PPT-1 JWST FGS

Status Update on NIRISS Observing Modes and their APT Templates Oct 20 2015 Paul Goudfrooij Reminder c urrent version of NIRISS Ops Concept Document available at httptinyurlcomq64jsut. R. epeatability. WFC3 – spatial . s. can mode analysis – . work in progress. Mark Swain, Pieter . Deroo. , . Kiri. . Wagstaff. IPAC . JWST workshop . 3/11/14. Jet Propulsion Laboratory, California Institute of Technology. . . Victoria Meadows, Eddie . Schwieterman. , . Giada. . Arney. , Drake Deming. ,. . Amit. . Misra. , Benjamin . Charnay. , Ty Robinson, . Antigona. Segura, Shawn. . JWST Community Lecture. Jay Anderson, STScI. Nov 29, 2016. Astrometric Calibration. What is Distortion?. Any “non-conformal” mapping . . (shift, scale, rotation). Linear terms (“skew”). Non-linear terms. Goddard Space Flight Center, Greenbelt MD. Joint Base Andrews, MD. Johnson Space . Center,. Houston TX. Northrop-Grumman, Los Angeles CA. Panama Canal. ESA Kourou, French Guiana. L2. JWST. Road to. The stars. Mandell. NASA GSFC. Collaborators. :. Korey. Haynes. Evan . Sinukoff. Drake . Deming. Adam Burrows. Nikku. . Madhusudhan. Mark . Clampin. Don . Lindler. Natasha . Batalha. Heather Knutson. (others as well) . of transiting planets. . Drake Deming. University of Maryland at College Park. K2 Science Conference, November 5, 2015. In the early days of transiting planets, we were interested in what JWST could . NIRCam. Grism Mode for Transit Observations. C. Beichman, Dimitra . Touli. ,. Gautam . Vasisht. , Roger Smith. Tom Greene. 4 March 2014. JWST grism simulator. 1. Caltech Detector Testbed. Caltech testbed (Roger Smith) projects simulated spectra and other images onto HgCdTe array to assess precision photometry for transits, weak lensing, etc. for Explorer concepts, JWST, WFIRST, EUCLID. . 2013 NASA Annual IV&V Workshop . Chris Lescinsky IV&V Analyst, TASC. Rick Hess, IV&V Analyst, TASC. 9/10/2013. Agenda. JWST Overview (ORBIT and ISIM). JWST Key Elements. ISIM Layout. JIST Test Bed. JWST:Coronagraphy. 2. High Contrast Imaging allows observing. Extended emission. surrounding stars. Debris disks. AGN. . hosts. Faint companions. High contrast imaging combines the suppression of light from the host (“optical cancellation”) with post-processing by subtracting the scaled point-spread function (PSF) from the science image. Space . Telescope. John . Mather . JWST . Senior Project Scientist . AAAC Oct 13 2011. JWST . Science Updates. 4 (. original) . major themes: first light, galaxy assembly, star & planet formation, evolution of planetary systems. 40 Balmer jump and slopes 4000 age Very young population x0000- emission lines UV slopes Old star populations in high-z objects eg Egami et al 2005 Eyles et al 2005 Richard et al 2011 Zeng e Optical Telescope Element (OTE). Northrop Grumman: Charlie Atkinson, Scott C. Texter. NASA/GSFC: Lee Feinberg, Ritva Keski-Kuha. July 6th, 2012. JWST Observatory Breakdown. Optical Telescope Element (OTE). PAH evolution along the stellar lifecycle. Check marks indicate the importance of PAH formation and/or destruction during each stage and if NIR emission from PAHs with deuterium and nitrogen containing side groups is predicted. CSE and . contained in this document is subject to export controls under the International Traffic in Arms Regulations (Title 22, CFR . Presented by Basil Jeffers. JWST Project Lead EEE Parts Engineer. JWST Worldwide Team/Partners. .