An Unexpected Hysteresis Effect Seen in Hawaii-2RG Detectors

Slides:



Advertisements
Similar presentations
A NEW CTE PHOTOMETRIC CORRECTION FORMULA FOR ACS Marco Chiaberge TIPS meeting 05/16/2012.
Advertisements

25th CoRoT Scientific Council : sept M.O. - L.J. Evaluation of exo N1 data M.Ollivier - L Jorda.
Observational techniques meeting #7. Detectors CMOS (active pixel arrays) Arrays of pixels, each composed on a photodetector (photodiode), amplifier,
Precision Spectroscopy: some considerations S. Deustua STSCI 2014 STSCI Calibration Workshop 1.
Proposed CalJWST Structure M. Robberto. Cross-Instrument Rationale 2 level processing  CALinsA: from RAMP to calibrated images  CALinsB: associated.
SDW Marco Sirianni Marco Sirianni (ESA/STScI) Max Mutchler (STSci) Radiation Damage in HST Detectors.
ACS/WFC Geometric Distortion and CTE V. Kozhurina-Platais & ACS team.
Following the Photons… Empirical, Pixel-Based Corrections for CTE Jay Anderson STScI October 12, 2011 Back-Tracking the Electrons.
Towards Creation of a JWST Astrometric Reference Field: Calibration of HST/ACS Absolute Scale and Rotation Roeland van der Marel Jay Anderson, Colin Cox,
Astrometry for NGAO Brian Cameron, Matthew Britton, Jessica Lu, Andrea Ghez, Rich Dekany, Claire Max, and Chris Neyman NGAO Meeting #6 April 25, 2007.
Introduction to Spitzer and some applications Data products Pipelines Preliminary work K. Nilsson, J.M. Castro Cerón, J.P.U. Fynbo, D.J. Watson, J. Hjorth.
We have the first, direct measure of photometric loss due to imperfect CTE on ACS.
S. Baggett, J. Anderson, K. S. Long, J. W. MacKenty, K. Noeske, J. Biretta, and the WFC3 team (STScI) WFC3 : Understanding and mitigating UVIS charge.
0. To first order, the instrument is working very well ! 1.Evolution of the IR detector with time 2.Stability of the L channel 3.Saturation 4.Linearity.
Distortion in the WFC Jay Anderson Rice University
STATUS REPORT OF FPC SPICA Task Force Meeting March 29, 2010 MATSUMOTO, Toshio (SNU)
Progress Report on PSFs and Pixels Jay Anderson, Elena Sabbi, Kailash Sahu, and Matthew Bourque TIPS Feb 19, 2015.
+ AstroDrizzle Products for HST & JWST 2014 STScI Calibration Workshop Jennifer Mack, STScI.
NIRSpec Operations Concept Michael Regan(STScI), Jeff Valenti (STScI) Wolfram Freduling(ECF), Harald Kuntschner(ECF), Robert Fosbury (ECF)
AST 443/PHY 517 : Observational Techniques November 6, 2007 ASTROMETRY By: Jackie Faherty.
2004 January 27Mathematical Challenges of Using Point Spread Function Analysis Algorithms in Astronomical ImagingMighell 1 Mathematical Challenges of Using.
ACS Drizzling Overview J. Mack; DA Training 10/5/07 Distortion Dither Strategies MultiDrizzle ‘Fine-tuning’ Data Quality Photometry.
JWST Calibration Error Budget Jerry Kriss. 15 March 20072/14 JWST Flux & Wavelength Calibration Requirements SR-20: JWST shall be capable of achieving.
The Status of HST/WFC3 John W. MacKenty Space Telescope Science Institute 12 August 2014 Calibration Workshop.
ACS/WFC CTE correction for point source photometry Marco Chiaberge ACS Team STScI.
The Hubble Space Telescope explores the limits of “roundness”: Ceres and Vesta Max Mutchler (Space Telescope Science Institute), Lucy McFadden, Jian-Yang.
1 Space Telescope Science Institute JWST S&OC JWST S&OC Contract Peter Stockman TIPS March 20, 2003.
1 ACS Press Releases Science  Grism spectroscopy of UDF galaxies  Mass of the MACHO-LMC-5 lens  Earliest star-forming galaxies in UDF  Kepler’s SNR.
TIPS - Oct 13, 2005 M. Sirianni Temperature change for ACS CCDs: initial study on scientific performance M. Sirianni, T. Wheeler, C.Cox, M. Mutchler, A.
MOS Data Reduction Michael Balogh University of Durham.
The Second Generation of IR detectors for WFC3 Massimo Robberto European Space Agency and Space Telescope Science Institute.
11-Jun-04 1 Joseph Hora & the IRAC instrument team Harvard-Smithsonian Center for Astrophysics The Infrared Array Camera (IRAC) on the Spitzer Space Telescope.
WFC3 SMOV Report for TIPS 16 July 2009 John MacKenty This presentation contains material that is embargoed until after the SM4 ERO press conference. Images/spectra.
Progress Report on Modeling CTE in ACS/WFC TIPS May 19, 2011 Jay Anderson.
Calibration for WFPC2 Vera Platais Astrometric X g =a 1 +a 2 X+a 3 Y+a 4 X 2 +a 5 XY+a 6 Y 2 +a 7 X 3 +a 8 X 2 Y+a 9 XY 2 +a 10 Y 3 Y g =b 1 +b 2 X+b.
1 WFC3 – Critical Science Review Science Driven CEIs Requirements.
Selection and Characterization of Interesting Grism Spectra Gerhardt R. Meurer The Johns Hopkins University Gerhardt R. Meurer The Johns Hopkins University.
Image Stability  ACS SMOV image stability test (prop 9017) went from a cold soak (anti-solar pointing) for 8 orbits to a hot attitude (including off-nominal.
François Rigaut, Gemini Observatory GSMT SWG Meeting, LAX, 2003/03/06 François Rigaut, Gemini Observatory GSMT SWG Meeting, LAX, 2003/03/06 GSMT AO Simulations.
SMOVSMOV  ACS has now completed SMOV Program –Transitioned to interim calibration plan  Final SMOV programs –Further coronagraph calibration –Coronagraph.
STScI TIPS, 15 January 2004MultiDrizzle Overview - Anton Koekemoer1 MultiDrizzle Status and Development Overview Anton Koekemoer, ACS+WFPC2 Branch Project.
HST Cal Conf -- Oct 27, Calibration Status and Results for Wide Field Camera 3 – R. Kimble/GSFC, Calibration Status and Results.
The STIS NUV-MAMA objective prism … … and looking beyond for HST UV slitless spectroscopy Jes ú s Ma í z Apell á niz HST Calibration worskhop 26 October.
Improved ACS Geometrical Distortion Correction Richard Hook TIPS Meeting, STScI, 18th December 2003.
Application of a Charge Transfer Model to Space Telescope Data Paul Bristow Dec’03
S. Baggett, J. Anderson, J. MacKenty, J. Biretta, K. Noeske, and the WFC3 team (STScI) HST/WFC3 UVIS Detectors: Radiation Damage Effects and Mitigation.
WFC3 SMOV UVIS and IR Geometric Distortion Calibration and Multidrizzle Vera Kozhurina-Platais and WFC3 team.
A. Ealet Berkeley, december Spectrograph calibration Determination of specifications Calibration strategy Note in
Single Object Spectroscopy and Time Series Observations with NIRSpec
JWST-MIRIM (The MIRI Imager)
NIRCam Readout Pattern Considerations
Alex Fullerton STScI / NIRISS Team Lead
Single Object Slitless Spectroscopy Simulations
JWST FGS Guide Star Studies
NIRSpec Time Series Observations
Imaging with the James Webb Space Telescope
JWST Pipeline Overview
Single Object & Time Series Spectroscopy with JWST NIRCam
Time Series Observations with MIRI
NIRSpec simulation data-package
ESAC 2017 JWST Workshop JWST User Documentation Hands on experience
Summary Single Object & Time Series Spectroscopy Jeff Valenti JWST Mission Scientist Space Telescope Science Institute.
The Medium Resolution Spectrometer on behalf of the MRS team
ESAC 2017 JWST Workshop NIRSpec MSA Planning Tool (MPT)
The art of imaging with Hubble
GPI Astrometric Calibration
MIRI Observing Templates
Astronomical Observational Techniques and Instrumentation
ACS PSF Variations Over The Field of View & ACS Coronagraph Status
Observational techniques meeting #6
Presentation transcript:

