output
19932026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2018 · astro-ph.GAShow all

56 papers · 2 filters

astro-ph.GA2018★ 26 cited

Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9

L. Rodríguez-Muñoz, G. Rodighiero, C. Mancini +21

We quantify the star formation (SF) in the inner cores (/0.3) of 24 massive galaxy clusters at 0.20.9 observed by the …

astro-ph.GA2018★ 101 cited

The FMOS-COSMOS survey of star-forming galaxies at VI: Redshift and emission-line catalog and basic properties of star-forming galaxies

Daichi Kashino, John D. Silverman, David Sanders +12

We present a new data release from the Fiber Multi-Object Spectrograph (FMOS)-COSMOS survey, which contains the measurements of spectroscopic redshift and flux of rest-frame optica…

astro-ph.GA2018★ 16 cited

Possible Evidence of the Radio AGN Quenching of Neighboring Galaxies at z 1

Lu Shen, Adam R. Tomczak, Brian C. Lemaux +9

Using 57 Radio Active Galactic nuclei (RAGN) at 0.55 z 1.3 drawn from five fields of the Observations of Redshift Evolution in Large Scale Environments (ORELSE) surve…

astro-ph.GA2018★ 41 cited

Conditional Quenching: A detailed look at the SFR-Density Relation at z ~ 0.9 from ORELSE

Adam R. Tomczak, Brian C. Lemaux, Lori M. Lubin +10

We present a study of the star-formation rate (SFR)-density relation at z ~ 0.9 using data drawn from the Observations of Redshift Evolution in Large Scale Environments (ORELSE) su…

astro-ph.GA2018★ 9 cited

Multi-band Optical and Near-infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections

Pallavi Patil, Kristina Nyland, Mark Lacy +4

We present a catalog of 26 faint submillimeter galaxies (SMGs) in the XMM-LSS field identified by cross-matching serendipitously detected sources in archival ALMA Band 6 and 7 data…

astro-ph.GA2018★ 35 cited

The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE

Mathilde Jauzac, Guillaume Mahler, Alastair C. Edge +11

We present a multi-wavelength analysis of the core of the massive galaxy cluster MACS\,J0417.5-1154 (; MACS\;J0417). Our analysis takes advantage of VLT/MUSE observation…

astro-ph.GA2018★ 65 cited

Persistence of the Color-Density Relation and Efficient Environmental Quenching to

Brian C. Lemaux, Adam R. Tomczak, Lori M. Lubin +10

Using ~5000 spectroscopically-confirmed galaxies drawn from the Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey we investigate the relationship betwe…

astro-ph.GA2018★ 3 cited

PS1-13cbe: The Rapid "Turn on" of a Seyfert 1

Reza Katebi, Ryan Chornock, Edo Berger +11

We present a nuclear transient event, PS1-13cbe, that was first discovered in the Pan-STARRS1 survey in 2013. The outburst occurred in the nucleus of the galaxy SDSS J222153.87+003…

astro-ph.GA2018★ 123 cited

A Survey of Atomic Carbon [C I] in High-redshift Main-Sequence Galaxies

F. Valentino, G. E. Magdis, E. Daddi +15

We present the first results of an ALMA survey of the lower fine structure line of atomic carbon [C I] in far infrared-selected galaxies on the main sequence a…

astro-ph.GA2018★ 18 cited

Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES

Andrew G. Barr, Adwin Boogert, Curtis N. DeWitt +8

We have performed a 5-8 m spectral line survey of the hot molecular core associated with the massive protostar AFGL 2591, using the Echelon-Cross-Echelle Spectrograph (EXES) on…

astro-ph.GA2018★ 24 cited

An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S

A. Schulze, J. D. Silverman, D. Kashino +13

We present near-IR spectroscopy in J- and H-band for a large sample of 243 X-ray selected moderate-luminosity type-1 AGN in the COSMOS, SXDS and E-CDF-S survey fields using the mul…

astro-ph.GA2018★ 50 cited

C-GOALS II. Chandra Observations of the Lower Luminosity Sample of Nearby Luminous Infrared Galaxies in GOALS

