activity
20102021
most citedSpectroscopic detection of CIV in a galaxy at z=7.045: Implications for the ionizing spectra of reionization-era galaxies

252 citations · 2.3k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.CO2021★ 37 cited

Strong lensing in UNIONS: Toward a pipeline from discovery to modeling

E. Savary, K. Rojas, M. Maus +16

We present a search for galaxy-scale strong gravitational lenses in the initial 2 500 square degrees of the Canada-France Imaging Survey (CFIS). We designed a convolutional neural…

astro-ph.GA2021★ 20 cited

ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies (SMGs) Selected by Herschel: Discovery of Spatially Extended SMGs and Implications

Fengwu Sun, Eiichi Egami, Timothy D. Rawle +19

We present an ALMA 1.3 mm (Band 6) continuum survey of lensed submillimeter galaxies (SMGs) at with an angular resolution of ". These galaxies were uncovere…

astro-ph.GA2020

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…

astro-ph.GA2018★ 54 cited

Kinematics, Turbulence and Star Formation of z ~1 Strongly Lensed Galaxies seen with MUSE

V. Patricio, J. Richard, D. Carton +18

We analyse a sample of 8 highly magnified galaxies at redshift 0.6<z<1.5 observed with MUSE, exploring the resolved properties of these galaxies at sub-kiloparsec scales. Combining…

astro-ph.GA2017★ 180 cited

The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

H. Inami, R. Bacon, J. Brinchmann +22

We have conducted a two-layered spectroscopic survey (1'x1' ultra deep and 3'x3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUS…

astro-ph.GA2016★ 126 cited

[CII] emission in z ~ 6 strongly lensed, star-forming galaxies

Kirsten K. Knudsen, Johan Richard, Jean-Paul Kneib +5

The far-infrared fine-structure line [CII] at 1900.5\,GHz is known to be one of the brightest cooling lines in local galaxies, and therefore it has been suggested to be an efficien…