activity
20242026
collaborators

6 papers

astro-ph.GA2026

Exploring biases in derived stellar parameters and the ionizing photon production efficiency

Ravi Jaiswar, Anshu Gupta, Elisabete da Cunha +8

Constraining the timescale and manner in which the Epoch of Reionization (EoR) occurred is a major JWST science goal. However, any constraints on the stellar or ionizing parameters…

astro-ph.GA2026

A Census of Double-Peaked Lyman-alpha Emitters in MAGPI: Classification, Global Characteristics, and Spatially Resolved Properties

Tamal Mukherjee, Tayyaba Zafar, Themiya Nanayakkara +17

Double-peaked Ly profiles provide critical insights into gas kinematics and the distribution of neutral hydrogen (HI) from the interstellar to the intergalactic medium (ISM to…

astro-ph.GA2025

The MAGPI Survey: the kinematic morphology-density relation (or lack thereof) and the Hubble sequence at

Caroline Foster, Mark W. Donoghoe, Andrew Battisti +26

This work presents visual morphological and dynamical classifications for 637 spatially resolved galaxies, most of which are at intermediate redshift (), in the Middle-Ag…

astro-ph.GA2024

The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at 0.3

Marcie Mun, Emily Wisnioski, Katherine E. Harborne +20

We investigate the internal and external mechanisms that regulate and quench star formation (SF) in galaxies at using MAGPI observations and the EAGLE, Magneticum, and…

astro-ph.GA2024

The MAGPI Survey: Insights into the Lyman-alpha line widths and the size of ionized bubbles at the edge of cosmic reionization

T. Mukherjee, T. Zafar, T. Nanayakkara +18

We present spectroscopic properties of 22 Lyman-alpha emitters(LAEs) at z=5.5-6.6 with Lyman-alpha(Lya) luminosity log([])=42.4-43.5, obtained using VLT/MUSE as…

astro-ph.CO2024

A Jet-Induced Shock in a Young, Powerful Radio Galaxy at z=3.00

Nick Seymour, Jess W. Broderick, Gael Noirot +9

The bright radio source, GLEAM J091734-001243 (hereafter GLEAM J0917-0012), was previously selected as a candidate ultra-high redshift (z>5) radio galaxy due to its compact radio s…