activity
20082026
most citedESPRESSO@VLT -- On-sky performance and first results

537 citations · 10.5k across the 192 of their papers we have counts for

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Showing 2018Show all

18 papers · 1 filter

astro-ph.EP2018★ 44 cited

HD219666b: A hot-Neptune from TESS Sector 1

M. Esposito, D. J. Armstrong, D. Gandolfi +73

We report on the confirmation and mass determination of a transiting planet orbiting the old and inactive G7 dwarf star HD219666 (Mstar = 0.92 +/- 0.03 MSun, Rstar = 1.03 +/- 0.03…

astro-ph.IM2018★ 72 cited

ACTIN: A tool to calculate stellar activity indices

J. Gomes da Silva, P. Figueira, N. C. Santos +1

Magnetic activity in the atmospheres of stars produces a number of spectroscopic signatures that are visible in the shape and strength of spectral lines. These signatures can be us…

astro-ph.IM2018★ 33 cited

Telluric correction in the near-infrared: Standard star or synthetic transmission?

S. Ulmer-Moll, P. Figueira, J. J. Neal +2

Context. The atmospheric absorption of the Earth is an important limiting factor for ground-based spectroscopic observations and the near-infrared and infrared regions are the most…

astro-ph.EP2018★ 93 cited

SWEET-Cat updated. New homogenous spectroscopic parameters

S. G. Sousa, V. Adibekyan, E. Delgado-Mena +14

Context: Exoplanets have now been proven to be very common. The number of its detections continues to grow following the development of better instruments and missions. One key ste…

astro-ph.EP2018★ 16 cited

K2-263b: A 50-day period sub-Neptune with a mass measurement using HARPS-N

A. Mortier, A. S. Bonomo, V. M. Rajpaul +32

This paper reports on the validation and mass measurement of K2-263b, a sub-Neptune orbiting a quiet G9V star. Using K2 data from campaigns C5 and C16, we find this planet to have…

astro-ph.EP2018★ 31 cited

Activity induced variation in spin-orbit angles as derived from Rossiter-McLaughlin measurements

M. Oshagh, A. H. M. J. Triaud, A. Burdanov +17

One of the most powerful methods used to estimate sky-projected spin-orbit angles of exoplanetary systems is through a spectroscopic transit observation known as the Rossiter-McLau…