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Benjamin Magnelli

Affiliations: 
2009 Université Paris-Sud XI, Orsay, Essonne, France 
Website:
http://benjaminmagnelli.weebly.com
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Parents

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David Elbaz grad student 2009 Université Paris-Sud
 (Histoire cosmique de la formation d'étoiles vue dans l'infrarouge)
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Publications

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Leslie SK, Schinnerer E, Liu D, et al. (2020) The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼ 5 The Astrophysical Journal. 899: 58
Magnelli B, Boogaard L, Decarli R, et al. (2020) The ALMA spectroscopic survey in the HUDF : the cosmic dust and gas mass densities in galaxies up to z ∼ 3. The Astrophysical Journal. 892: 66
González-López J, Novak M, Decarli R, et al. (2020) The ALMA Spectroscopic Survey in the HUDF : deep 1.2 mm continuum number counts. The Astrophysical Journal. 897: 91
Jiménez-Andrade EF, Zavala JA, Magnelli B, et al. (2020) The Redshift and Star Formation Mode of AzTEC2: A Pair of Massive Galaxies at z = 4.63 The Astrophysical Journal. 890: 171
Fudamoto Y, Oesch PA, Magnelli B, et al. (2020) A3COSMOS: the dust attenuation of star-forming galaxies at z=2.5−4.0 from the COSMOS-ALMA archive Monthly Notices of the Royal Astronomical Society. 491: 4724-4734
Franco M, Elbaz D, Zhou L, et al. (2020) GOODS-ALMA: The slow downfall of star-formation in $z$ = 2-3 massive galaxies Astronomy and Astrophysics
Franco M, Elbaz D, Zhou L, et al. (2020) GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies Astronomy and Astrophysics
Zhou L, Elbaz D, Franco M, et al. (2020) GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5 Astronomy and Astrophysics
Liu D, Lang P, Magnelli B, et al. (2019) Automated mining of the ALMA archive in the COSMOS field (A3COSMOS): I. Robust ALMA continuum photometry catalogs and stellar mass and star formation properties for ∼700 galaxies at z = 0.5–6 Astrophysical Journal Supplement Series. 244: 40
Liu D, Schinnerer E, Groves B, et al. (2019) Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6 The Astrophysical Journal. 887: 235
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