★ 116 cited

The Brightest Galaxies over the COSMOS UltraVISTA Field

Mauro Stefanon, Ivo Labbé, Rychard J. Bouwens +12

We present 16 new ultrabright galaxy candidates at z~8 identified over the COSMOS/UltraVISTA field. The new search takes advantage of the deepest-available groun…

astro-ph.GA2019★ 19 cited

High Redshift Massive Quiescent Galaxies are as Flat as Star Forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST

Allison R. Hill, Arjen van der Wel, Marijn Franx +5

We investigate the median flattening of galaxies at in all five CANDELS/3D-HST fields via the apparent axis ratio . We separate the sample into bins of redshift, ste…