PABLO GUILLERMO
PÉREZ GONZÁLEZ
Investigador en el periodo 2007-2018
University of California, Santa Cruz
Santa Cruz, Estados UnidosPublicaciones en colaboración con investigadores/as de University of California, Santa Cruz (53)
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
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
2021
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An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era
Monthly Notices of the Royal Astronomical Society, Vol. 507, Núm. 4, pp. 5144-5160
2020
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Physical properties from VLT spectroscopy of a sample of star-forming dwarf galaxies at intermediate redshift
Proceedings of the 10th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics VII, SEA 2012
2019
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The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
Astrophysical Journal, Supplement Series, Vol. 243, Núm. 2
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The structural properties of classical bulges and discs from z ∼ 2
Monthly Notices of the Royal Astronomical Society, Vol. 489, Núm. 3, pp. 4135-4154
2018
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A catalog of polychromatic bulge-disc decompositions of ~17.600 galaxies in CANDELS
Monthly Notices of the Royal Astronomical Society, Vol. 478, Núm. 4, pp. 5410-5426
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3
Astrophysical Journal, Vol. 853, Núm. 2
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Demographics of Star-forming Galaxies since z ∼ 2.5. I. the UVJ Diagram in CANDELS
Astrophysical Journal, Vol. 858, Núm. 2
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Evolution of the anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey: II. Structural and photometric evolution
Astronomy and Astrophysics, Vol. 615
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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
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Galaxy Inclination and the IRX-β Relation: Effects on UV Star Formation Rate Measurements at Intermediate to High Redshifts
Astrophysical Journal, Vol. 869, Núm. 2
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Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy-galaxy pairs from z = 3 to z ~ 0
Monthly Notices of the Royal Astronomical Society, Vol. 475, Núm. 2, pp. 1549-1573
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On the Transition of the Galaxy Quenching Mode at 0.5 < z < 1 in CANDELS
Astrophysical Journal, Vol. 860, Núm. 1
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The relationship between galaxy and dark matter halo size from z ~ 3 to the present
Monthly Notices of the Royal Astronomical Society, Vol. 473, Núm. 2, pp. 2714-2736
2017
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CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
Astrophysical Journal Letters, Vol. 841, Núm. 2
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CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2
Astrophysical Journal, Vol. 846, Núm. 2
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Spatially Resolved Kinematics in the Central 1 kpc of a Compact Star-forming Galaxy at z ∼ 2.3 from ALMA CO Observations
Astrophysical Journal Letters, Vol. 851, Núm. 2
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Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
Astrophysical Journal, Vol. 840, Núm. 1
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The AGN-Star Formation Connection: Future Prospects with JWST
Astrophysical Journal, Vol. 849, Núm. 2