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19952023
most citedThe COSMOS [OII] Survey: Evolution of Electron Density with Star Formation Rate

91 citations · 617 across the 30 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 8 cited

MOSEL and IllustrisTNG: Massive Extended Galaxies at z=2 Quench Later Than Normal-size Galaxies

Anshu Gupta, Kim-Vy Tran, Annalisa Pillepich +4

Using the TNG100 (100 Mpc)^3 simulation of the IllustrisTNG project, we demonstrate a strong connection between the onset of star formation quenching and the stellar size of galaxi…

gr-qc2020★ 33 cited

Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications

Sunil Choudhary, Nicolas Sanchis-Gual, Anshu Gupta +3

We show how gravitational-wave observations of binary black hole (BBH) mergers can constrain the physical characteristics of a scalar field cloud parameterized by mass an…

astro-ph.GA2020★ 24 cited

MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3<z<4) from the ZFOURGE Survey

Kim-Vy H. Tran, Ben Forrest, Leo Y. Alcorn +13

To understand how strong emission line galaxies (ELGs) contribute to the overall growth of galaxies and star formation history of the universe, we target Strong ELGs (SELGs) from t…

gr-qc2020★ 37 cited

News from horizons in binary black hole mergers

Vaishak Prasad, Anshu Gupta, Sukanta Bose +2

In a binary black hole merger, it is known that the inspiral portion of the waveform corresponds to two distinct horizons orbiting each other, and the merger and ringdown signals c…

astro-ph.GA2020★ 10 cited

MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation

Anshu Gupta, Kim-Vy Tran, Jonathan Cohn +13

We use K-band spectroscopic data from the Multi-Object Spectroscopic Emission Line (MOSEL) survey to analyze the kinematic properties of galaxies at z>3. Our sample consists of 34…

astro-ph.GA2020★ 16 cited

ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62

Anishya Harshan, Anshu Gupta, Kim-Vy Tran +8

The global star formation rates (SFR) of galaxies at fixed stellar masses increase with redshift and are known to vary with environment unto z~2. We explore here whether the change…