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20092026
most citedInferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey

244 citations · 4.5k across the 87 of their papers we have counts for

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20 papers · 1 filter

astro-ph.CO2019★ 12 cited

The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation

R. Thomas, L. Pentericci, O. Le Fèvre +22

Aims. Our aim is to estimate the intergalactic medium transmission towards UV-selected star-forming galaxies at redshift 4 and above and study the effect of the dust attenuation on…

astro-ph.CO2019★ 244 cited

Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey

Charlotte A. Mason, Adriano Fontana, Tommaso Treu +12

Detections and non-detections of Lyman alpha (Ly) emission from galaxies ( Gyr after the Big Bang) can be used to measure the timeline of cosmic reionization. Of key i…

astro-ph.CO2013★ 39 cited

To Stack or Not to Stack: Spectral Energy Distribution Properties of Lya-Emitting Galaxies at z=2.1

Carlos J. Vargas, Hannah Bish, Viviana Acquaviva +13

We use the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) GOODS-S multi-wavelength catalog to identify counterparts for 20 Lya Emitting (LAE) galaxies at…

astro-ph.CO2013★ 143 cited

The Lyman alpha Reference Sample: II. HST imaging results, integrated properties and trends

Matthew Hayes, Göran Östlin, Florent Duval +16

We report upon new results regarding the Lya output of galaxies, derived from the Lyman alpha Reference Sample (LARS), focusing on Hubble Space Telescope imaging. For 14 galaxies w…

astro-ph.CO2013★ 134 cited

The Lyman alpha Reference Sample: Extended Lyman alpha Halos Produced at Low Dust Content

Matthew Hayes, Göran Östlin, Daniel Schaerer +14

We report on new imaging observations of the Lyman alpha emission line (Lya), performed with the Hubble Space Telescope, that comprise the backbone of the Lyman alpha Reference Sam…

astro-ph.CO2013★ 55 cited

High resolution study of the cluster complexes in a lensed spiral at redshift ~1.5; constraints on the bulge formation and disk evolution

Angela Adamo, Goeran Ostlin, Nate Bastian +3

We analyse the clump population of the spiral galaxy Sp 1149 at redshift 1.5. Located behind the galaxy cluster MACS J1149.5+2223, Sp 1149 has been significantly magnified allowing…

astro-ph.CO2013★ 28 cited

Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star forming galaxies at 2<z<3

Lucia Guaita, Harold Francke, Eric Gawiser +4

To investigate the ingredients, which allow star-forming galaxies to present Lyalpha line in emission, we studied the kinematics and gas phase metallicity (Z) of the interstellar m…

astro-ph.CO2013★ 56 cited

Searching for Neutral Hydrogen Halos around z ~ 2.1 and z ~ 3.1 Ly-alpha Emitting Galaxies

John Feldmeier, Alex Hagen, Robin Ciardullo +9

We search for evidence of diffuse Ly-alpha emission from extended neutral hydrogen surrounding Ly-alpha emitting galaxies (LAEs) using deep narrow-band images of the Extended Chand…

astro-ph.CO2012★ 50 cited

Detecting gravitationally lensed population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope

E. Zackrisson, A. Zitrin, M. Trenti +6

Small galaxies consisting entirely of population III (pop III) stars may form at high redshifts, and could constitute one of the best probes of such stars. Here, we explore the pro…

astro-ph.CO2012★ 40 cited

Stacked Rest-Frame UV Spectra of Ly-Emitting and Continuum-Selected Galaxies at 2<z<3.5

Michael Berry, Eric Gawiser, Lucia Guaita +6

We present properties of individual and composite rest-UV spectra of continuum- and narrowband-selected star-forming galaxies (SFGs) at a redshift of 2<z<3.5 discovered by the MUSY…

astro-ph.CO2011★ 21 cited

The Curious Case of Lyman Alpha Emitters: Growing Younger from z ~ 3 to z ~ 2?

