Pablo G. Perez-Gonzalez

Universidad Complutense de Madrid

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Articles (20)

Collaborators (17)

Göran Östlin

Stockholm University

Georgios Magdis

Technical University of Denmark

Kevin Hainline

UNITED STATES

Carlos Gómez-Guijarro

Københavns Universitet

Armando Gil de Paz

Associate Professor

Universidad Complutense de Madrid

Jorge Zavala

Project Assistant Professor

National Astronomical Observatory of Japan

Stefi A. Baum

University of Manitoba

Thomas R. Greve

Technical University of Denmark

Patricia Sanchez-Blazquez

Senior Lecturer

Universidad Complutense de Madrid

Stijn Wuyts

University of Bath

UNITED KINGDOM

Emanuele Daddi

Université Paris-Saclay

Steven L Finkelstein

University of Texas at Austin

UNITED STATES

Marc Huertas-Company

Universidad de la Laguna

Steven Gillman

Technical University of Denmark

Laura Bisigello

University of Padova

G Yang

University of Groningen

Elizabeth McGrath

Colby College

UNITED STATES

Pablo G. Perez-Gonzalez

Research Interests

Explore related searches

Contact this professor

Articles (20)

Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI

Measuring the gas reservoirs in 108 < M⋆ < 1011 M⊙ galaxies at 1 ≤ z ≤ 3

Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?

What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition

MIDIS: JWST/MIRI Reveals the Stellar Structure of ALMA-selected Galaxies in the Hubble Ultra Deep Field at Cosmic Noon

MIDIS: The Relation between Strong (Hβ + [O iii]) Emission, Star Formation, and Burstiness around the Epoch of Reionization

MIDIS: Unveiling the Role of Strong Hα Emitters During the Epoch of Reionization with JWST

A NIRCam-dark Galaxy Detected with the MIRI/F1000W Filter in the MIDIS/JADES Hubble Ultra Deep Field

A fast-rotator post-starburst galaxy quenched by supermassive black-hole feedback at z = 3

5–25 μm Galaxy Number Counts from Deep JWST Data

CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies

JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies

Probing the Earliest Phases in the Formation of Massive Galaxies with Simulated HST+JWST Imaging Data from Illustris

Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

Probing the Star Formation Main Sequence Down to 108 M ⊙ at 1.0 < z < 3.0

MIDIS: Strong (Hβ+[O iii]) and Hα Emitters at Redshift z ≃ 7–8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field

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

NGDEEP Epoch 1: The Faint End of the Luminosity Function at z ∼ 9–12 from Ultradeep JWST Imaging

CEERS Key Paper. V. Galaxies at 4 < z < 9 Are Bluer than They Appear–Characterizing Galaxy Stellar Populations from Rest-frame ∼1 μm Imaging

CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results

Collaborators (17)

Göran Östlin

Georgios Magdis

Kevin Hainline

Carlos Gómez-Guijarro

Armando Gil de Paz

Jorge Zavala

Stefi A. Baum

Thomas R. Greve

Patricia Sanchez-Blazquez

Stijn Wuyts

Emanuele Daddi

Steven L Finkelstein

Marc Huertas-Company

Steven Gillman

Laura Bisigello

G Yang

Elizabeth McGrath

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