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20042025
most citedAn ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2

1k citations · 18.5k across the 175 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

astro-ph.GA2017★ 59 cited

Spatially resolved kinematics in the central 1 kpc of a compact star-forming galaxy at z=2.3 from ALMA CO observations

G. Barro, M. Kriek, P. G. Perez-Gonzalez +9

We present high spatial resolution (FWHM0.14'') observations of the CO() line in GDS-14876, a compact star-forming galaxy at with total stellar mass of $\log(M_{…

astro-ph.GA2017★ 142 cited

The MOSDEF survey: a stellar mass-SFR-metallicity relation exists at

Ryan L. Sanders, Alice E. Shapley, Mariska Kriek +15

We investigate the nature of the relation among stellar mass, star-formation rate, and gas-phase metallicity (the M-SFR-Z relation) at high redshifts using a sample of 260 star…

astro-ph.GA2017★ 138 cited

The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, , at z~2

Irene Shivaei, Naveen A. Reddy, Brian Siana +11

We combine spectroscopic measurements of H and H and UV continuum photometry for a sample of 673 galaxies from the MOSFIRE Deep Evolution Field survey to constrain hydrogen i…

astro-ph.GA2017

The MOSDEF Survey: Broad Emission Lines at z=1.4-3.8

William R. Freeman, Brian Siana, Mariska Kriek +12

We present results from the MOSFIRE Deep Evolution Field (MOSDEF) survey on broad flux from the nebular emission lines H, [NII], [OIII], H, and [SII]. The sample consists of…

astro-ph.GA2017★ 28 cited

The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at

Alice E. Shapley, Ryan L. Sanders, Naveen A. Reddy +11

We present the first spectroscopic measurement of multiple rest-frame optical emission lines at . During the MOSFIRE Deep Evolution Field (MOSDEF) survey, we observed the gala…

astro-ph.GA2017★ 85 cited

Massive quenched galaxies at z~0.7 retain large molecular gas reservoirs

Katherine A. Suess, Rachel Bezanson, Justin S. Spilker +5

The physical mechanisms that quench star formation, turning blue star-forming galaxies into red quiescent galaxies, remain unclear. In this Letter, we investigate the role of gas s…