scholarly journals The GAPS Programme with HARPS-N at TNG. XXXII. The revealing non-detection of metastable HeI in the atmosphere of the hot Jupiter WASP-80b

2021 ◽  
Author(s):  
L. Fossati ◽  
G. Guilluy ◽  
I. F. Shaikhislamov ◽  
I. Carleo ◽  
F. Borsa ◽  
...  
Keyword(s):  
Hot Jupiter

scholarly journals Probing Signatures of a Distant Planet around the Young T-Tauri Star CI Tau Hosting a Possible Hot Jupiter

2018 ◽  
Vol 859 (2) ◽  
pp. L28 ◽  
Author(s):  
Mihoko Konishi ◽  
Jun Hashimoto ◽  
Yasunori Hori
Keyword(s):  
Tauri Star ◽  
T Tauri ◽  
Hot Jupiter

scholarly journals TiO and VO broad band absorption features in the optical spectrum of the atmosphere of the hot-Jupiter HD 209458b

2008 ◽  
Vol 492 (2) ◽  
pp. 585-592 ◽  
Author(s):  
J.-M. Désert ◽  
A. Vidal-Madjar ◽  
A. Lecavelier des Etangs ◽  
D. Sing ◽  
D. Ehrenreich ◽  
...  
Keyword(s):  
Optical Spectrum ◽  
Broad Band ◽  
Band Absorption ◽  
Absorption Features ◽  
Hot Jupiter

scholarly journals Hot Jupiter Variability in Eclipse Depth

2007 ◽  
Vol 662 (2) ◽  
pp. L115-L118 ◽  
Author(s):  
Emily Rauscher ◽  
Kristen Menou ◽  
James Y.-K. Cho ◽  
Sara Seager ◽  
Bradley M. S. Hansen
Keyword(s):  
Hot Jupiter

0.94-2.42 μm GROUND-BASED TRANSMISSION SPECTRA OF THE HOT JUPITER HD-189733b

2014 ◽  
Vol 785 (1) ◽  
pp. 35 ◽  
Author(s):  
C. Danielski ◽  
P. Deroo ◽  
I. P. Waldmann ◽  
M. D. J. Hollis ◽  
G. Tinetti ◽  
...  
Keyword(s):  
Transmission Spectra ◽  
Hot Jupiter

scholarly journals Tidally induced stellar oscillations: converting modelled oscillations excited by hot Jupiters into observables

2020 ◽  
Vol 500 (2) ◽  
pp. 2711-2731
Author(s):  
Andrew Bunting ◽  
Caroline Terquem
Keyword(s):  
Radial Velocity ◽  
Orbital Period ◽  
Planetary Systems ◽  
Velocity Signal ◽  
Convective Flux ◽  
Hot Jupiters ◽  
Stellar Oscillations ◽  
Orbital Periods ◽  
Hot Jupiter

ABSTRACT We calculate the conversion from non-adiabatic, non-radial oscillations tidally induced by a hot Jupiter on a star to observable spectroscopic and photometric signals. Models with both frozen convection and an approximation for a perturbation to the convective flux are discussed. Observables are calculated for some real planetary systems to give specific predictions. The photometric signal is predicted to be proportional to the inverse square of the orbital period, P−2, as in the equilibrium tide approximation. However, the radial velocity signal is predicted to be proportional to P−1, and is therefore much larger at long orbital periods than the signal corresponding to the equilibrium tide approximation, which is proportional to P−3. The prospects for detecting these oscillations and the implications for the detection and characterization of planets are discussed.

scholarly journals Signatures of Nitrogen Chemistry in Hot Jupiter Atmospheres

2017 ◽  
Vol 850 (1) ◽  
pp. L15 ◽  
Author(s):  
Ryan J. MacDonald ◽  
Nikku Madhusudhan
Keyword(s):  
Hot Jupiter

scholarly journals NGTS-1b: a hot Jupiter transiting an M-dwarf

2017 ◽  
Vol 475 (4) ◽  
pp. 4467-4475 ◽  
Author(s):  
Daniel Bayliss ◽  
Edward Gillen ◽  
Philipp Eigmüller ◽  
James McCormac ◽  
Richard D Alexander ◽  
...  
Keyword(s):  
M Dwarf ◽  
Hot Jupiter

scholarly journals SOPHIE velocimetry ofKeplertransit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter

2014 ◽  
Vol 564 ◽  
pp. A56 ◽  
Author(s):  
M. Deleuil ◽  
J.-M. Almenara ◽  
A. Santerne ◽  
S. C. C. Barros ◽  
M. Havel ◽  
...  
Keyword(s):  
Hot Jupiter

scholarly journals WASP-23b: a transiting hot Jupiter around a K dwarf and its Rossiter-McLaughlin effect

2011 ◽  
Vol 531 ◽  
pp. A24 ◽  
Author(s):  
A. H. M. J. Triaud ◽  
D. Queloz ◽  
C. Hellier ◽  
M. Gillon ◽  
B. Smalley ◽  
...  
Keyword(s):  
Hot Jupiter
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