Ismael
Pérez Fournon
Profesor Titular Universidad
University of Maryland, College Park
College Park, Estados UnidosPublicacións en colaboración con investigadores/as de University of Maryland, College Park (25)
2024
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A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
Monthly Notices of the Royal Astronomical Society, Vol. 530, Núm. 4, pp. 4578-4596
2023
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Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets
Monthly Notices of the Royal Astronomical Society, Vol. 521, Núm. 4, pp. 5508-5535
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The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates
Monthly Notices of the Royal Astronomical Society, Vol. 522, Núm. 2, pp. 2995-3017
2022
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The bright extragalactic ALMA redshift survey (BEARS) I: Redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS
Monthly Notices of the Royal Astronomical Society, Vol. 511, Núm. 2, pp. 3017-3033
2021
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Close-up view of a luminous star-forming galaxy at z = 2.95
Astronomy and Astrophysics, Vol. 646
2020
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NOEMA redshift measurements of bright Herschel galaxies
Astronomy and Astrophysics, Vol. 635
2018
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Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens
Nature Astronomy, Vol. 2, Núm. 4, pp. 334-342
2017
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SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
Publications of the Astronomical Society of Australia, Vol. 34
2016
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CANDIDATE GRAVITATIONALLY LENSED DUSTY STAR-FORMING GALAXIES in the HERSCHEL WIDE AREA SURVEYS
Astrophysical Journal, Vol. 823, Núm. 1
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Dust properties of Lyman-break galaxies at z ∼ 3
Astronomy and Astrophysics, Vol. 587
2013
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Gravitational lens models based on Submillimeter Array Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.-selected strongly lensed sub-millimeter galaxies at z > 1.5
Astrophysical Journal, Vol. 779, Núm. 1
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HerMES: Candidate gravitationally lensed galaxies and lensing statistics at submillimeter wavelengths
Astrophysical Journal, Vol. 762, Núm. 1
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The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3
Nature, Vol. 498, Núm. 7454, pp. 338-341
2012
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A comprehensive view of a strongly lensed planck-associated submillimeter galaxy
Astrophysical Journal, Vol. 753, Núm. 2
2011
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Dynamical structure of the molecular interstellar medium in an extremely bright, multiply lensed z≃3 submillimeter galaxy discovered with Herschel
Astrophysical Journal Letters, Vol. 733, Núm. 1 PART 2
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Redshift determination and CO line excitation modeling for the multiply lensed galaxy HLSW-01
Astrophysical Journal, Vol. 733, Núm. 1
2010
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The herschel reference survey
Publications of the Astronomical Society of the Pacific, Vol. 122, Núm. 889, pp. 261-287
1996
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An early-time infrared and optical study of the type Ia supernovae SN 1994D and 1991T
Monthly Notices of the Royal Astronomical Society, Vol. 281, Núm. 1, pp. 263-280
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Circumnuclear emission line regions in Cygnus A
Vistas in Astronomy, Vol. 40, Núm. 1, pp. 51-55
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Toward an understanding of the seyfert galaxy NGC 5252: A spectroscopic study
Astrophysical Journal, Vol. 464, Núm. 1 PART I, pp. 177-197