10.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR2k papers
- University of ManchesterGB1.8k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1.8k papers
- University of MichiganUS1.7k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.7k papers
- Charles UniversityCZ1.7k papers
- Brookhaven National LaboratoryUS1.6k papers
- Stony Brook UniversityUS1.6k papers
- University of WashingtonUS1.6k papers
- Michigan State UniversityUS1.6k papers
- Ludwig-Maximilians-Universität MünchenDE1.6k papers
- The University of Texas at ArlingtonUS1.6k papers
26 papers · 2 filters
The First Integral Field Unit Spectroscopic View of Shocked Cluster Galaxies
Andra Stroe, Maryam Hussaini, Bernd Husemann +2
Galaxy clusters grow by merging with other clusters, giving rise to Mpc-wide shock waves that travel at 1000-2500 km/s through the intra-cluster medium. To study the effects of mer…
Dust, gas, and metal content in star-forming galaxies at revealed with ALMA and Near-IR spectroscopy
Tomoko L. Suzuki, Masato Onodera, Tadayuki Kodama +8
We conducted sub-millimeter observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) of star-forming galaxies at , whose gas-phase metallicities have be…
A kpc-scale resolved study of unobscured and obscured star-formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS
Cheng Cheng, Edo Ibar, Ian Smail +12
We present Atacama Large Millimeter/Submillimeter Array (ALMA) continuum observations of a sample of nine star-forming galaxies at redshifts 1.47 and 2.23 selected from the High-$z…
Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo
Vihang Mehta, Claudia Scarlata, Lucy Fortson +7
Giant, star-forming clumps are a common feature prevalent amongst high-redshift star-forming galaxies and play a critical role in shaping their chaotic morphologies and yet, their…
Tightly coupled morpho-kinematic evolution for massive star-forming and quiescent galaxies across 7 Gyr of cosmic time
Anna de Graaff, Rachel Bezanson, Marijn Franx +11
We use the Fundamental Plane (FP) to measure the redshift evolution of the dynamical mass-to-light ratio () and the dynamical-to-stellar mass ratio ($M_{\mathrm…
An ALMA survey of the S2CLS UDS field: Optically invisible submillimetre galaxies
Ian Smail, U. Dudzevičiūtė, S. M. Stach +16
We analyse a robust sample of 30 near-infrared-faint (K>25.3, 5 sigma) submillimetre galaxies selected across a 0.96 deg^2 field, to investigate their properties and the cause of t…
Dust Attenuation Curves at z 0.8 from LEGA-C: Precise Constraints on the Slope and 2175 Bump Strength
Ivana Barisic, Camila Pacifici, Arjen van der Wel +11
We present a novel approach to measure the attenuation curves of 485 individual star-forming galaxies with M 10 M based on deep optical spectra from the VL…
The clustering of submillimeter galaxies detected with ALMA
Cristina Garcia-Vergara, Jacqueline Hodge, Joseph F. Hennawi +4
Previous studies measuring the clustering of submillimeter galaxies (SMGs) have based their measurements on single-dish detected sources, finding evidence for strong clustering. Ho…
The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at
S. Gillman, A. L. Tiley, A. M. Swinbank +10
We present an analysis of the chemical abundance properties of 650 star-forming galaxies at . Using integral-field observations from the -band Multi-O…
An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
H. S. B. Algera, I. Smail, U. Dudzevičiūtė +17
We study the radio properties of 706 sub-millimeter galaxies (SMGs) selected at 870m with the Atacama Large Millimeter Array from the SCUBA-2 Cosmology Legacy Survey map of the…
An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies
Jack E. Birkin, Axel Weiss, J. L. Wardlow +18
We present a survey of the molecular gas in 61 submillimetre galaxies (SMGs) selected from 870m continuum surveys of the COSMOS, UDS and ECDFS fields, using the Atacama Large Mi…
The nature of CR7 revealed with MUSE: a young starburst powering extended Lyman- emission at z=6.6
Jorryt Matthee, Gabriele Pezzulli, Ruari Mackenzie +11
CR7 is among the most luminous Lyman- emitters (LAEs) known at and consists of at least three UV components that are surrounded by Lyman- (Ly) emission. Previous…
Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
Francesco D'Eugenio, Arjen van der Wel, Po-Feng Wu +13
We use deep, spatially resolved spectroscopy from the LEGA-C Survey to study radial variations in the stellar population of 17 spectroscopically-selected post-starburst (PSB) galax…
J-PLUS: Unveiling the brightest-end of the Lyα luminosity function at 2.0<z<3.3 over 1000 deg^2
Daniele Spinoso, Alvaro Orsi, Carlos López-Sanjuan +21
We present the photometric determination of the bright-end (L_Lya>10^43.5 erg/s) of the Lya luminosity function (LF) within four redshifts windows in the interval 2.2<z<3.3. Our wo…
K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
Sam P. Vaughan, Alfred L. Tiley, Roger L. Davies +8
Galaxy clusters have long been theorised to quench the star-formation of their members. This study uses integral-field unit observations from the -band Multi-Object Spectrograph…
Quasar Sightline and Galaxy Evolution (QSAGE) survey -- II. Galaxy overdensities around UV luminous quasars at z=1-2
J. P. Stott, R. M. Bielby, F. Cullen +8
We demonstrate that the UV brightest quasars at z=1-2 live in overdense environments. This is based on an analysis of deep Hubble Space Telescope WFC3 G141 grism spectroscopy of th…
K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at -
Alfred L. Tiley, Sam P. Vaughan, John P. Stott +10
We present the KMOS-CLASH (K-CLASH) survey, a K-band Multi-Object Spectrograph (KMOS) survey of the spatially-resolved gas properties and kinematics of 191 (predominantly blue) H$α…
See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies
S. C. Williams, I. M. Hook, B. Hayden +9
The Supernova Cosmology Project has conducted the `See Change' programme, aimed at discovering and observing high-redshift (1.13 z 1.75) Type Ia supernovae (SNe Ia).…
Differences and similarities of stellar populations in LAEs and LBGs at 3.4 - 6.8
P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón +6
The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burs…
Emergence of an Ultra-Red Ultra-Massive Galaxy Cluster Core at
Arianna S. Long, Asantha Cooray, Jingzhe Ma +6
Recent simulations and observations of massive galaxy cluster evolution predict that the majority of stellar mass build up happens within cluster members by , before cluster v…
Extended H over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at
Chian-Chou Chen, C. M. Harrison, I. Smail +15
Using data from ALMA and near-infrared (NIR) integral field spectrographs including both SINFONI and KMOS on the VLT, we investigate the two-dimensional distributions of H and r…
Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2
Behnam Darvish, Nick Z. Scoville, Christopher Martin +17
We report the spectroscopic confirmation of a new protocluster in the COSMOS field at 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity of narrowb…
Stellar Kinematics and Environment at z~0.8 in the LEGA-C Survey: Massive, Slow-Rotators are Built First in Overdense Environments
Justin Cole, Rachel Bezanson, Arjen van der Wel +11
In this letter, we investigate the impact of environment on integrated and spatially-resolved stellar kinematics of a sample of massive, quiescent galaxies at intermediate redshift…
Galactic Conformity in both Star-formation and Morphological Properties
Justin A. Otter, Karen L. Masters, Brooke Simmons +1
We investigate one-halo galactic conformity (the tendency for satellite galaxies to mirror the properties of their central) in both star-formation and morphology using a sample of…