activity
20172021
most citedThe VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to

140 citations · 515 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.GA202227 cited

The average dust attenuation curve at z~1.3 based on HST grism surveys

A. J. Battisti, M. B. Bagley, I. Baronchelli +12

We present the first characterisation of the average dust attenuation curve at by combining rest-frame ultraviolet through near-IR photometry with Balmer decrement ($\ma…

astro-ph.GA202249 cited

Metallicity, ionization parameter, and pressure variations of HII regions in the TYPHOON spiral galaxies

K. Grasha, Q. H. Chen, A. J. Battisti +12

We present a spatially-resolved HII region study of the gas-phase metallicity, ionization parameter, and ISM pressure maps of 6 local star-forming and face-on spiral galaxies from…

astro-ph.GA2021

Revisiting Attenuation Curves: the Case of NGC 3351

Daniela Calzetti, Andrew J. Battisti, Irene Shivaei +14

Multi-wavelength images from the farUV (~0.15 micron) to the sub-millimeter of the central region of the galaxy NGC 3351 are analyzed to constrain its stellar populations and dust…

astro-ph.GA2020

The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

C. Foster, J. T. Mendel, C. D. P. Lagos +40

We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical dri…

astro-ph.GA2020140 cited

The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to

Sarah Leslie, Eva Schinnerer, Daizhong Liu +17

We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass () relation, called the main sequence of star-forming g…

astro-ph.GA2020119 cited

The MOSDEF Survey: the Variation of the Dust Attenuation Curve with Metallicity

Irene Shivaei, Naveen Reddy, George Rieke +14

We derive the UV-optical stellar dust attenuation curve of galaxies at z=1.4-2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding tho…