WFC3 slitless spectroscopy Harald Kuntschner Martin K mmel, Jeremy R. Walsh (ST-ECF) WFC3-team at STScI and NASA WFC3 Grism Parameters WFC3-IR G141 Ground ...
LIM: Near IR from a mini-satellite Dani Maoz HST WFC3 IR channel: 1k x 1k HgCdTe detector, QE 80% 18 micron pixels (0.13 /pix), ~2 x2 FOV Detector sensitivity ...
The WFC3 IR channel will provide an efficient wide area coverage, with imaging ... Agency/Space Telescope Science Institute. 2Space Telescope Science Institute ...
within two weeks three groups had submitted papers on z~7-8 galaxies, followed ... searches conducted using the very robust and well-tested photometric 'dropout' ...
Chandra NASA s Great Observatories an astronomical Mount Rushmore Compton Hubble Spitzer Gains in orbit No atmospheric blurring Wider accessible wavelength ...
Flight will be on Atlantis - last flight of this shuttle ... Atlantis Shuttle Crew ... That Space Shuttle Atlantis is named after the Woods' Hole Oceanographic ...
... and little growth of red mass function (solid lines) ... IMPRS Galaxies course (with Rix) Source of baby clothes. Coffee, bowling, playing with children ...
At present there are two main technologies for large megapixel arrays: InSb: under development by the ALADDIN (Advanced Large Area Detector Development ...
Title: High Contrast Imaging with the Hubble Space Telescope Author: krist Last modified by: krist Created Date: 4/8/2004 12:58:34 AM Document presentation format
... it works (the guts) Basic processing. Low-level ... Search Sizes and Triggers (background info) Documentation ... New Bright Object Tool Documentation ...
Paul R Jorden, Peter Pool Marconi Applied Technologies. Simon M Tulloch ... XMM-Newton Epic CCD22 SXI CCD64. 600 *600 FT, 40 um, open pixels 512*580, 16 um ...
pulsar planetary system first discovered in 1992 - and to date the lowest mass planet ... are such disks suitable for planet formation? disks or rings? ...
Title: Uno Author: Marco Sirianni Last modified by: Marco Sirianni Created Date: 6/3/2005 8:22:17 PM Document presentation format: On-screen Show Company
Tracking stations. South Africa, Argentina. CDTI Ministerio de Industria. UCM ... ORFEUS flown on the Space Shuttle on two space shuttle flights in 1993 and 1996 ...
What is SHARE? SHARE = Study of Hubble Archive & Reprocessing Enhancements Chartered by Rodger Doxsey Study participants include Jerry Kriss (chair) HST/STIS & NGST
Past ...future? NASA's Great Observatories 'an astronomical Mount Rushmore' Spitzer ... Hubble constant from Cepheid variable stars. Black holes in (almost all) ...
Terry Bridges (Queens, Kingston); Mike Hudson (Waterloo) ... Bryan Miller (Gemini); Jennifer Lotz (NOAO) ... Smith (Durham) and Mike Hudson (Waterloo) Summary ...
Star formation is one of the most fundamental processes in astronomy, ... of stellar populations, revealing young stars that are still hidden by dust at ...
HUBBLE Past future? Gains in orbit No atmospheric blurring Wider accessible wavelength range Instrumental stability No clouds/daylight (timing) Some HST Science ...
NASA's Great Observatories 'an astronomical Mount Rushmore' Spitzer. Chandra. Compton ... Hubble constant from Cepheid variable stars. Black holes in (almost ...
An extraordinary panchromatic survey efficiency covering a critical decade of ... What determined the properties that galaxies ... Downsizing in Star Formation ...
... Institute of Astronomy (Canada) Massimo Capaccioli - Universit degli Studi di Napoli (Italy) ... SBF: distance indicator for a much larger family of ...
Destruction of the Twin Towers The Event The Event The Event The Event The Event The Event The Stage World Trade Center World Trade Center 110 stories WTC 1-2 ...
Much material obtained from Tarle and Bebek SNAP DOE talks. NIR System Concept. 150 NIR Megapixels: 36 (2k 2k) 18 mm HgCdTe detectors (0.34 sq. deg) ...
Water in Martian rocks as revealed by WFPC2 (left panel) and NICMOS (right panel) ... The bluer shade along the edges of the Martian disk in the left panel is due to ...