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20052026
most citedSeven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1

1.6k citations · 8.5k across the 94 of their papers we have counts for

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Showing 2013Show all

8 papers · 1 filter

astro-ph.SR2013★ 37 cited

Properties of the Eclipsing Double-White Dwarf Binary NLTT 11748

David L. Kaplan, Thomas R. Marsh, Arielle N. Walker +9

We present high-quality ULTRACAM photometry of the eclipsing detached double-white dwarf binary NLTT 11748. This system consists of a carbon/oxygen white dwarf and an extremely-low…

astro-ph.EP2013★ 44 cited

Optical transmission photometry of the highly inflated exoplanet WASP-17b

J. Bento, P. J. Wheatley, C. M. Copperwheat +7

We present ground-based high-precision observations of the transit of WASP-17b using the multi-band photometer ULTRACAM on ESO's NTT in the context of performing transmission spect…

astro-ph.SR2013★ 18 cited

The AM CVn binary SDSS J173047.59+554518.5

P. J. Carter, D. Steeghs, T. R. Marsh +4

The AM Canum Venaticorum (AM CVn) binaries are a rare group of hydrogen-deficient, ultra-short period, mass-transferring white dwarf binaries, and are possible progenitors of type…

astro-ph.SR2013★ 121 cited

The planets around NN Ser: still there

T. R. Marsh, S. G. Parsons, M. C. P. Bours +6

We present 25 new eclipse times of the white dwarf binary NN Ser taken with the high-speed camera ULTRACAM on the WHT and NTT, the RISE camera on the Liverpool Telescope, and HAWK-…

astro-ph.EP2013★ 34 cited

ULTRACAM z'-band Detection of the Secondary Eclipse of WASP-12b

D. Föhring, V. S. Dhillon, Nikku Madhusudhan +4

We present z'-band secondary eclipse photometry of the highly irradiated hot Jupiter WASP-12b using ULTRACAM on the 4.2m William Herschel Telescope. We measure a decrease in flux o…

astro-ph.SR2013★ 16 cited

Hot subdwarf stars in close-up view IV. Helium abundances and the He isotopic anomaly of subdwarf B star

S. Geier, U. Heber, H. Edelmann +5

Atmospheric parameters and helium abundances of 44 bright subdwarf B stars have been determined. More than half of our sample consists of newly discovered stars from the Edinburgh…