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"secondary bartley"
WASP-33b Secondary transit
Thermal emission from WASP-33b, the hottest known planet http://arxiv.org/abs/1101.2432 We report ground-based observations at 0.91 microns of the occultation of the hot Jupiter WASP-33b by its A5 host star. We measure the planet to be 0.090 +/- 0.016
Thermal emission from WASP-33b, the hottest known planet http://arxiv.org/abs/1101.2432 We report ground-based observations at 0.91 microns of the occultation of the hot Jupiter WASP-33b by its A5 host star. We measure the planet to be 0.090 +/- 0.016
HD 80606 secondary transits detected.
Greg on the Systemic blog at www.oklo.org wrote Greg wrote: Hi Everyone, HD 80606b was indeed observed in secondary transit by Spitzer. Well be submitting a paper on the detection very shortly, and Ill put up all the details here as soon as I
Greg on the Systemic blog at www.oklo.org wrote Greg wrote: Hi Everyone, HD 80606b was indeed observed in secondary transit by Spitzer. Well be submitting a paper on the detection very shortly, and Ill put up all the details here as soon as I
WASP-4 b 3.6 and 4.5 µm secondary eclipse photometry with Spitzer
Secondary Eclipse Photometry of WASP-4b with Warm Spitzer http://arxiv.org/abs/1011.4066 We present photometry of the giant extrasolar planet WASP-4b at 3.6 and 4.5 micron taken with the Infrared Array Camera on board the Spitzer Space Telescope as
Secondary Eclipse Photometry of WASP-4b with Warm Spitzer http://arxiv.org/abs/1011.4066 We present photometry of the giant extrasolar planet WASP-4b at 3.6 and 4.5 micron taken with the Infrared Array Camera on board the Spitzer Space Telescope as
Equation for secondary transit depth?
Anyone have an equation handy for the secondary transit depth? I figure part of it is probably A(Rstar/Rplanet)2 where A is the albedo of the planet, but I'm not sure how to work in the difference in brightness between the two.
Anyone have an equation handy for the secondary transit depth? I figure part of it is probably A(Rstar/Rplanet)2 where A is the albedo of the planet, but I'm not sure how to work in the difference in brightness between the two.
First Secondary Grade Short Stories
Hi , my dearest. I am very glad to introduce you this short pamphlet which consists of a whole explanation of your short stories. I hope you will study it carefully and try to answer the exercises individually and if you have a problem meet or
Hi , my dearest. I am very glad to introduce you this short pamphlet which consists of a whole explanation of your short stories. I hope you will study it carefully and try to answer the exercises individually and if you have a problem meet or
Secondary transit of WASP-12 b
Day-side z'-band emission and eccentricity of Wasp-12b http://arxiv.org/abs/0912.2359 Abstract wrote:We report the detection of the eclipse of the very-hot Jupiter WASP-12b via z'-band time-series photometry obtained with the 3.5-meter ARC telescope a
Day-side z'-band emission and eccentricity of Wasp-12b http://arxiv.org/abs/0912.2359 Abstract wrote:We report the detection of the eclipse of the very-hot Jupiter WASP-12b via z'-band time-series photometry obtained with the 3.5-meter ARC telescope a
Now, that's secondary cause of migraine!...
holy... what a story: A man who went to the doctor complaining of a headache was shocked to discover he'd had a 4in knife blade stuck in his brain for more than four years. Li Fu from Yunnan Province, China, was stabbed during a robbery in 2006, and
holy... what a story: A man who went to the doctor complaining of a headache was shocked to discover he'd had a 4in knife blade stuck in his brain for more than four years. Li Fu from Yunnan Province, China, was stabbed during a robbery in 2006, and
Secondary eclipse of HAT-P-1 from Spitzer
Spitzer IRAC Secondary Eclipse Photometry of the Transiting Extrasolar Planet HAT-P-1b http://arxiv.org/abs/0911.2218 Abstract wrote:We report Spitzer/IRAC photometry of the transiting giant exoplanet HAT-P-1b during its secondary eclipse. This planet
Spitzer IRAC Secondary Eclipse Photometry of the Transiting Extrasolar Planet HAT-P-1b http://arxiv.org/abs/0911.2218 Abstract wrote:We report Spitzer/IRAC photometry of the transiting giant exoplanet HAT-P-1b during its secondary eclipse. This planet
TrES-3 b secondary eclipse detection.