Viviana Acquaviva, Carlos Vargas, Eric Gawiser +1

Lyman Alpha Emitting (LAE) galaxies are thought to be progenitors of present-day L* galaxies. Clustering analyses have suggested that LAEs at z ~ 3 might evolve into LAEs at z ~ 2,…

astro-ph.CO2011★ 6 cited

SED fitting with MCMC: methodology and application to large galaxy surveys

Viviana Acquaviva, Eric Gawiser, Lucia Guaita

We present GalMC (Acquaviva et al 2011), our publicly available Markov Chain Monte Carlo algorithm for SED fitting, show the results obtained for a stacked sample of Lyman Alpha Em…

astro-ph.CO2011★ 113 cited

The Evolution of Ly-alpha Emitting Galaxies Between z = 2.1 and z = 3.1

Robin Ciardullo, Caryl Gronwall, Christopher Wolf +11

We describe the results of a new, wide-field survey for z=3.1 Ly-alpha emission-line galaxies (LAEs) in the Extended Chandra Deep Field South (ECDF-S). By using a nearly top-hat 50…

astro-ph.CO2011★ 19 cited

X-ray Constraints on the Lyman-Alpha Escape Fraction

Zhen-Ya Zheng, Sangeeta Malhotra, Jun-Xian Wang +7

We have coadded X-ray flux of all known Lyman Alpha Emitters (LAEs) in the 4 Msec Chandra Deep Field South (CDF-S) region, to place sensitive upper limits on the average unobscured…

astro-ph.CO2011★ 37 cited

Evolution in the Continuum Morphological Properties of Lyman-Alpha-Emitting Galaxies from z=3.1 to z=2.1

Nicholas Bond, Eric Gawiser, Lucia Guaita +4

We present a rest-frame ultraviolet morphological analysis of 108 z=2.1 Lyman Alpha Emitters (LAEs) in the Extended Chandra Deep Field South (ECDF-S) and compare it to a similar sa…

astro-ph.CO2011★ 107 cited

Ly-alpha Emitting Galaxies at z = 2.1: Stellar Masses, Dust and Star Formation Histories from Spectral Energy Distribution Fitting

Lucia Guaita, Viviana Acquaviva, Nelson Padilla +8

We study the physical properties of 216 z ~ 2.1 LAEs discovered in an ultra-deep narrow-band MUSYC image of the ECDF-S. We fit their stacked Spectral Energy Distribution (SED) usin…

astro-ph.CO2011★ 89 cited

SED fitting with Markov Chain Monte Carlo: Methodology and Application to z=3.1 Lyman Alpha Emitting Galaxies

Viviana Acquaviva, Eric Gawiser, Lucia Guaita

We present GalMC, a MCMC algorithm designed to fit the spectral energy distributions (SED) of galaxies to infer physical properties such as age, stellar mass, dust reddening, metal…

astro-ph.CO2010★ 16 cited

MIPS 24 Micron Observations of the Hubble Deep Field South: Probing the IR-Radio Correlation of Galaxies at z > 1

M. T. Huynh, E. Gawiser, D. Marchesini +2

We present MIPS 24 micron observations of the Hubble Deep Field South taken with the Spitzer Space Telescope. The resulting image is 254 arcmin^2 in size and has a sensitivity rang…

astro-ph.CO2010★ 9 cited

Clustering and descendants of MUSYC galaxies at z<1.5

Nelson Padilla, Daniel Christlein, Eric Gawiser +3

We measure the evolution of galaxy clustering out to a redshift of z~1.5 using data from two MUSYC fields, the Extended Hubble Deep Field South (EHDF-S) and the Extended Chandra De…

astro-ph.CO2009★ 189 cited

Lyman-Alpha-Emitting Galaxies at z = 2.1 in ECDF-S: Building Blocks of Typical Present-day Galaxies?

L. Guaita, E. Gawiser, N. Padilla +8

We discovered a sample of 250 Ly-Alpha emitting (LAE) galaxies at z=2.1 in an ultra-deep 3727 A narrow-band MUSYC image of the Extended Chandra Deep Field-South. LAEs were selected…