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 2017 · astro-ph.GAShow all

30 papers · 2 filters

astro-ph.GA2017★ 13 cited

The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS

C. Balland, F. Cellier-Holzem, C. Lidman +24

We aim to present 70 spectra of 68 new high-redshift type Ia supernovae (SNeIa) measured at ESO's VLT during the final two years of operation (2006-2008) of the Supernova Legacy Su…

astro-ph.GA2017★ 157 cited

Kiloparsec-scale gaseous clumps and star formation at

S. Carniani, R. Maiolino, R. Amorin +13

We investigate the morphology of the [CII] emission in a sample of "normal" star-forming galaxies at in relation to their UV (rest-frame) counterpart. We use new ALMA obs…

astro-ph.GA2017★ 123 cited

Slicing COSMOS with SC4K: the evolution of typical Lya emitters and the Lya escape fraction from z~2 to z~6

David Sobral, Sérgio Santos, Jorryt Matthee +4

We present and explore deep narrow- and medium-band data obtained with the Subaru and the Isaac Newton telescopes in the ~2 deg COSMOS field. We use these data as an extremely…

astro-ph.GA2017★ 12 cited

Bulgeless galaxies in the COSMOS field: environment and star formation evolution at

M. Grossi, C. A. C. Fernandes, D. Sobral +5

Combining the catalogue of galaxy morphologies in the COSMOS field and the sample of H emitters at redshifts and of the HiZELS survey, we selected 220 st…

astro-ph.GA2017★ 19 cited

The KMOS Cluster Survey (KCS) III: fundamental plane of cluster galaxies at in JKCS 041

Laura J. Prichard, Roger L. Davies, Alessandra Beifiori +12

We present data for 16 galaxies in the overdensity JKCS 041 at as part of the K-band Multi-Object Spectrograph (KMOS) Cluster Survey (KCS). With 20-hour integration…

astro-ph.GA2017★ 60 cited

On the nature and physical conditions of the luminous Lya emitter CR7 and its rest-frame UV components

David Sobral, Jorryt Matthee, Gabriel Brammer +6

We present new HST/WFC3 observations and re-analyse VLT data to unveil the continuum, variability and rest-frame UV lines of the multiple UV clumps of the most luminous Ly emitt…

astro-ph.GA2017★ 21 cited

The interstellar medium in [OIII]-selected star-forming galaxies at

Tomoko L. Suzuki, Tadayuki Kodama, Masato Onodera +11

We present new results from near-infrared spectroscopy with Keck/MOSFIRE of [OIII]-selected galaxies at . With our and -band spectra, we investigate the interstell…

astro-ph.GA2017★ 104 cited

ALMA reveals metals yet no dust within multiple components in CR7

J. Matthee, D. Sobral, F. Boone +8

We present spectroscopic follow-up observations of CR7 with ALMA, targeted at constraining the infrared (IR) continuum and [CII] line-emission at high spatial resolu…

astro-ph.GA2017★ 65 cited

On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6

Ana Paulino-Afonso, David Sobral, Bruno Ribeiro +8

We investigate the rest-frame UV morphologies of a large sample of Lyman-a emitters (LAEs) from z~2 to z~6, selected in a uniform way with 16 different narrow- and medium-bands ove…

astro-ph.GA2017★ 35 cited

Stellar Dynamics and Star-Formation Histories of z 1 Radio-loud Galaxies

Ivana Barišić, Arjen van der Wel, Rachel Bezanson +18

We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L 10 W Hz ) at 0.6 < z < 1. This s…

astro-ph.GA2017★ 10 cited

Spectroscopic confirmation of the low-latitude object FSR 1716 as an old globular cluster