N. Torres-Albà, K. Iwasawa, T. Díaz-Santos +14

We analyze Chandra X-ray observatory data for a sample of 63 luminous infrared galaxies (LIRGs), sampling the lower-infrared luminosity range of the Great Observatories All-Sky LIR…

astro-ph.GA2018★ 15 cited

The White Dwarf Luminosity Functions from the Pan-STARRS 1 3π Steradian Survey

Marco C. Lam, Nigel C. Hambly, Nicholas Rowell +9

A large sample of white dwarfs is selected by both proper motion and colours from the Pan-STARRS 1 3π Steradian Survey Processing Version 2 to construct the White Dwarf Luminosity…

astro-ph.GA2018★ 54 cited

The molecular gas content and fuel efficiency of starbursts at z ~ 1.6 with ALMA

J. Silverman, W. Rujopakarn, E. Daddi +17

We present an analysis of the molecular gas properties, based on CO(2 - 1) emission, of twelve starburst galaxies at z~1.6 selected by having a boost (>~4x) in their star formation…

astro-ph.GA2018

Quantitative Spectroscopy of the Young Stellar Population in Star Forming Galaxies

Rolf Kudritzki, Miguel A. Urbaneja

The determination of chemical composition is crucial for investigating the formation and evolution of star forming galaxies and provides a powerful tool to constrain the effects of…

astro-ph.GA2018★ 40 cited

The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN

J. S. Brown, K. Z. Stanek, T. W. -S. Holoien +10

We analyze the 476 SN Ia host galaxies from the All-Sky Automated Survey for Supernova (ASAS-SN) Bright Supernova Catalogs to determine the observed relative Type Ia supernova (SN)…

astro-ph.GA2018★ 7 cited

VALES V: A kinematic analysis of the molecular gas content in -ATLAS galaxies at using ALMA

J. Molina, Edo Ibar, V. Villanueva +19

We present Atacama Large Millimeter/submillimeter Array (ALMA) resolved observations of molecular gas in galaxies up to to characterise the role of global galactic dynamic…

astro-ph.GA2018★ 87 cited

X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field

Dale D. Kocevski, Guenther Hasinger, Murray Brightman +25

We present the X-UDS survey, a set of wide and deep Chandra observations of the Subaru-XMM Deep/UKIDSS Ultra Deep Survey (SXDS/UDS) field. The survey consists of 25 observations th…

astro-ph.GA2018★ 12 cited

On the multiplicity of ALMA Compact Array counterparts of far-infrared bright quasars

E. Hatziminaoglou, D. Farrah, E. Humphreys +5

We present ALMA Atacama Compact Array (ACA) 870 micron continuum maps of 28 infrared-bright SDSS quasars with Herschel/SPIRE detections at redshifts 2-4, the largest such sample ev…

astro-ph.GA2018★ 114 cited

HELP: modelling the spectral energy distributions of Herschel detected galaxies in the ELAIS N1 field

K. Malek, V. Buat, Y. Roehlly +10

The HELP project focuses on the data from ESA's Herschel mission, which covered over 1300 and is preparing to publish a multi-wavelength catalogue of millions of objects. Ou…

astro-ph.GA2018★ 101 cited

Velocity-resolved reverberation mapping of five bright Seyfert 1 galaxies

G. De Rosa, M. M. Fausnaugh, C. J. Grier +99

We present the first results from a reverberation-mapping campaign undertaken during the first half of 2012, with additional data on one AGN (NGC 3227) from a 2014 campaign. Our ma…

astro-ph.GA2018★ 102 cited

The Unusual Initial Mass Function of the Arches Cluster

M. W. Hosek, J. R. Lu, J. Anderson +5

As a young massive cluster in the Central Molecular Zone, the Arches cluster is a valuable probe of the stellar Initial Mass Function (IMF) in the extreme Galactic Center environme…

astro-ph.GA2018★ 38 cited

Mid-Infrared Spectroscopic Evidence for AGN Heating Warm Molecular Gas

Erini L. Lambrides, Andreea O. Petric, Kirill Tchernyshyov +2

We analyse 2,015 mid-infrared (MIR) spectra of galaxies observed with Spitzer's Infrared Spectrograph, including objects with growing super-massive black holes and objects where mo…

astro-ph.GA2018★ 6 cited

Cosmic happenstance: 24-m selected, multi-component Herschel sources are line-of-sight projections

Jillian M. Scudder, Seb Oliver, Peter D. Hurley +3

In this paper, we investigate the physical associations between blended far-infrared (FIR)-emitting galaxies, in order to identify the level of line-of-sight projection contaminati…