Jorge Zavala

Project Assistant Professor

National Astronomical Observatory of Japan

Japan

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About

Jorge Zavala is a Project Assistant Professor at the National Astronomical Observatory of Japan. His research focuses on the nature and evolution of massive compact stellar systems, as well as the ionization conditions and metallicity of distant galaxies. Recent articles include studies on high-redshift galaxies, utilizing advanced observational techniques such as those from JWST and ALMA. His contributions to the field enhance our understanding of galaxy formation and evolution in the early universe.

Articles (16)

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2024

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2023

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2023

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2023

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2023

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2022

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2022

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2022

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2022

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2021

Collaborators (15)

Charlotte Mason

Associate Professor

Københavns Universitet Niels Bohr Instituttet

DENMARK

Jorge Zavala

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Articles (16)

Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS

JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34

Evidence of Extreme Ionization Conditions and Low Metallicity in GHZ2/GLASS-Z12 from a Combined Analysis of NIRSpec and MIRI Observations

ALMA Detection of [O iii] 88 μm at z = 12.33: Exploring the Nature and Evolution of GHZ2 as a Massive Compact Stellar System

A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]

Missing Giants: Predictions on Dust-obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time

Broad Emission Lines in Optical Spectra of Hot, Dust-obscured Galaxies Can Contribute Significantly to JWST/NIRCam Photometry

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

The SCUBA-2 Cosmology Legacy Survey: the EGS deep field – III. The evolution of faint submillimetre galaxies at z &lt; 4

Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z ∼ 11–17: Blue Monsters or Low-z Red Interlopers?

Central concentration of warm and dense molecular gas in a strongly lensed submillimeter galaxy at z = 6

Probing Cold Gas in a Massive, Compact Star-forming Galaxy at z = 6

Searching Far and Long. I. Pilot ALMA 2 mm Follow-up of Bright Dusty Galaxies as a Redshift Filter

Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies

Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies

Collaborators (15)

Charlotte Mason

Fumi Egusa

Pablo G. Perez-Gonzalez

Maximilien FRANCO

Bunyo Hatsukade

Claudia Lagos

Arianna Long

Emanuele Daddi

Alexandra Pope

Francesco Valentino

Hideki Umehata

Tom Bakx

Yoichi Tamura

Ken-ichi Tadaki

Elizabeth McGrath

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The SCUBA-2 Cosmology Legacy Survey: the EGS deep field – III. The evolution of faint submillimetre galaxies at z < 4