Andreas Koch, Andrea Kunder, Jennifer Wojno

Star clusters are invaluable tracers of the Galactic components and the discovery and characterization of low-mass stellar systems can be used to appraise their prevailing disrupti…

astro-ph.GA2017★ 24 cited

The Evolutionary Sequence of Post-Starburst Galaxies

C. L. Wilkinson, K. A. Pimbblet, J. P. Stott

There are multiple ways in which to select post-starburst galaxies in the literature. In this work, we present a study into how two well-used selection techniques have consequences…

astro-ph.GA2017★ 17 cited

Detection of magnetized quark-nuggets, a candidate for dark matter

J. Pace VanDevender, Aaron P. VanDevender, T. Sloan +7

Quark nuggets are theoretical objects composed of approximately equal numbers of up, down, and strange quarks and are also called strangelets and nuclearites. They have been propos…

astro-ph.GA2017★ 45 cited

The KMOS Cluster Survey (KCS) I: The fundamental plane and the formation ages of cluster galaxies at redshift

Alessandra Beifiori, J. Trevor Mendel, Jeffrey C. C. Chan +13

We present the analysis of the fundamental plane (FP) for a sample of 19 massive red-sequence galaxies () in 3 known overdensities at $1.39<z<1…

astro-ph.GA2017★ 30 cited

The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22

David Rubin, Brian Hayden, Xiaosheng Huang +32

We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very L…

astro-ph.GA2017★ 114 cited

The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disk turbulence in z~0.9 star-forming galaxies

H. L. Johnson, C. M. Harrison, A. M. Swinbank +27

We analyse the velocity dispersion properties of 472 z~0.9 star-forming galaxies observed as part of the KMOS Redshift One Spectroscopic Survey (KROSS). The majority of this sample…

astro-ph.GA2017★ 50 cited

The binary fraction of stars in dwarf galaxies: the case of Leo II

Meghin Spencer, Mario Mateo, Matthew Walker +4

We combine precision radial velocity data from four different published works of the stars in the Leo II dwarf spheroidal galaxy. This yields a dataset that spans 19 years, has 14…

astro-ph.GA2017★ 108 cited

Dependence of Type Ia supernova luminosities on their local environment

Matthieu Roman, Delphine Hardin, Marc Betoule +18

We present a fully consistent catalog of local and global properties of host galaxies of 882 Type Ia supernovæ (SNIa) that were selected based on their light-curve properties, span…

astro-ph.GA2017★ 83 cited

Spectroscopic properties of luminous Lyman-α emitters at and comparison to the Lyman-break population

Jorryt Matthee, David Sobral, Behnam Darvish +5

We present spectroscopic follow-up of candidate luminous Ly emitters (LAEs) at in the SA22 field with VLT/X-SHOOTER. We confirm two new luminous LAEs at (S…

astro-ph.GA2017★ 23 cited

The clustering of H+[OIII] and [OII] emitters since : dependencies with line luminosity and stellar mass

Ali Ahmad Khostovan, David Sobral, Bahram Mobasher +7

We investigate the clustering properties of H+[OIII] and [OII] narrowband-selected emitters at from the High- Emission Line Survey. We find clu…

astro-ph.GA2017★ 118 cited

The KMOS Deep Survey (KDS) I: dynamical measurements of typical star-forming galaxies at z 3.5

O. J. Turner, M. Cirasuolo, C. M. Harrison +7

We present dynamical measurements from the KMOS (K-band Multi-Object Spectrograph) Deep Survey (KDS), which is comprised of 77 typical star-forming galaxies at z 3.5 in th…

astro-ph.GA2017★ 44 cited

The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS

R. K. Cochrane, P. N Best, D. Sobral +4

We present clustering analyses of identically-selected star-forming galaxies in 3 narrow redshift slices (at z=0.8, z=1.47 and z=2.23), from HiZELS, a deep, near-infrared narrow-ba…

astro-ph.GA2017★ 10 cited

A deg blind survey for CII], CIII] and CIV at . II: luminosity functions and cosmic average line ratios

Andra Stroe, David Sobral, Jorryt Matthee +2

Recently, the CIII] and CIV emission lines have been observed in galaxies in the early Universe (), providing new ways to measure their redshift and study their stellar popula…

astro-ph.GA2017★ 12 cited

Galactic Pal-eontology: Abundance Analysis of the Disrupting Globular Cluster Palomar 5

Andreas Koch, Patrick Côté

We present a chemical abundance analysis of the tidally disrupted globular cluster (GC) Palomar 5. By co-adding high-resolution spectra of 15 member stars from the cluster's main b…