Eshita Banerjee

collaborators

3 papers

astro-ph.GA2026

MUSEQuBES: Investigating the Physical and Chemical Properties of Circumgalactic Gas Around Ly $I^\pm$ Emitters at $z \approx 3.3$

Eshita Banerjee, Sowgat Muzahid, Joop Schaye +2

We present a detailed study of the physical properties of absorbers associated with $z \approx 3.3$ \lya\ emitters (LAEs) from the MUSEQuBES survey. Using \HI\ and ionic column densi…

astro-ph.GA2025

MUSEQuBES: Connecting HI absorption with Ly $I^\pm$ emitters at $z \approx 3.3$

Eshita Banerjee, Sowgat Muzahid, Joop Schaye +6

We present a comprehensive analysis of HI absorption around 96 lya emitters (LAEs) at $z \approx 3.3$ (median lya luminosity $\approx 1 0^{42}$ erg.s $^{- 1}$ ). These LAEs were identifie…

astro-ph.GA2025

MUSEQuBES: Unveiling Cosmic Web Filaments at $z \approx 3.6$ through Dual Absorption and Emission Line Analysis

Eshita Banerjee, Sowgat Muzahid, Joop Schaye +2

According to modern cosmological models, galaxies are embedded within cosmic filaments, which supply a continuous flow of pristine gas, fueling star formation and driving their evo…

MUSEQuBES: Investigating the Physical and Chemical Properties of Circumgalactic Gas Around LyI^± Emitters at z≈3.3

MUSEQuBES: Connecting HI absorption with LyI^± emitters at z≈3.3

MUSEQuBES: Unveiling Cosmic Web Filaments at z≈3.6 through Dual Absorption and Emission Line Analysis

MUSEQuBES: Investigating the Physical and Chemical Properties of Circumgalactic Gas Around Ly $I^\pm$ Emitters at $z \approx 3.3$

MUSEQuBES: Connecting HI absorption with Ly $I^\pm$ emitters at $z \approx 3.3$

MUSEQuBES: Unveiling Cosmic Web Filaments at $z \approx 3.6$ through Dual Absorption and Emission Line Analysis