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James G. Ingalls

California Institute of Technology · US
Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Planet, Transit (satellite), Exoplanet, and Stars.
h-index
citations
2,879
works
12
NIH funding
primary concept
email

Recent publications

Transit Timing Variations for AU Microscopii b and c
The Astronomical Journal 2022cited by 19position: middledoi
Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides
The Planetary Science Journal 2021cited by 318position: middledoi
Spitzer IRAC Photometry of JWST Calibration Stars
The Astronomical Journal 2021cited by 16position: middledoi
TRAPPIST-1: Global results of the Spitzer Exploration Science Program Red Worlds★
Apollo (University of Cambridge) 2020cited by 60position: middledoi
Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides
arXiv (Cornell University) 2020cited by 21position: middledoi
Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the “Planetary” Mass Regime
The Astrophysical Journal Supplement Series 2019cited by 131position: middledoi
The nature of the TRAPPIST-1 exoplanets
Astronomy and Astrophysics 2018cited by 339position: middledoi
Early 2017 observations of TRAPPIST-1 with Spitzer
Monthly Notices of the Royal Astronomical Society 2018cited by 102position: middledoi
Multiwavelength Light Curves of Two Remarkable Sagittarius A* Flares
The Astrophysical Journal 2018cited by 35position: middledoi
Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1
Nature 2017cited by 1,550position: middledoi
<i>SPITZER</i>SECONDARY ECLIPSES OF THE DENSE, MODESTLY-IRRADIATED, GIANT EXOPLANET HAT-P-$20{\rm b}$ USING PIXEL-LEVEL DECORRELATION
The Astrophysical Journal 2015cited by 283position: middledoi
The pros and cons of the inversion method approach to derive 3D dust emission properties in the ISM: the Hi-GAL field centred on (l, b) = (30 , 0 )
Monthly Notices of the Royal Astronomical Society 2014cited by 5position: middledoi

Grants

No grants ingested yet.

Frequent collaborators

S. Carey · California Institute of Technology6 papers (2014–2021)Eric Agol · University of Washington3 papers (2015–2020)L. Delrez · University of Liège2 papers (2018–2020)Émeline Bolmont · University of Geneva2 papers (2018–2020) · 2 papers (2018–2020) · 2 papers (2018–2020) · 2 papers (2018–2020) · 2 papers (2018–2021)Jérémy Leconte · Centre National de la Recherche Scientifique2 papers (2018–2020)Julien de Wit · Massachusetts Institute of Technology2 papers (2018–2020)Patrick Lowrance · California Institute of Technology2 papers (2019–2021)M. Gillon · Planetary Science Institute2 papers (2018–2020)Emmanuël Jehin · Planetary Science Institute2 papers (2018–2020)D. Queloz · University of Cambridge2 papers (2018–2020) · 2 papers (2018–2021)Adam J. Burgasser · UC San Diego Health System2 papers (2018–2020) · 1 papers (2018–2018)Jessica Krick · California Institute of Technology1 papers (2021–2021) · 1 papers (2015–2015)M. Morris · University of California, Los Angeles1 papers (2018–2018)