PPT-The New WFC3 Photometric Calibration

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. . 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 (. (FNAL). DES Director’s Council Review. 10-11 May 2011. Calibration Plan for Early DES Data . Basic DES Observing Strategy. Survey Area. Overlap with SDSS . Stripe 82 (200 sq deg) . Connector region. 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:. . 17 . April. 2012. Outline:. Basic Strategy. Evolving Strategy. Particular Problems for Year 1. A . Call to Cooperate. Photometric Calibration Strategy . of the Dark Energy Survey (DES). Douglas L. Tucker. RESEARCH. q. uality and quantity. Paul Dowling. Institute of Education. University of London. Photometric . redshifts. can be routinely obtained to accuracies of better than 0.1 in Deltaz/(1 +. z. ). The issue of dust extinction, however, is one that has still not been well quantified. In this paper the success of two template-fitting photometric . Data Flow. Jason Surace. IPAC/Caltech. Complicated Data Path. Data flows through multiple pipelines, creating a variety of science products tailored for different purposes. These pipelines operate on multiple timescales. What data you want depends in large part on what science you want to do.. 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?. 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). . 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 (. 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. Announcements. Project 4 (stereo) released today, due Friday, April 1, at 8pm. To be done in groups of 2. Recap: . Lambertian (Diffuse) Reflectance. I . : observed image intensity. k. d. . : object albedo. Add 12 event classes for SVX detector. .  . Done. Generate calibration parameters for Q-vector and flattening run by run .  . on-going. Status of centrality calibration. The calibrations for run-343031-347349 are good to use..