An Unexpected Hysteresis Effect Seen in Hawaii-2RG Detectors Background Distortion calibration important for JWST Coronagraphy, MSA, slits Self-calibration will be difficult ACS field observed in 2006 In LMC, in JWST’s CVZ 55: big enough for all detectors Good density of stars Many well-measured stars More than 100,000 good to 1 mas Good, but… Not big enough for cross-calibration No IR color information 17" Jay Anderson --- TIPS Feb 21, 2008 J1

Ground-based Observations HAWK-I: new IR camera Being commissioned on VLT at Paranal 7.57.5 FOV 22 mosaic of 20482048 NIR detectors “Active optics” Luigi Bedin (STScI) observed the JWST field For them: exquisite distortion solution For us: IR photometry & larger field We got an additional benefit… Jay Anderson --- TIPS Feb 21, 2008 J2

HAWK-I distortion: After global correction: Raw residuals One chip J3 x x One chip x x x x x x Jay Anderson --- TIPS Feb 21, 2008 J3

Periodic residuals Same throughout detector Periodogram Square wave Phase Diagram Phase Diagram Same throughout detector Periodogram Square wave removes periodic signature Jay Anderson --- TIPS Feb 21, 2008 J4

Why do we care? Rockwell Scientific HAWAII-2RG Very important to Prototype for JWST! Very important to understand the source Geometric, like HST? WFPC2’s 34-row effect ACS/WFC’s 68-column effect Check flat fields No evidence WFC FLAT FIELDS HAWK-I Jay Anderson --- TIPS Feb 21, 2008 J5

Why do we care? Rockwell Scientific HAWAII 2RG 32 amplifiers  AMP#0 AMP#1 AMP#2 AMP#3 AMP#4 Rockwell Scientific HAWAII 2RG Prototype for JWST! Very important to understand the source Geometric? No! Readout artifact? HAWK-I Readout CTE-like hysteresis PSF asymmetry? Look at CRs… Likely cause pixel dwell time All CRs Even Amps Odd Amps inter-pixel capacitance Jay Anderson --- TIPS Feb 21, 2008 J6

Possible Implications for JWST JWST will have four amplifiers four 512-pixel zones Not clear if effect comes before or after the amplifiers… Really a problem? How to deal with hysteresis? Mild deconvolution? (will amplify noise) Leave in, but model Similar to the inter-pixel capacitance Effective PSF will treat it implicitly as (x,y) Need to study impact on: subarray mode, guider, spectra, dithering, noise model Early NIRCam/U.AZ tests encouraging! Jay Anderson --- TIPS Feb 21, 2008 J7