activity
20142026
most citedThe MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8

442 citations · 4.9k across the 98 of their papers we have counts for

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Showing 2022Show all

15 papers · 1 filter

astro-ph.GA2022★ 177 cited

The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques

Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher +52

The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy…

astro-ph.GA2022★ 55 cited

The gas and stellar content of a metal-poor galaxy at as revealed by JWST and ALMA

K. E. Heintz, C. Giménez-Arteaga, S. Fujimoto +27

We present a joint analysis of the galaxy S04590 at based on NIRSpec, NIRCam, and NIRISS observations obtained through as part of Early Release Observations programme of…

astro-ph.GA2022

Resolved velocity profiles of galactic winds at Cosmic Noon

Keerthi Vasan G. C., Tucker Jones, Ryan L. Sanders +7

We study the kinematics of the interstellar medium (ISM) viewed "down the barrel" in 20 gravitationally lensed galaxies during Cosmic Noon (). We use moderate-resoluti…

astro-ph.GA2022★ 3 cited

The MOSDEF Survey: Probing Resolved Stellar Populations at Using a New Bayesian-defined Morphology Metric Called Patchiness

Tara Fetherolf, Naveen A. Reddy, Alice E. Shapley +12

We define a new morphology metric called "patchiness" () that is sensitive to deviations from the average of a resolved distribution, does not require the galaxy center to be de…

astro-ph.GA2022★ 37 cited

A Preview of JWST Metallicity Studies at Cosmic Noon: The First Detection of Auroral [O II] Emission at High Redshift

Ryan L. Sanders, Alice E. Shapley, Leonardo Clarke +6

We present ultra-deep Keck/MOSFIRE rest-optical spectra of two star-forming galaxies at z=2.18 in the COSMOS field with bright emission lines, representing more than 20~hours of to…

astro-ph.GA2022★ 19 cited

CLASSY V: The impact of aperture effects on the inferred nebular properties of local star-forming galaxies

Karla Z. Arellano-Córdova, Matilde Mingozzi, Danielle A. Berg +23

Strong nebular emission lines are an important diagnostic tool for tracing the evolution of star-forming galaxies across cosmic time. However, different observational setups can af…

astro-ph.GA2022★ 5 cited

The MOSDEF Survey: Towards a Complete Census of the z ~ 2.3 Star-forming Galaxy Population

Jordan N. Runco, Alice E. Shapley, Ryan L. Sanders +16

We analyze the completeness of the MOSDEF survey, in which z ~ 2 galaxies were selected for rest-optical spectroscopy from well-studied HST extragalactic legacy fields down to a fi…

astro-ph.GA2022★ 2 cited

The MOSDEF Survey: A New View of a Remarkable z=1.89 Merger

Jordan N. Runco, Alice E. Shapley, Mariska Kriek +13

We present a detailed study of a galaxy merger taking place at in the GOODS-S field. Here we analyze Keck/MOSFIRE spectroscopic observations from the MOSFIRE Deep Evolutio…

astro-ph.GA2022

The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Networks

Kim-Vy H. Tran, Anishya Harshan, Karl Glazebrook +13

We present spectroscopic confirmation of candidate strong gravitational lenses using the Keck Observatory and Very Large Telescope as part of our ASTRO 3D Galaxy Evolution with Len…

astro-ph.GA2022★ 31 cited

CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at

Ryan L. Sanders, Alice E. Shapley, Tucker Jones +9

We present observations of CO(3-2) in 13 main-sequence star-forming galaxies at that span a wide range in metallicity (O/H) based on res…

astro-ph.GA2022★ 19 cited

The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon

Gergö Popping, Irene Shivaei, Ryan L. Sanders +6

We aim to quantify the relation between the dust-to-gas mass ratio (DTG) and gas-phase metallicity of 2.1-2.5 luminous galaxies and contrast this high-redshift relation against…

astro-ph.GA2022★ 17 cited

The MOSDEF-LRIS Survey: Connection between Galactic-scale Outflows and the Properties of ~2 star-forming Galaxies

Andrew Weldon, Naveen Reddy, Michael Topping +10

We investigate the conditions that facilitate galactic-scale outflows using a sample of 155 typical star-forming galaxies at ~2 drawn from the MOSFIRE Deep Evolution Field (MOSD…

astro-ph.GA2022★ 114 cited

The COS Legacy Archive Spectroscopy SurveY (CLASSY) Treasury Atlas

Danielle A. Berg, Bethan L. James, Teagan King +46

Far-ultraviolet (FUV; ~1200-2000 angstroms) spectra are fundamental to our understanding of star-forming galaxies, providing a unique window on massive stellar populations, chemica…

astro-ph.GA2022★ 24 cited

IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3

Irene Shivaei, Gergö Popping, George Rieke +12

We present results from ALMA 1.2mm continuum observations of a sample of 27 star-forming galaxies at z=2.1-2.5 from the MOSFIRE Deep Evolution Field (MOSDEF) survey. These galaxies…

astro-ph.GA2022★ 31 cited

The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift

Prerak Garg, Desika Narayanan, Nell Byler +9

The Baldwin, Philips, & Terlevich diagram of [O III]/H vs. [N II]/H (hereafter N2-BPT) has long been used as a tool for classifying galaxies based on the dominant source of i…