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.
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Papers
Spectroscopy, MOST Photometry, and Interferometry of MWC 314: Is it an LBV or an interacting binary?
Noel D. Richardson,Anthony F. J. Moffat,Raphael Maltais-Tariant,Herbert Pablo,Douglas R. Gies,Hideyuki Saio,Nicole St-Louis,Gail Schaefer,Anatoly S. Miroshnichenko,Chris Farrington,Emily J. Aldoretta,Étienne Artigau,Tabetha S. Boyajian,Kathryn Gordon,Jeremy Jones,Rachel A. Matson,Harold A. McAlister,David O'Brien,Deepak Raghavan,Tahina Ramiaramanantsoa,Stephen T. Ridgway,Nic Scott,Judit Sturmann,Laszlo Sturmann,T. ten Brummelaar,Joshua D. Thomas,Nils H. Turner,Norm Vargas,Sergey Zharikov,Jaymie M. Matthews,C. Cameron,David B. Guenther,Rainer Kuschnig,Rainer Kuschnig,Jason F. Rowe,Slavek M. Rucinski,Dimitar Sasselov,Werner W. Weiss +37 more
TL;DR: In this article, a luminous blue variable (LBV) was observed with a combination of optical spectroscopy, broad-band ground and space-based photometry, as well as with long baseline, near-infrared interferometry.
MOST★ photometry of the RRd Lyrae variable AQ Leo: two radial modes, 32 combination frequencies and beyond
Michael Gruberbauer,Katrien Kolenberg,Katrien Kolenberg,Jason F. Rowe,Daniel Huber,Jaymie M. Matthews,P. Reegen,Rainer Kuschnig,Chris Cameron,Thomas Kallinger,Werner W. Weiss,David B. Guenther,Anthony F. J. Moffat,Slavek M. Rucinski,Dimitar Sasselov,Gordon A. H. Walker +15 more
TL;DR: In this article, the MOST observations have revealed that the RR Lyrae star AQ Leo oscillates with at least 42 frequencies, of which 32 are linear combinations (up to the sixth order) of the radial fundamental mode and its first overtone.
Regular frequency patterns in the young δ Scuti star HD 261711 observed by the CoRoT and MOST satellites
Konstanze Zwintz,Konstanze Zwintz,Luca Fossati,David B. Guenther,T. A. Ryabchikova,A. Baglin,N. Themessl,Thomas G. Barnes,Jaymie M. Matthews,M. Auvergne,D. A. Bohlender,S. Chaintreuil,Rainer Kuschnig,A. F. J. Moffat,Jason F. Rowe,Slavek M. Rucinski,Dimitar Sasselov,Werner W. Weiss +17 more
TL;DR: In this article, an asteroseismological study of a star called HD 261711, a relatively hot δ Scuti-type pulsating member of the young open cluster NGC 2264 located at the blue border of the instability region is presented.
Revised Masses and Densities of the Planets around Kepler-10
Lauren M. Weiss,Leslie A. Rogers,Howard Isaacson,Eric Agol,Eric Agol,Geoffrey W. Marcy,Jason F. Rowe,David M. Kipping,Benjamin J. Fulton,Jack J. Lissauer,Andrew W. Howard,Daniel C. Fabrycky +11 more
TL;DR: In this paper, the authors used 220 radial velocities (RVs), including 72 precise RVs from Keck-HIRES of which 20 are new from 2014 to 2015, and 17 quarters of Kepler photometry, to obtain the most complete picture of the Kepler-10 system to date.
MOST Detects g-Modes in the Late-Type Be Star β Canis Minoris (B8 Ve)
Hideyuki Saio,Chris Cameron,Rainer Kuschnig,Gordon A. H. Walker,Jaymie M. Matthews,Jason F. Rowe,Umin Lee,Daniel Huber,Werner W. Weiss,David B. Guenther,Anthony F. J. Moffat,Slavek M. Rucinski,Dimitar Sasselov +12 more
TL;DR: In this paper, the Microvariability and Oscillations of Stars (MOST) satellite has detected low-amplitude light variations (?m ~ 1 mmag) in the Be star? CMi (B8 Ve).