Jason F. Rowe
Bishop's University
388 Papers
13.2K Citations
Jason F. Rowe is an academic researcher from Bishop's University. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 110, co-authored 374 publications. Previous affiliations of Jason F. Rowe include Ames Research Center & University of British Columbia.
Chat about Author
Papers
MOST * DETECTS TRANSITS OF HD 97658b, A WARM, LIKELY VOLATILE-RICH SUPER-EARTH
Diana Dragomir,Diana Dragomir,Jaymie M. Matthews,Jason D. Eastman,Jason D. Eastman,Chris Cameron,Andrew W. Howard,David B. Guenther,Rainer Kuschnig,Anthony F. J. Moffat,Jason F. Rowe,Jason F. Rowe,Slavek M. Rucinski,Dimitar Sasselov,Werner W. Weiss +14 more
TL;DR: In this paper, the authors used photometric monitoring of the extended transit window of HD 97658b with the MOST space telescope, and they found that this exoplanet transits with an ephemeris consistent with that predicted from radial velocity measurements.
The distribution of transit durations for kepler planet candidates and implications for their orbital eccentricities
Althea V. Moorhead,Eric B. Ford,Robert C. Morehead,Jason F. Rowe,Jason F. Rowe,William J. Borucki,Natalie M. Batalha,Stephen T. Bryson,Douglas A. Caldwell,Douglas A. Caldwell,Daniel C. Fabrycky,Thomas N. Gautier,David G. Koch,Matthew J. Holman,Jon M. Jenkins,Jon M. Jenkins,Jie Li,Jie Li,Jack J. Lissauer,Philip W. Lucas,Geoffrey W. Marcy,Samuel N. Quinn,Elisa V. Quintana,Elisa V. Quintana,Darin Ragozzine,Avi Shporer,Avi Shporer,Martin Still,Guillermo Torres +28 more
TL;DR: In this paper, the authors analyzed the transit duration distribution of Kepler planet candidates and found that for host stars with T eff > 5100 K, they cannot invert this to infer the eccentricity distribution at this time due to uncertainties and possible systematics in the host star densities.
No Conclusive Evidence for Transits of Proxima b in MOST Photometry
David M. Kipping,Chris Cameron,Joel D. Hartman,James R. A. Davenport,Jaymie M. Matthews,Dimitar Sasselov,Jason F. Rowe,Robert J. Siverd,Jingjing Chen,Emily Sandford,Gáspár Á. Bakos,Andrés Jordán,Andrés Jordán,Daniel Bayliss,Thomas Henning,Luigi Mancini,Kaloyan Penev,Z. Csubry,Waqas Bhatti,Joao Bento,David B. Guenther,Rainer Kuschnig,Anthony F. J. Moffat,Slavek M. Rucinski,Werner W. Weiss +24 more
TL;DR: In this paper, D.M.G., J.R.M., A.F.K. and J.C.D. acknowledge support from FONDECYT project 1130857, BASAL CATA PFB-06, and the Ministry of Economy, Development, and Tourism’s Programa Iniciativa through grant IC 120009.
The most massive heartbeat: an in-depth analysis of ι Orionis
Herbert Pablo,Noel D. Richardson,Jim Fuller,Jim Fuller,Jason F. Rowe,A. F. J. Moffat,Rainer Kuschnig,Adam Popowicz,Gerald Handler,Coralie Neiner,Andrzej Pigulski,Gregg A. Wade,Werner W. Weiss,B. Buysschaert,B. Buysschaert,Tahina Ramiaramanantsoa,A. D. Bratcher,Cody Gerhartz,Jennifer J. Greco,Kevin K. Hardegree-Ullman,Ludwik Lembryk,Wayne L. Oswald +21 more
TL;DR: In this article, the authors used spectroscopic and light-curve analyses to measure the masses and radii of the components, revealing Ori to be the most massive heartbeat system known to date.
Using MOST to reveal the secrets of the mischievous Wolf—Rayet binary CV Ser
Alexandre David-Uraz,Anthony F. J. Moffat,André-Nicolas Chené,André-Nicolas Chené,Jason F. Rowe,Nicholas Lange,David B. Guenther,Rainer Kuschnig,Rainer Kuschnig,Jaymie M. Matthews,Slavek M. Rucinski,Dimitar Sasselov,Werner W. Weiss +12 more
TL;DR: In this paper, the Wolf-Rayet (WR) binary CV Serpentis (WR113, WC8d + O8-9IV) was observed to have two consecutive eclipses over the 29-d orbit, with varying depths.