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20132022
most citedThe SOPHIE search for northern extrasolar planets VIII. A warm Neptune orbiting HD164595

84 citations · 1.3k across the 43 of their papers we have counts for

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Showing 2019Show all

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astro-ph.EP2019★ 36 cited

A HARPS RV search for planets around young nearby stars

A. Grandjean, A. -M. Lagrange, M. Keppler +9

Young nearby stars are good candidates in the search for planets with both radial velocity (RV) and direct imaging techniques. This, in turn, allows for the computation of the gian…

astro-ph.EP2019★ 51 cited

The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain

N. C. Hara, F. Bouchy, M. Stalport +32

Since 2011, the SOPHIE spectrograph has been used to search for Neptunes and super-Earths in the Northern Hemisphere. As part of this observational program, 290 radial velocity mea…

astro-ph.SR2019★ 1 cited

The Leavitt law of Milky Way Cepheids from Gaia DR2 static companion parallaxes

Louise Breuval, Pierre Kervella, Frédéric Arenou +13

Classical Cepheids (CCs) are at the heart of the empirical extragalactic distance ladder. Milky Way CCs are the only stars of this class accessible to trigonometric parallax measur…

astro-ph.SR2019★ 31 cited

A thin shell of ionized gas explaining the IR excess of classical Cepheids

V. Hocdé, N. Nardetto, E. Lagadec +12

Despite observational evidences, InfraRed (IR) excess of classical Cepheids are seldom studied and poorly understood, but probably induces systematics on the Period-Luminosity (PL)…

astro-ph.SR2019★ 65 cited

The detection and characterisation of 54 massive companions with the SOPHIE spectrograph -- 7 new brown dwarfs and constraints on the BD desert

F. Kiefer, G. Hébrard, J. Sahlmann +35

Brown-dwarfs are substellar objects with masses intermediate between planets and stars within about 13-80Mjup. While isolated BDs are most likely produced by gravitational collapse…

astro-ph.SR2019★ 24 cited

Consistent radial velocities of classical Cepheids from the cross-correlation technique

Simon Borgniet, Pierre Kervella, Nicolas Nardetto +11

Accurate radial velocities () of Cepheids are mandatory within the context of distance measurements via the Baade-Wesselink technique. The most common de…

astro-ph.EP2019★ 2 cited

Constraints on HD113337 fundamental parameters and planetary system. Combining long-base visible interferometry, disk imaging and high-contrast imaging

S. Borgniet, K. Perraut, K. Su +13

HD113337 is a Main-Sequence F6V field star more massive than the Sun, hosting one (possibly two) radial velocity (RV) giant planet(s) and a cold debris disk (marked by an infrared…

astro-ph.SR2019★ 34 cited

Activity time series of old stars from late F to early K. I. Simulating radial velocity, astrometry, photometry, and chromospheric emission

N. Meunier, A. -M. Lagrange, T. Boulet +1

Solar simulations and observations show that the detection of long-period Earth-like planets is expected to be very difficult with radial velocity techniques in the solar case beca…

astro-ph.EP2019★ 23 cited

The SOPHIE search for northern extrasolar planets XV. A Warm Neptune around the M-dwarf Gl378

M. J. Hobson, X. Delfosse, N. Astudillo-Defru +31

We present the detection of a Warm Neptune orbiting the M-dwarf Gl378, using radial velocity measurements obtained with the SOPHIE spectrograph at the Observatoire de Haute-Provenc…