Results 11 to 20 of about 242,108 (213)
CHEOPS: A transit photometry mission for ESA's small mission programme [PDF]
Ground based radial velocity (RV) searches continue to discover exoplanets below Neptune mass down to Earth mass. Furthermore, ground based transit searches now reach milli-mag photometric precision and can discover Neptune size planets around bright ...
Wolfgang Baumjohann +2 more
exaly +4 more sources
A SEARCH FOR THE TRANSIT OF HD 168443b: IMPROVED ORBITAL PARAMETERS AND PHOTOMETRY [PDF]
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.
Jason T Wright +2 more
exaly +10 more sources
Transit Analysis Package: An IDL Graphical User Interface for Exoplanet Transit Photometry [PDF]
We present an IDL graphical user-interface-driven software package designed for the analysis of exoplanet transit light curves. The Transit Analysis Package (TAP) software uses Markov Chain Monte Carlo (MCMC) techniques to fit light curves using the ...
J. Zachary Gazak +6 more
doaj +3 more sources
TERMS PHOTOMETRY OF KNOWN TRANSITING EXOPLANETS [PDF]
The Transit Ephemeris Refinement and Monitoring Survey (TERMS) conducts radial velocity and photometric monitoring of known exoplanets in order to refine planetary orbits and predictions of possible transit times. This effort is primarily directed towards planets not known to transit, but a small sample of our targets consist of known transiting ...
Dragomir, Diana +12 more
core +10 more sources
Transit Photometry of the Core‐dominated Planet HD 149026b [PDF]
18 pages, 4 figures, submitted to ...
Gaspar Bakos +2 more
exaly +5 more sources
Transit Photometry as an Exoplanet Discovery Method [PDF]
Photometry with the transit method has arguably been the most successful exoplanet discovery method to date. A short overview about the rise of that method to its present status is given. The method's strength is the rich set of parameters that can be obtained from transiting planets, in particular in combination with radial velocity observations; the ...
Roi Alonso, Hans J Deeg
exaly +5 more sources
Scintillation Noise in Exoplanet Transit Photometry
Transit photometry is a powerful technique for studying exoplanets. Transit observations from the ground of targets of magnitude V= 10 or brighter, however, are limited by scintillation noise due to Earth's atmosphere. Through turbulence profiling using instruments such as the stereo-SCIDAR, we have shown to able to accurately model scintillation noise,
James Osborn, Vik Dhillon
exaly +4 more sources
Comet C/2011 J2 (LINEAR): Photometry and stellar transit [PDF]
We present results of two-year photometric monitoring of Comet C/2011 J2 (LINEAR) that spans the time period from February 2013 through December 2014, before and after perihelion passage. The observations were conducted with broadband R filter. Analysis of observations of Comet C/2011 J2 (LINEAR) allows estimating the nucleus radius as function of ...
Oleksandra Ivanova +2 more
exaly +3 more sources
Some Tests to Establish Confidence in Planets Discovered by Transit Photometry
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 ...
Jon Jenkins, Douglas A Caldwell
exaly +3 more sources
Photometry and transit modelling of exoplanet WASP-140b [PDF]
Accepted by JAAVSO, 12 pages, 5 figures, 2 ...
North, Allen, Banks, Timothy
openaire +3 more sources

