activity
20192026
most citedReionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe

211 citations · 1.5k across the 35 of their papers we have counts for

collaborators
Showing 2022Show all

12 papers · 1 filter

astro-ph.GA2022★ 105 cited

The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7

Hiddo Algera, Hanae Inami, Pascal Oesch +21

Cosmic dust is an essential component shaping both the evolution of galaxies and their observational signatures. How quickly dust builds up in the early Universe remains an open qu…

astro-ph.GA2022★ 88 cited

Dual constraints with ALMA: new [O III] 88 m and dust-continuum observations reveal the ISM conditions of luminous LBGs at

Joris Witstok, Renske Smit, Roberto Maiolino +10

We present new [O III] 88 m observations of five bright Lyman-break galaxies spectroscopically confirmed by ALMA through the [C II] 158 m line, unlike…

astro-ph.GA2022

The ALMA REBELS Survey: Average [CII] sizes of Star-Forming Galaxies from to

Y. Fudamoto, R. Smit, R. A. A. Bowler +36

We present the average [CII] emission line sizes of UV-bright star-forming galaxies at . Our results are derived from a stacking analysis of [CII] $158\,\rm{…

astro-ph.GA2022★ 57 cited

ALMA Confirmation of an Obscured Hyperluminous Radio-Loud AGN at Associated with a Dusty Starburst in the 1.5 deg COSMOS Field

Ryan Endsley, Daniel P. Stark, Jianwei Lyu +7

We present band 6 ALMA observations of a heavily-obscured radio-loud ( W Hz) AGN candidate at found in the 1.5…

astro-ph.GA2022★ 93 cited

The ALMA REBELS Survey: Specific Star-Formation Rates in the Reionization Era

Michael W. Topping, Daniel P. Stark, Ryan Endsley +21

We present specific star-formation rates for 40 UV-bright galaxies at observed as part of the Reionization Era Bright Emission Line Survey (REBELS) ALMA large program. T…

astro-ph.GA2022★ 126 cited

The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5

Hanae Inami, Hiddo S. B. Algera, Sander Schouws +25

We report 18 dust continuum detections () at and out of 49 ultraviolet(UV)-bright galaxies ( mag) at , observed…

astro-ph.GA2022★ 10 cited

Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z = 6.827 using NOEMA

S. J. Molyneux, R. Smit, D. Schaerer +8

We present the spectroscopic confirmation of the brightest known gravitationally lensed Lyman break galaxy in the Epoch of Reionisation, A1703-zD1, through the detection of [C II]…

astro-ph.GA2022★ 124 cited

The ALMA REBELS Survey: the dust content of Lyman Break Galaxies

P. Dayal, A. Ferrara, L. Sommovigo +22

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LB…

astro-ph.GA2022★ 104 cited

The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at

A. Ferrara, L. Sommovigo, P. Dayal +27

We analyse FIR dust continuum measurements for 14 galaxies () in the ALMA REBELS LP to derive their physical properties. Our model uses three input data: (a) the UV spe…

astro-ph.GA2022★ 4 cited

ALMA as a Redshift Machine: Using [CII] to Efficiently Confirm Galaxies in the Epoch of Reionization

Sander Schouws, Rychard Bouwens, Renske Smit +11

The [CII] line has long been proposed as a promising line to spectroscopically confirm galaxies in the epoch of reionization. In this paper we present the results of new…

astro-ph.GA2022★ 131 cited

The REBELS ALMA Survey: cosmic dust temperature evolution out to z 7

L. Sommovigo, A. Ferrara, A. Pallottini +27

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature remains mostly unconstrained due to t…

astro-ph.GA2022★ 51 cited

The ALMA REBELS Survey: Efficient Ly Transmission of UV-Bright z7 Galaxies from Large Velocity Offsets and Broad Line Widths

Ryan Endsley, Daniel P. Stark, Rychard J. Bouwens +19

Recent work has shown that UV-luminous reionization-era galaxies often exhibit strong Lyman-alpha emission despite being situated at redshifts where the IGM is thought to be substa…