K
Kenneth J. Mighell
Researcher at ASTRON
Publications - 23
Citations - 912
Kenneth J. Mighell is an academic researcher from ASTRON. The author has contributed to research in topics: Light curve & RR Lyrae variable. The author has an hindex of 13, co-authored 23 publications receiving 887 citations. Previous affiliations of Kenneth J. Mighell include National Science Foundation.
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Journal ArticleDOI
Orbital Phase Variations of the Eccentric Giant Planet HAT-P-2b
Nikole K. Lewis,Nikole K. Lewis,Heather Knutson,Adam P. Showman,Nicolas B. Cowan,Gregory Laughlin,Adam Burrows,Drake Deming,Justin R. Crepp,Kenneth J. Mighell,Eric Agol,Gáspár Á. Bakos,David Charbonneau,Jean-Michel Desert,Debra A. Fischer,Jonathan J. Fortney,Joel D. Hartman,Sasha Hinkley,Andrew W. Howard,John Asher Johnson,Melodie M. Kao,Jonathan Langton,Geoffrey W. Marcy +22 more
TL;DR: In this paper, the authors presented the first phase curve observations for the highly eccentric hot Jupiter HAT-P-2b in the 3.6, 4.5, 5.8, and 8.0 μm bands of the Spitzer Space Telescope.
Journal ArticleDOI
Orbital Phase Variations of the Eccentric Giant Planet HAT-P-2b
Nikole K. Lewis,Heather Knutson,Adam P. Showman,Nicolas B. Cowan,Gregory Laughlin,Adam Burrows,Drake Deming,Justin R. Crepp,Kenneth J. Mighell,Eric Agol,Gáspár Á. Bakos,David Charbonneau,Jean-Michel Desert,Debra A. Fischer,Jonathan J. Fortney,Joel D. Hartman,Sasha Hinkley,Andrew W. Howard,John Asher Johnson,Melodie M. Kao,Jonathan Langton,Geoffrey W. Marcy,Joshua N. Winn +22 more
TL;DR: In this paper, the authors presented the first phase curve observations for the highly eccentric hot Jupiter HAT-P-2b in the 3.6, 4.5, 5.8, and 8.0 \mu m bands of the Spitzer Space Telescope.
Proceedings ArticleDOI
M32: Is there an Ancient, Metal‐Poor Population?
Giuliana Fiorentino,Antonela Monachesi,Scott Trager,Tod R. Lauer,A. Saha,Kenneth J. Mighell,Wendy L. Freedman,Alan Dressler,Carl J. Grillmair,Eline Tolstoy +9 more
TL;DR: In this paper, the authors focused on the detection of variability on RR Lyrae variable stars, which represents the only way to obtain information about the presence of a very old population (larger than 10 Gyr) in M32 from optical data.
Journal ArticleDOI
The deepest hubble space telescope color-magnitude diagram of m32. evidence for intermediate-age populations*
Antonela Monachesi,Scott Trager,Tod R. Lauer,Wendy L. Freedman,Alan Dressler,Carl J. Grillmair,Kenneth J. Mighell +6 more
TL;DR: In this article, the authors presented the deep optical color-magnitude diagram (CMD) of the local elliptical galaxy M32 and obtained F435W and F555W photometry based on HST images for a region 110 000 from the center of M32 (F1) and a background field about 320 000 away from M32 center.
Journal ArticleDOI
The star formation history of m32
Antonela Monachesi,Scott Trager,Tod R. Lauer,Sebastian L. Hidalgo,Wendy L. Freedman,Alan Dressler,Carl J. Grillmair,Kenneth J. Mighell +7 more
TL;DR: In this paper, the authors used deep Hubble Space Telescope Advanced Camera for Surveys/High Resolution Channel observations of a field within M32 (F1) and an M31 background field (F2) to determine the star formation history (SFH) of M32 from its resolved stellar population.