#jwst observations

topicjwst observations

8 papers · 1 filter

astro-ph.GA2026

How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations

Sophie Koudmani, Jan Scholtz, Anthony J. Taylor +11

The paper uses the AESOPICA suite of cosmological simulations, varying black hole seed masses and accretion physics, to interpret the abundance and apparent overmassiveness of earl…

astro-ph.EP20261 cited

Methane on the temperate exo-Saturn TOI-199b

Aaron Bello-Arufe, Renyu Hu, Mantas Zilinskas +10

The authors present a JWST NIRSpec transmission spectrum of the temperate exo‑Saturn TOI‑199b, detecting methane and suggesting the presence of ammonia, while evaluating cloud/haze…

astro-ph.GA2026

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383

Josephine F. W. Baggen, Pieter van Dokkum, Ivo Labbé +1

The paper reports JWST NIRCam observations of a strongly lensed, luminous "little red dot" galaxy at redshift 6.0 behind the cluster A383, revealing a complex morphology with disti…

astro-ph.EP2026

Piercing through the Haze: Characterizing Titan-like terrestrial exoplanets with JWST

L. C. Mayorga, Jacob Lustig-Yaeger, Andrew P. Lincowski +5

The paper evaluates how well JWST can characterize Titan-like exoplanet atmospheres by testing retrieval methods on Cassini data and applying them to a hypothetical TRAPPIST-1 plan…

astro-ph.GA2026

The onset of stellar bars at Cosmic Noon. Bar-driven quenching and AGN co-evolution in a mature disc galaxy

Luca Costantin, Lorenzo Morelli, Cristina Cabello +15

The paper analyzes a barred spiral galaxy at redshift 1.17 using JWST NIRSpec data, showing that the bar formed early (z~5) and contributed to long‑term star‑formation quenching wh…

astro-ph.GA2026

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster

J. Nadolny, J. M. Pérez-Martínez, H. Dannerbauer +8

The paper uses JWST/NIRCam imaging to study how galaxy sizes and structures in the Spiderweb protocluster at z=2.16 depend on environment, finding distinct mass‑size relations for…