Results 21 to 30 of about 2,666 (219)
A Blind Search for Transit Depth Variability with TESS
The phenomenon of transit depth variability offers a pathway through which processes such as exoplanet atmospheric activity and orbital dynamics can be studied.
Gavin Wang, Néstor Espinoza
doaj +1 more source
TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf
We report the discovery and validation of two long-period giant exoplanets orbiting the early K dwarf TOI-4600 ( V = 12.6, T = 11.9), first detected using observations from the Transiting Exoplanet Survey Satellite (TESS) by the TESS Single Transit ...
Ismael Mireles +33 more
doaj +1 more source
Exoplanet transit spectro-photometry with SOFIA [PDF]
AbstractWe present the prospects of observing extrasolar planets with the Stratospheric Observatory for Infrared Astronomy (SOFIA). Our analysis shows that optical and near-infrared photometric and spectrophotometric follow-up observations during planetary transits and\break eclipses will be feasible with SOFIA's instrumentation, especially with the ...
Daniel Angerhausen +2 more
openaire +1 more source
Transit origami: a method to coherently fold exomoon transits in time series photometry [PDF]
ABSTRACT One of the simplest ways to identify an exoplanetary transit is to phase fold a photometric time series upon a trial period – leading to a coherent stack when using the correct value. Such phase-folded transits have become a standard data visualization in modern transit discovery papers.
openaire +2 more sources
High-precision photometry of WASP-12 b transits [PDF]
5 pages, 3 figures, accepted for publication in A& ...
Maciejewski, G. +5 more
openaire +2 more sources
No Conclusive Evidence for Transits of Proxima b in MOST Photometry [PDF]
Abstract The analysis of Proxima Centauri’s radial velocities recently led Anglada-Escudé et al. to claim the presence of a low-mass planet orbiting the Sun’s nearest star once every 11.2 days. Although the a priori probability that Proxima b transits its parent star is just 1.5%, the potential impact of such a discovery would be ...
David M. Kipping +23 more
openaire +4 more sources
Constraining the oblateness of transiting planets with photometry and spectroscopy [PDF]
ABSTRACT Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle ingress and egress features in photometric transit light curves, we investigate the effect of oblateness on the spectroscopic Rossiter–McLaughlin (RM) signals. We found that
B Akinsanmi +4 more
openaire +3 more sources
TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and then confirmed using a combination of precise radial velocities ...
Shubham Kanodia +29 more
doaj +1 more source
VLT transit and occultation photometry for the bloated planet CoRoT-1b [PDF]
peer reviewedWe present VLT eclipse photometry for the giant planet CoRoT-1b. We observed a transit in the R-band filter and an occultation in a narrow filter centered on 2.09 microns.
J. Montalbán +26 more
core +1 more source
Transit Photometry of the Core‐dominated Planet HD 149026b [PDF]
18 pages, 4 figures, submitted to ...
Charbonneau, David +10 more
openaire +4 more sources