Near-Infrared Thermal Emission from TrES-3b: A Ks-band detection and an H-band upper limit on the depth of the secondary eclipse http://arxiv.org/abs/1006.0737 Abstract wrote:We present H and Ks-band photometry bracketing the secondary eclipse of the
Near-Infrared Thermal Emission from TrES-3b: A Ks-band detection and an H-band upper limit on the depth of the secondary eclipse http://arxiv.org/abs/1006.0737 Abstract wrote:We present H and Ks-band photometry bracketing the secondary eclipse of the
Spitzer observes secondary transit of WASP-18 b
Spitzer Secondary Eclipses of WASP-18b http://arxiv.org/abs/1005.1017 Abstract wrote:The transiting exoplanet WASP-18b was discovered in 2008 by the Wide Angle Search for Planets (WASP) project. The \textit{Spitzer}\ Exoplanet Target of Opportunity
Spitzer Secondary Eclipses of WASP-18b http://arxiv.org/abs/1005.1017 Abstract wrote:The transiting exoplanet WASP-18b was discovered in 2008 by the Wide Angle Search for Planets (WASP) project. The \textit{Spitzer}\ Exoplanet Target of Opportunity
Spitzer CoRoT-1, CoRoT-2 secondary eclipse photometry
Warm Spitzer Photometry of the Transiting Exoplanets CoRoT-1 and CoRoT-2 at Secondary Eclipse http://arxiv.org/abs/1011.1019 We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 microns, and CoRoT-2 at 3.6 microns, both
Warm Spitzer Photometry of the Transiting Exoplanets CoRoT-1 and CoRoT-2 at Secondary Eclipse http://arxiv.org/abs/1011.1019 We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 microns, and CoRoT-2 at 3.6 microns, both
Secondary Transit of CoRoT-Exo-2 b
Searching for the secondary eclipse of CoRoT-Exo-2b and its transit timing variations http://arxiv.org/abs/0807.4828 Abstract wrote:With more than 80 transits observed in the CoRoT light curve with a cadence of 32 s, CoRoT-Exo-2b provides an excellent
Searching for the secondary eclipse of CoRoT-Exo-2b and its transit timing variations http://arxiv.org/abs/0807.4828 Abstract wrote:With more than 80 transits observed in the CoRoT light curve with a cadence of 32 s, CoRoT-Exo-2b provides an excellent
WASP-17 b secondary eclipse -- 2 R_J, slightly eccentric,
Thermal emission at 4.5 and 8 micron of WASP-17b, an extremely large planet in a slightly eccentric orbit http://arxiv.org/abs/1101.5620 We report the detection of thermal emission at 4.5 and 8 micron from the planet WASP-17b. We used Spitzer to
Thermal emission at 4.5 and 8 micron of WASP-17b, an extremely large planet in a slightly eccentric orbit http://arxiv.org/abs/1101.5620 We report the detection of thermal emission at 4.5 and 8 micron from the planet WASP-17b. We used Spitzer to
Introduction
Hello, I'm Russell Darnley. I'm the Computer Coordinator at Sydney Secondary College - Leichhardt Campus. I'm interested in any discussion on the application of the DER Laptops to education. I've a few ideas that I'll share. I've been involved
Hello, I'm Russell Darnley. I'm the Computer Coordinator at Sydney Secondary College - Leichhardt Campus. I'm interested in any discussion on the application of the DER Laptops to education. I've a few ideas that I'll share. I've been involved
Espiro or BCP??
Immorthal,I would like to know wich one is safer,if I have to choose one... My skin and hair it´s terribly oily,I can´t stand it anymore,I have to take one of this too,or propecia. Wich one has less side effects?
Immorthal,I would like to know wich one is safer,if I have to choose one... My skin and hair it´s terribly oily,I can´t stand it anymore,I have to take one of this too,or propecia. Wich one has less side effects?
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CBI ECONOMIC DATA 27-05-2012
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