PPT-WFC3 Spatial Scanning (

Exoplanets STScI Calibration Workshop Aug 13 2014 Peter R McCullough H 2 O H 2 O 0 th order 1 st order 2 nd order Spatially Scanned vertically Staring Mode nominal . . C. luster . L. ensing . A. nd . S. upernova survey with . H. ubble. ACS Parallels. WFC3 Parallels. 6 arcmin. = 2.2 Mpc @ z=0.5. Footprints of HST Cameras: . ACS FOV in yellow, . WFC3/IR FOV in red, . An Innovative. Multi-cycle Hubble Treasury Program to . Study the Dark Universe. Marc . Postman. Space Telescope Science . Institute. Science with HST III, Venice, Italy. October 2010. MACS 2129-0741 z = 0.57 HST/ACS image (. Kozhurina-Platais. Ω. Cen observed with the . WFC3/UVIS and IR . F606W & F160W filters. Wide . Range PA_V3 . and Large . POSTARG ±40. ”. Observations. L_Flat. and Distortion Cal Programs:. Outline. 1.) Step 1 – TV3 Calibration. 2.) Step 2 – SMOV4 (+ Cycle 17 Calibration). 3.) Step 3 – Final Calibration (present analysis). - More data. - New flat fields. - Astrodrizzle. - Precise calibration. Acknowledgments. Zach . Berta (Harvard), the P.I. of HST program 12251, “The first characterization of a Super-Earth Atmosphere,” graciously agreed to our request to use GJ 1214 also for our engineering test, program 12325. Many persons, especially Merle Reinhart, Alan Welty, and William “Bill” Januszewski (STScI) helped plan the observations. Art Bradley (SSES) and Mike Wenz (GSFC) provided FGS data and analysis. . Redshift. Galaxies . in Cluster Fields. Wei Zheng, Larry Bradley, and the CLASH high-. z. search group. High-Redshift Galaxies. Key Science Questions:. How do the first generations of galaxies build up and evolve at the earliest times?. Prof Phil Withers. Manchester X-ray imaging Facility. University of Manchester. Volume Scanning. Computer Tomography (CT). The great advantage of computer tomography is that not only do you get the external surface geometry you capture any . An Innovative. Multi-cycle Hubble Treasury Program to . Study the Dark Universe. Marc . Postman. Space Telescope Science . Institute. Science with HST III, Venice, Italy. October 2010. MACS 2129-0741 z = 0.57 HST/ACS image (. Flyer 1. What event is advertised here?. How do you know?. Do you have to pay to come here?. What are the activities?. Flyer 2. What is the event advertised?. Date?. Time?. Activities?. Important Reading Skills. Imagery. Forming . a picture in the mind without sensory . input. Mental imagery. Visual imagery. Paivio. , Smyth and . Yuille. (1968. ). Subject studied word-pairs with each member varying in imagery. Protect from. Target acquisition and information gathering. footprinting. scanning. enumeration. initial access. privilege escalation. covering tracks. Footprinting. gathering target information. profile of security posture. Harald Kuntschner. Martin . Kümmel. , Jeremy Walsh (ST-ECF). Howard . Bushouse. (. STScI. ). Grism Workshop, . STScI. November 15, 2010. WFC3. UV Channel. IR Channel. Filter wheels with . WFC3 grisms. (g) Candidates should be able to show an understanding of how the image of an 8-voxel cube can . be developed . using CT scanning.. X-ray: The beginning . X-Rays . discovered . in 1895 by Wilhelm Conrad Roentgen . March 9, 2016. Considerations:. What size originals will you be scanning :. . 35mm slides, mounted. . 35mm slides, unmounted – rolls. . 35mm negatives color. . 35 mm negatives BW.