A SEARCH FOR THE TRANSIT OF HD 168443b: IMPROVED ORBITAL PARAMETERS AND PHOTOMETRY [PDF]
The Astrophysical Journal, 2011 The discovery of transiting planets around bright stars holds the potential to greatly enhance our understanding of planetary atmospheres. In this work we present the search for transits of HD 168443b, a massive planet orbiting the bright star HD 168443 V=6.92 with a period of 58.11 days.
Genady Pilyavsky +31 more
openalex +9 more sources
Training a convolutional neural network for exoplanet classification with transit photometry data [PDF]
Scientific ReportsThe search for exoplanets aims to identify planets with compositions similar to Earth’s, providing insights into planetary formation and habitability.
Juliana Wang
doaj +2 more sources
A posteriori detection of the planetary transit of HD 189733 b in the Hipparcos photometry [PDF]
Astronomy & Astrophysics, 2005 7 pages, to be published in Astronomy & ...
G. Hébrard, A. Lecavelier des Etangs
openalex +3 more sources
Multilayer modeling of the aureole photometry during the Venus transit: comparison between SDO/HMI and VEx/SOIR data [PDF]
, 2016 The mesosphere of Venus is a critical range of altitudes in which complex temperature variability has been extensively studied by the space mission Venus Express (Vex) during its eight-years mission (2006-2014).
C. Pere +6 more
openalex +3 more sources
Relative photometry of transiting exoplanet CoRoT-Exo-2b [PDF]
, 2009 Relative CCD photometry of the extrasolar planet COROT-Exo-2b transiting in front of its parent star was carried out at the Astronomical and Geophysical Observatory of Comenius University at Modra (AGO). Physical and orbital parameters were determined and compared with the previous published data.
Peter Vereš +4 more
openalex +3 more sources
Some Tests to Establish Confidence in Planets Discovered by Transit Photometry
The Astrophysical Journal, 2002 Increased attention is being paid to transit photometry as a viable method for discovering or confirming detections of extrasolar planets. Several ground-based efforts are underway that target short-period, giant planets such as 51 Peg b, and several missions have been proposed to NASA and ESA to detect planets as small as Earth from spaceborne ...
J. Jenkins, D. Caldwell, W. Borucki
semanticscholar +3 more sources
Precision Near-Infrared Photometry for Exoplanet Transit Observations. I. Ensemble Spot Photometry for an All-Sky Survey [PDF]
Publications of the Astronomical Society of the Pacific, 2012 Near-IR observations are important for the detection and characterization of exoplanets using the transit technique, either in surveys of large numbers of stars or for follow-up spectroscopic observations of individual planets. In a controlled laboratory
C. Clanton +4 more
semanticscholar +5 more sources
Long-term photometry of IC 348 with the Young Exoplanet Transit Initiative network [PDF]
, 2016 D. J. Fritzewski +31 more
openalex +2 more sources
Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars [PDF]
Astrophysical Journal Supplement Series, 2023 The Transiting Exoplanet Survey Satellite (TESS) follow-up of a large number of known transiting exoplanets provides a unique opportunity to study their physical properties more precisely.
Suman Saha
semanticscholar +1 more source
Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems [PDF]
Astronomical Journal, 2019 We present ground-based infrared transit observations for four dynamically interacting Kepler planets, including Kepler-29b, Kepler-36c, KOI-1783.01, and Kepler-177c, obtained using the Wide-field Infrared Camera on the Hale 200 inch telescope at Palomar
S. Vissapragada +13 more
semanticscholar +1 more source