PABLO GUILLERMO
PÉREZ GONZÁLEZ
Investigador no período 2007-2018
Niels Bohr Institute
Copenaguen, DinamarcaPublicacións en colaboración con investigadores/as de Niels Bohr Institute (8)
2024
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A new derivation of the Hubble constant from γ -ray attenuation using improved optical depths for the Fermi and CTA era
Monthly Notices of the Royal Astronomical Society, Vol. 527, Núm. 3, pp. 4632-4642
2023
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Life beyond 30: Probing the −20 < M UV < −17 Luminosity Function at 8 < z < 13 with the NIRCam Parallel Field of the MIRI Deep Survey
Astrophysical Journal Letters, Vol. 951, Núm. 1
2022
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A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging
Astrophysical Journal Letters, Vol. 940, Núm. 2
2019
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ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
Astrophysical Journal, Vol. 882, Núm. 2
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Investigating the physical properties of galaxies in the Epoch of Reionization with MIRI/JWST spectroscopy
Astronomy and Astrophysics, Vol. 629
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Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2≲ z ≲0.9
Monthly Notices of the Royal Astronomical Society, Vol. 485, Núm. 1, pp. 586-619
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Statistical Stellar Mass Corrections for High-z Galaxies Observed with JWST Broadband Filters Due to Template Degeneracies
Astrophysical Journal, Supplement Series, Vol. 243, Núm. 2
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