activity
20242026
collaborators

16 papers

astro-ph.GA2026

ALMA observations of pre-JWST z ~ 10 galaxy candidates: A CO(J = 9-8) line from a ULIRG at z = 2.54 and revisit of the photometric redshifts with JWST photometry

Suzuka Arai, Yuma Sugahara, Akio K. Inoue +15

We present Atacama Large Millimetre/submillimetre Array (ALMA) observations targeting the [OIII]m line for six galaxy candidates selected with the Hubble Space Tel…

astro-ph.IM2026

Performance of Photometric Template Fitting for Ultra-High Redshift Galaxies

Thorbjørn Clausen, Charles L. Steinhardt, Arden Shao +1

The James Webb Space Telescope (JWST) has enabled the discovery of a significant population of galaxies at z > 10. Our understanding of the astrophysical properties of these galaxi…

astro-ph.GA2026

Direct Evidence for Stellar Initial Mass Function Variation in the Milky Way

Charles L. Steinhardt, Carter Meyerhoff, Alexander J. Luening

Because direct measurements require resolved stellar populations including low-mass stars, determining the stellar initial mass function (IMF) has been a historically difficult pro…

astro-ph.GA2026

Direct pathway to the Early Supermassive Black Holes: A Red Super-Eddington Quasar in a Massive Starburst Host at

Qinyue Fei, Seiji Fujimoto, Gabriel Brammer +24

We present a panchromatic optical-mm characterization of GNz7q, a recently identified X-ray weak, rapidly growing red quasar embedded within a dusty starburst galaxy at ,…

astro-ph.GA2025

Diverse reddening distributions in sight lines to type Ia supernovae

Lucas Hallgren, Radoslaw Wojtak, Jens Hjorth +1

Precise cosmological constraints from type Ia supernovae require adequately accurate corrections for host-galaxy extinction. Modelling these corrections is challenged by the proble…

astro-ph.GA2025

Evidence for Multiple Types of Post-Starburst Galaxies

Emma W. Nielsen, Charles L. Steinhardt, Mathieux Harper +2

The quenching mechanisms of galaxies are not yet fully understood, but post-starburst galaxies provide one explanation for the rapid transition between star-forming and quiescent g…