Pablo G. Pérez‐González

Jet Propulsion Laboratory — United States

Physics and Astronomy · Physical Sciences

81h-index23.8kcitations596works20.32yr avg
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Research Topics

Astronomy and Astrophysical Research(399), Galaxies: Formation, Evolution, Phenomena(394), Stellar, planetary, and galactic studies(158), Gamma-ray bursts and supernovae(123), Astrophysics and Star Formation Studies(112)

Publications596 total

THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift Catalog
arXiv (Cornell University)·2025Open Access
JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster
Astronomy and Astrophysics·2025Open Access
JADES: carbon-enhanced, nitrogen-normal compact galaxy at z = 11.2
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
PRIMER and JADES reveal an abundance of massive quiescent galaxies at <b> 2 &amp;lt;   <i>z</i>  &amp;lt;  5 </b>
Monthly Notices of the Royal Astronomical Society·2025· 2 citedOpen Access
Confirming Near- to Mid-infrared Photometrically Identified Obscured AGNs in the JWST Era
The Astrophysical Journal·2025· 3 citedOpen Access
Deciphering the Nature of Virgil: An Obscured Active Galactic Nucleus Lurking within an Apparently Normal Ly <i>α</i> Emitter during Cosmic Reionization
The Astrophysical Journal·2025· 1 citedOpen Access
Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe
The Open Journal of Astrophysics·2025Open Access
Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe
Infoscience (Ecole Polytechnique Fédérale de Lausanne)·2025· 2 citedOpen Access
<i>JWST</i> PRIMER: a deep <i>JWST</i> study of all ALMA-detected galaxies in PRIMER COSMOS – dust-obscured star formation history back to <i>z</i> ≃ 7
Monthly Notices of the Royal Astronomical Society·2025· 4 citedOpen Access
Very Bright, Very Blue, and Very Red: JWST CAPERS Analysis of Highly Luminous Galaxies with Extreme Ultraviolet Slopes at <i>z</i> = 10
The Astrophysical Journal·2025· 5 citedOpen Access
Simulation-based inference of galaxy properties from JWST pixels
Astronomy and Astrophysics·2025· 4 citedOpen Access
Confirming Near- to Mid-IR Photometrically-Identified Obscured AGNs in the JWST era
arXiv (Cornell University)·2025Open Access
Not Just a Dot: The Complex UV Morphology and Underlying Properties of Little Red Dots
The Astrophysical Journal·2025· 15 citedOpen Access
The <i>z</i> ≳ 9 Galaxy UV Luminosity Function from the JWST Advanced Deep Extragalactic Survey: Insights into Early Galaxy Evolution and Reionization
The Astrophysical Journal·2025· 17 citedOpen Access
Exploring the Nature of Little Red Dots: Constraints on Active Galactic Nucleus and Stellar Contributions from PRIMER MIRI Imaging
The Astrophysical Journal·2025· 15 citedOpen Access
Analysis of the plane of satellites around Milky Way-like galaxies in $Λ$CDM cosmology
arXiv (Cornell University)·2025Open Access
The Rise of the Galactic Empire: Ultraviolet Luminosity Functions at <i>z</i> ∼ 17 and <i>z</i> ∼ 25 Estimated with the MIDIS+NGDEEP Ultra-deep JWST/NIRCam Data Set
The Astrophysical Journal·2025· 12 citedOpen Access
COSMOS-Web: The emergence of the Hubble sequence
Astronomy and Astrophysics·2025· 3 citedOpen Access
MIDIS: Unveiling the star formation history in massive galaxies at 1  &lt;   <i>z</i>   &lt;  4.5 with spectro-photometric analysis
Astronomy and Astrophysics·2025Open Access
PRIMER &amp; JADES reveal an abundance of massive quiescent galaxies at 2 &lt; z &lt; 5
St Andrews Research Repository (St Andrews Research Repository)·2025· 1 citedOpen Access
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Frequent Co-authors

Casey Papovich(26), G. H. Rieke(18), Anton M. Koekemoer(18), Mark Dickinson(16), Jonathan R. Trump(15), Jeyhan S. Kartaltepe(14), Dale D. Kocevski(14), Eiichi Egami(13), Steven L. Finkelstein(13), Henry C. Ferguson(13), Ray A. Lucas(13), Pablo Arrabal Haro(12), A. Fontana(12), Mauro Giavalisco(12), Norman A. Grogin(12), Nor Pirzkal(12), Karl D. Gordon(11), K. A. Misselt(11), Micaela B. Bagley(11), Stephen M. Wilkins(11)