FOCUSBullying How do we respond as Christians?
Bullying - How do we respond as Christians? From: Missy (Original Message) Sent: 29/01/2006 13:50 This is a topic which Im sure has effected everyone in some way, whether it was persoanlly or a friend or family member suffering because of bullying.

Bullying boss
My boss basically forced me out of an organisation that was founded by my late father thriough her bullying behaviour this year. Recently, when after I had been out of my post for several months one of the board asked me to prepare a piece of work that wa

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

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. We’ll be submitting a paper on the detection very shortly, and I’ll put up all the details here as soon as I

Bullying
Please don't react to this as though I mean bullying is a good thing because it isn't, what I want to ask is some bullying normal, even very young children do it sometimes, before they're even aware of what bullying is and before they can hold a

Bullying Spirits
I was walking down the street under a train railing (I live in NYC) and i was with my kids who were much younger. And there father was being chased by a gang of kids (it was a gang) and he was with a hispanic kid, both of them were teenagers in the dream.

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

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.

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

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

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

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

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

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 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