activity
19982022
most citedHerschel Detects a Massive Dust Reservoir in Supernova 1987A

368 citations · 2.1k across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.GA2022★ 43 cited

GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching

C. Gómez-Guijarro, D. Elbaz, M. Xiao +38

Compact star formation appears to be generally common in dusty star-forming galaxies (SFGs). However, its role in the framework set by the scaling relations in galaxy evolution rem…

astro-ph.GA2021★ 89 cited

GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

C. Gómez-Guijarro, D. Elbaz, M. Xiao +36

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally…

astro-ph.GA2020★ 37 cited

GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5

L. Zhou, D. Elbaz, M. Franco +30

In this paper we study the properties of the six optically dark galaxies detected in the 69 arcmin^2 GOODS-ALMA 1.1mm continuum survey. While none of them are listed in the deepest…

astro-ph.GA2020★ 51 cited

GOODS-ALMA: The slow downfall of star-formation in = 2-3 massive galaxies

M. Franco, D. Elbaz, L. Zhou +34

We investigate the properties of a sample of 35 galaxies, detected with ALMA at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin, resolution = 0.60", RMS 0.18 mJy bea…

astro-ph.GA2020★ 24 cited

GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies

M. Franco, D. Elbaz, L. Zhou +33

In this paper, we extend the source detection in the GOODS-ALMA field (69 arcmin, rms sensitivity 0.18 mJy.beam), to deeper levels than presented in Franco…

astro-ph.GA2018★ 51 cited

GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxies

M. Franco, D. Elbaz, M. Béthermin +36

We present a 69 arcmin ALMA survey at 1.1mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band part of the GOODS-South field. We taper the 0"24 original image with a homogeneous…