activity
20142023
most citedGlobal Climate and Atmospheric Composition of the Ultra-Hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

221 citations · 2.6k across the 44 of their papers we have counts for

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Showing 2018Show all

12 papers · 1 filter

astro-ph.SR2018★ 47 cited

Detection of a giant flare displaying quasi-periodic pulsations from a pre-main sequence M star with NGTS

James A. G. Jackman, Peter J. Wheatley, Chloe E. Pugh +18

We present the detection of an energetic flare on the pre-main sequence M3 star NGTS J121939.5-355557, which we estimate as only 2 Myr old. The flare had an energy of $3.2\pm^{0.4}…

astro-ph.EP2018★ 24 cited

K2-265 b: A Transiting Rocky Super-Earth

K. W. F. Lam, A. Santerne, S. G. Sousa +34

We report the discovery of the super-Earth K2-265 b detected with K2 photometry. The planet orbits a bright (V_mag = 11.1) star of spectral type G8V with a period of 2.37 days. We…

astro-ph.EP2018★ 84 cited

NGTS-4b: A sub-Neptune Transiting in the Desert

Richard G. West, Edward Gillen, Daniel Bayliss +48

We report the discovery of NGTS-4b, a sub-Neptune-sized planet transiting a 13th magnitude K-dwarf in a 1.34d orbit. NGTS-4b has a mass M=M_E and radius R=…

astro-ph.SR2018★ 17 cited

A low-mass eclipsing binary within the fully convective zone from the NGTS

S. L. Casewell, L. Raynard, C. A. Watson +22

We have discovered a new, near-equal mass, eclipsing M dwarf binary from the Next Generation Transit Survey. This system is only one of 3 field age ( 1 Gyr), late M dwarf eclips…

astro-ph.EP2018★ 221 cited

Global Climate and Atmospheric Composition of the Ultra-Hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

Laura Kreidberg, Michael R. Line, Vivien Parmentier +12

We present thermal phase curve measurements for the hot Jupiter WASP-103b observed with Hubble/WFC3 and Spitzer/IRAC. The phase curves have large amplitudes and negligible hotspot…

astro-ph.EP2018★ 112 cited

An Earth-sized exoplanet with a Mercury-like composition

A. Santerne, B. Brugger, D. J. Armstrong +43

The Earth, Venus, Mars, and some extrasolar terrestrial planets have a mass and radius that is consistent with a mass fraction of about 30% metallic core and 70% silicate mantle. A…

astro-ph.EP2018★ 34 cited

Automatic vetting of planet candidates from ground based surveys: Machine learning with NGTS

David J. Armstrong, Maximilian N. Günther, James McCormac +22

State of the art exoplanet transit surveys are producing ever increasing quantities of data. To make the best use of this resource, in detecting interesting planetary systems or in…

astro-ph.EP2018★ 32 cited

Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system

Maximilian N. Günther, Didier Queloz, Edward Gillen +36

We present the discovery of NGTS-3Ab, a hot Jupiter found transiting the primary star of an unresolved binary system. We develop a joint analysis of multi-colour photometry, centro…

astro-ph.EP2018★ 28 cited

NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf

Liam Raynard, Michael R. Goad, Edward Gillen +42

We report the discovery of NGTS-2b, an inflated hot-Jupiter transiting a bright F5V star (2MASS J14202949-3112074; = K), discovered as part of the Ne…

astro-ph.EP2018★ 54 cited

The XUV environments of exoplanets from Jupiter-size to super-Earth

George W. King, Peter J. Wheatley, Michael Salz +8

Planets that reside close-in to their host star are subject to intense high-energy irradiation. Extreme-ultraviolet (EUV) and X-ray radiation (together, XUV) is thought to drive ma…

astro-ph.EP2018★ 122 cited

The Transiting Exoplanet Community Early Release Science Program for JWST

Jacob L. Bean, Kevin B. Stevenson, Natalie M. Batalha +99

The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structur…

astro-ph.EP2018★ 137 cited

An ultra-short period rocky super-Earth with a secondary eclipse and a Neptune-like companion around K2-141

Luca Malavolta, Andrew W. Mayo, Tom Louden +44

Ultra-short period (USP) planets are a class of low mass planets with periods shorter than one day. Their origin is still unknown, with photo-evaporation of mini-Neptunes and in-si…