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20162021
most citedEphemeris refinement of 21 Hot Jupiter exoplanets with high timing uncertainties

33 citations · 33 across the 1 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2021

The orbit and stellar masses of the archetype colliding-wind binary WR 140

Joshua D. Thomas, Noel D. Richardson, J. J. Eldridge +33

We present updated orbital elements for the Wolf-Rayet (WR) binary WR\,140 (HD\,193793; WC7pd + O5.5fc). The new orbital elements were derived using previously published measuremen…

astro-ph.SR2020

Irregular emission cycles in the Oe star HD 60848

Gregor Rauw, Yael Naze, Fran Campos +2

We analyse the spectroscopic and photometric variability of the Oe star HD 60848 over the last twenty five years. The spectra reveal recurrent, but irregular cycles of increased ci…

astro-ph.SR2019

Quest for the tertiary component in Cyg OB2 #5

Gregor Rauw, Yaël Nazé, Fran Campos

The Cyg OB2 #5 system is thought to consist of a short-period (6.6 d) eclipsing massive binary orbited by an OB-star orbiting with a period of ~6.7 yr; these stars in turn are orbi…

astro-ph.EP201933 cited

Ephemeris refinement of 21 Hot Jupiter exoplanets with high timing uncertainties

M. Mallonn, C. von Essen, E. Herrero +32

Transit events of extrasolar planets offer a wealth of information for planetary characterization. However, for many known targets, the uncertainty of their predicted transit windo…

astro-ph.HE2018

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters

Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…

astro-ph.SR2018

Intriguing X-ray and optical variations of the gamma Cas analog HD45314

G. Rauw, Y. Nazé, M. A. Smith +11

A growing number of Be and Oe stars, named the gamma Cas stars, are known for their unusually hard and intense X-ray emission. This emission could either trace accretion by a compa…