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20172026
most citedThe MOSDEF Survey: the Variation of the Dust Attenuation Curve with Metallicity

119 citations · 796 across the 59 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.GA2019★ 6 cited

The MOSDEF Survey: [SIII] as a New Probe of Evolving ISM Conditions

Ryan L. Sanders, Tucker Jones, Alice E. Shapley +15

We present measurements of [SIII]9069,9531 for a sample of star-forming galaxies, the first sample with measurements of these lines at z>0.1. We employ the line rati…

astro-ph.EP2019★ 40 cited

Phase Curve of the Hot Jupiter WASP-19b

Ian Wong, Björn Benneke, Avi Shporer +13

We analyze the phase curve of the short-period transiting hot Jupiter system WASP-19, which was observed by the Transiting Exoplanet Survey Satellite () in Sector 9. WASP-19…

astro-ph.EP2019

TESS Reveals HD 118203 b to be a Transiting Planet

Joshua Pepper, Stephen R. Kane, Joseph E. Rodriguez +30

The exoplanet HD 118203 b, orbiting a bright (V = 8.05) host star, was discovered using the radial velocity method by da Silva et al. (2006), but was not previously known to transi…

astro-ph.GA2019★ 19 cited

Spatially resolved properties of galaxies from CANDELS+MUSE: Radial extinction profile and insights on quenching

Marziye Jafariyazani, Bahram Mobasher, Shoubaneh Hemmati +3

Studying the internal processes of individual galaxies at kilo-parsec scales is crucial in enhancing our understanding of galaxy formation and evolution processes. In this work, we…

astro-ph.EP2019

Exploring the atmospheric dynamics of the extreme ultra-hot Jupiter KELT-9b using TESS photometry

Ian Wong, Avi Shporer, Daniel Kitzmann +24

We carry out a phase-curve analysis of the KELT-9 system using photometric observations from NASA's Transiting Exoplanet Survey Satellite (TESS). The measured secondary eclipse dep…

astro-ph.SR2019★ 7 cited

Stellar Properties of KIC 8736245: An Eclipsing Binary with a Solar-type Star Leaving the Main Sequence

Tara Fetherolf, William F. Welsh, Jerome A. Orosz +5

There is a well-known stellar parameter discrepancy for late K and M dwarfs, in that the observed radii and temperatures are often respectively larger and cooler than predicted by…