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EChO - The Exoplanet Characterisation Observatory | echo-spacemission.com Reviews
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EChO the Exoplanet CHaracterisation Observatory. Jump to main navigation and login. EChO ESA conference July 1-3 2013. Meudon Workshop - July 2012. Florence Workshop, Jan 31st 2012. Meudon Workshop - March 24th. Netherlands Workshop - Nov. 4/5. Barcelona EU Workshop - Sep. 30/Oct. 1. London Workshop - July 2010. Palermo Workshop - June 2010. Heidelberg Workshop - February 2010. Paris Workshop - Dec. 2009. London Workshop - Nov. 2009. The Exoplanet Characterisation Observatory. What are exoplanets made of?
WASP planets | WASP Planets
https://wasp-planets.net/category/wasp-planets
Transiting exoplanets from the Wide Angle Search for Planets. Category Archives: WASP planets. Using the stellar rotation to trace a planet’s orbit. And Jonti Horner have written a. Nice introduction to such techniques on the widely read. Website. Since large numbers of WASP planets orbit stars bright enough to enable a detection of the Rossiter–McLaughlin effect, around half of the planets with measured orbits. This entry was posted in Hot Jupiters. And tagged Rossiter-McLaughlin effect. August 15, 2016.
Spitzer observations of cool WASP planets | WASP Planets
https://wasp-planets.net/2015/08/06/spitzer-observations-of-cool-wasp-planets
Transiting exoplanets from the Wide Angle Search for Planets. Observations of cool WASP planets. A new paper by Joshua Kammer et al. Reports observations of 5 transiting hot-Jupiter planets with the. Space Telescope. The. Infra-red observations looked for the occultation of the planet, when it passes behind its host star. By comparing the observed emission in and out of the occultation one can deduce the temperature of the planet’s atmosphere. The plot shows the brightness ratio in the two pass-bands aga...
Papers | WASP Planets
https://wasp-planets.net/papers
Transiting exoplanets from the Wide Angle Search for Planets. Refereed papers about WASP planets and other papers using WASP data. Fossati, L., France, K., Koskinen, T., Juvan, I. G., Haswell, C. A., and Lendl, M. 2015, ApJ, Far-UV Spectroscopy of the Planet-hosting Star WASP-13: High-energy Irradiance, Distance, Age, Planetary Mass-loss Rate, and Circumstellar Environment. Large Binocular Telescope occultation data confirm significant thermal flux at short wavelengths. Sanchis-Ojeda, Roberto, Winn, Josh...
WASP-67b | WASP Planets
https://wasp-planets.net/tag/wasp-67b
Transiting exoplanets from the Wide Angle Search for Planets. Observations of cool WASP planets. A new paper by Joshua Kammer et al. Reports observations of 5 transiting hot-Jupiter planets with the. Space Telescope. The. Infra-red observations looked for the occultation of the planet, when it passes behind its host star. By comparing the observed emission in and out of the occultation one can deduce the temperature of the planet’s atmosphere. The plot shows the brightness ratio in the two pass-bands aga...
Images | WASP Planets
https://wasp-planets.net/images
Transiting exoplanets from the Wide Angle Search for Planets. An artist’s impression of the planet WASP-142b, depicted as seen from a hypothetical moon. (Credit: David A. Hardy. http:/ www.astroart.org/. Click for large version. Photos related to press release. Tom Wagg at Keele Observatory 1. Click for high-res version (3MB). Tom Wagg at Keele Observatory 2. Click for un-cropped high-res version (3MB). Tom Wagg at Keele Observatory 3. Click for un-cropped high-res version (3MB). Cloudy Days on Exoplanet...
WASP-10b | WASP Planets
https://wasp-planets.net/tag/wasp-10b
Transiting exoplanets from the Wide Angle Search for Planets. Observations of cool WASP planets. A new paper by Joshua Kammer et al. Reports observations of 5 transiting hot-Jupiter planets with the. Space Telescope. The. Infra-red observations looked for the occultation of the planet, when it passes behind its host star. By comparing the observed emission in and out of the occultation one can deduce the temperature of the planet’s atmosphere. The plot shows the brightness ratio in the two pass-bands aga...
Greatest Hits | WASP Planets
https://wasp-planets.net/greatest-hits
Transiting exoplanets from the Wide Angle Search for Planets. Long-lasting starspots on exoplanet-host Qatar-2. Using the stellar rotation to trace a planet’s orbit. KELT-16b and sub-1-day hot-Jupiter exoplanets. Changeable weather on exoplanet WASP-43b? HATS-18b and short-period hot Jupiters. Cloudy Days on Exoplanets May Hide Atmospheric Water. Starspots on WASP-85 from K2 transits. Titanium and Vanadium on the exoplanet WASP-121b? Search ADS for latest WASP papers. Follow Blog via Email.
WASP-8b | WASP Planets
https://wasp-planets.net/tag/wasp-8b
Transiting exoplanets from the Wide Angle Search for Planets. Observations of cool WASP planets. A new paper by Joshua Kammer et al. Reports observations of 5 transiting hot-Jupiter planets with the. Space Telescope. The. Infra-red observations looked for the occultation of the planet, when it passes behind its host star. By comparing the observed emission in and out of the occultation one can deduce the temperature of the planet’s atmosphere. The plot shows the brightness ratio in the two pass-bands aga...
WASP Planets | WASP Planets
https://wasp-planets.net/wasp-planets
Transiting exoplanets from the Wide Angle Search for Planets. Močnik etal 2016. Clicking on name gives ADS search, Position gives exoplanet.eu data). Long-lasting starspots on exoplanet-host Qatar-2. Using the stellar rotation to trace a planet’s orbit. KELT-16b and sub-1-day hot-Jupiter exoplanets. Changeable weather on exoplanet WASP-43b? HATS-18b and short-period hot Jupiters. Cloudy Days on Exoplanets May Hide Atmospheric Water. Starspots on WASP-85 from K2 transits. Search ADS for latest WASP papers.
Faint stars adjacent to WASP planet hosts | WASP Planets
https://wasp-planets.net/2015/07/11/faint-stars-adjacent-to-wasp-planet-hosts
Transiting exoplanets from the Wide Angle Search for Planets. Faint stars adjacent to WASP planet hosts. To estimate the radius of a transiting planet we simply measure the amount of light that it blocks during the transit. However, if there are faint, unseen stars in the photometric aperture they can dilute the light of the host star, leading to incorrect system parameters. Thus Maria Wöllert and co-authors have made a. Here are their images of three WASP stars:. This entry was posted in WASP planets.
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EChO - The Exoplanet Characterisation Observatory
EChO is one of the ESA M3 mission candidates currently assessed for an expected launch in 2022. Our consortium includes the contributions of UK, France, Italy, Spain, MPS Germany, Poland, Denmark, Ireland, Portugal, Sweden, University of Liege, Hungary and US. EChO will focus on Hot Jupiters, Hot and Warm Neptunes and Hot, Warm and Habitable Zone Super Earths.
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