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. Chin-Jen Lin, George Liu. Institute of Earth Sciences, Academia . Sinica. , Taiwan. Outlines. Calibration . of the following rotational sensors. R-1 . R-2. Two applications to find . true north. Attitude . 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:. A. . Pasewaldt. 1. , . K. . Willner. 2. , . J. . Oberst. 1,2. , . Frank . Scholten. 1. , . M. . Wählisch. 1. , . K.-D. . Matz. 1. , . T. . Roatsch. 1. , . H. . Hoffmann. 1. , . A. . Grechishev. 3. . 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 . 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. . 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 (. Matt Galloway. 2. Volumetric water content . sensors. measure volumetric water content, right?. Do thermometers measure temperature?. 3. Temperature is measured by its effect on the physical properties on some substance. Craig Markwardt & Bev . LaMarr. GSFC. PI: Keith . Gendreau. , NASA GSFC . Science: . Understanding ultra-dense matter via soft X-ray timing spectroscopy of neutron stars . Platform: International Space Station . &. . adaptive power supply. *. J. Cvach. *,. Institute of Physics, ASCR, . PraGUE. Introduction. LED driver. Notched fibres. Adaptive power supply. Summary . _______________________________________. Radon Symposium. San Diego, California. September 21, 2016. Phillip H. Jenkins, PhD, CHP. Bowser-. Morner. , Inc.. Melinda . Ronca. -Battista. Tribal Air Monitoring Support Center, NAU. We Take it For Granted. Presenter: Phillip S. Kott . 1. WSS. . . R . d. k. . [1 . exp. (. x. k. T. g. )]. . z. k. = . T. z . .   . Corresponding author Calibration is an important process for continuity reliability ages from different has been performed before launch in most cases on-orbit calibration should be done especially 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.