most citedKepler-21b: A rocky planet around a V = 8.25 magnitude star

108 citations · 271 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201944 cited

Exoplanet Imitators: A test of stellar activity behavior in radial velocity signals

Chantanelle Nava, Mercedes López-Morales, Raphaëlle D. Haywood +1

Accurately modeling effects from stellar activity is a key step in detecting radial velocity signals of low-mass and long-period exoplanets. Radial velocities from stellar activity…

astro-ph.EP201915 cited

Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems

Sophie C. Dubber, Annelies Mortier, Ken Rice +26

We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and Kepler-103c are both long-peri…

astro-ph.EP201947 cited

Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPS

T. A. Lopez, S. C. C. Barros, A. Santerne +36

The detection of low-mass transiting exoplanets in multiple systems brings new constraints to planetary formation and evolution processes and challenges the current planet formatio…

astro-ph.EP201946 cited

The CORALIE survey for southern extrasolar planets XVIII. Three new massive planets and two low mass brown dwarfs at separation larger than 5 AU

E. L. Rickman, D. Ségransan, M. Marmier +36

Context. Since 1998, a planet-search around main sequence stars within 50~pc in the southern hemisphere has been carried out with the CORALIE spectrograph at La Silla Observatory.…

astro-ph.SR201911 cited

The Solar Benchmark: Rotational Modulation of the Sun Reconstructed from Archival Sunspot Records

Brett M. Morris, James R. A. Davenport, Helen A. C. Giles +5

We use archival daily spot coverage measurements from Howard et al. (1984) to study the rotational modulation of the Sun as though it were a distant star. A quasi-periodic Gaussian…

astro-ph.EP2016108 cited

Kepler-21b: A rocky planet around a V = 8.25 magnitude star

Mercedes Lopez-Morales, Raphaelle D. Haywood, Jeffrey L. Coughlin +36

HD 179070, aka Kepler-21, is a V = 8.25 F6IV star and the brightest exoplanet host discovered by Kepler. An early detailed analysis by Howell et al. (2012) of the first thirteen mo…