HST Quarterly Review Page 1 Space Telescope Science Institute 15 October 2003 SI Status: COS STScI COS Program Activity SubprojectSTScI Activity Instrument.

Slides:

Advertisements

Similar presentations

Early Results from the COS Time-Dependent Spectroscopic Sensitivity Programs Rachel Osten TIPS presentation, Jan. 21, 2010.

Advertisements

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Science Calibration & Instrument Status TIPS 20 Nov 2003 Last COS TIPS Aug 2003.

Post-SM4 Sensitivity Calibration of the STIS Echelle Modes Azalee Bostroem With help from: Ralph Bohlin, Alessandra Aloisi, Charles Proffitt, Kenneth Hart,

November 13, 2003COS Preship Review1 Resolution Specification Definition of resolution –In all cases the resolution is defined as , where  is the FWHM.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA TIPS / COS Update The NUV Gratings 18 October 2007 Last COS TIPS presentation: 21 December.

Initial Alignment Check / Calibration in Vacuum Dennis Ebbets With substantial contributions from Tom Delker, Erik Wilkinson, Steve Osterman, Ken Brownsberger,

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 21 August 2001.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA Cosmic Origins Spectrograph Hubble Mission Status Review Charles D. (Tony) Keyes Last Review:

STIS Closeout Plan Paul Goudfrooij 2005 HST Calibration Workshop, 10/26/2005.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA TIPS / COS TV Update 21 December 2006 Agenda Agenda Testing Setup and Status Testing Setup.

Cosmic Origins Spectrograph Hubble Space Telescope James C. Green University of Colorado Cosmic Origins Spectrograph Instrument Design and Capabilities.

Page 1. Page 2 SMOV Status SMOV is proceeding on-track Key programs executed –ERO program –Geometric distortion program completed –ACS to FGS alignment.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Status FUV Detector “1-bounce design” NUV Detector HST aberration fully-corrected Calibration.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS TAGFLASH System Requirements Review COS Lamp Lifetime Estimates for TAGFLASH Scenarios.

Keyes - 5 Mar 2001 Slide 1 of 16 COS Science Team Meeting – STScI Status  STScI Integrated Scheduling System Development – TIME-TAG (primary science mode)

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 20 October 1999.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA An Update on the COS Development Status TIPS 21 August 2003 (Last COS TIPS: Dec 2002) COS Integrated.

COS PIPELINE PDR Daryl Swade December 7, 2000OPUS / OTFR Space Telescope Science Institute 1 of 24 Science Data Processing

NIRSpec Operations Concept Michael Regan(STScI), Jeff Valenti (STScI) Wolfram Freduling(ECF), Harald Kuntschner(ECF), Robert Fosbury (ECF)

HST Quarterly Review Page 1 Space Telescope Science Institute 12 February 2004 SI Status: COS STScI Support of COS Thermal-Vacuum Testing COS Thermal-Vacuum.

18 May 2006 Slide 1 of 10 STScI TAGFLASH Ground System Development Current ground system could support immediate COS launch Current ground system could.

Figure 8.Color map of the geometric correction along the dispersion axis for segment A. Figure 4. Measured distortions for all PSA positions for segment.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA Hubble Mission Status Review Charles D. (Tony) Keyes Last Review: 10 June August 2003.

TIPS COS Overview - Keyes : 18 May 2000 COS Overview v CDR: April 2000 v FUV delivery: January 2001 v Environmental (Thermal-Vac): spring 2002 v Launch:

The Status of COS Flat Fields Tom Ake TIPS 21 August 2008.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Pipeline Calibration Outline of CALCOS Processing Steps and Keywords Reference Files Associations.

Performance of the Space Telescope Imaging Spectrograph after SM4 Charles R. Proffitt, A. Aloisi, K. A. Bostroem, C. R. Cox, R. I. Diaz, W. V. Dixon, P.

1-D Flat Fields for COS G130M and G160M Tom Ake TIPS 17 June 2010.

COS signal to noise capabilities Limitation of COS S/N No good 2-D flat available. Fixed pattern noise dominates COS spectra. An uncalibrated COS spectrum.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 15 January 2002.

Cosmic Origins Spectrograph

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Pipeline Calibration Goals of CALCOS Association Table Input and Output Files High Level.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA An Update on the COS Development Status TIPS 21 August 2003 (Last COS TIPS: Dec 2002) COS Integrated.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Pipeline PDR File Structure Overview Charles D. (Tony) Keyes 7 December 2000.

TIPS COS Status: SMOV update III STScI/CU COS Team 17 September 2009.

COS Training Series II. Optimizing Observations --- David Sahnow February mm.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA Cosmic Origins Spectrograph Status STIC 13 February 2001.

"Data contained herein is exempt from ITAR regulations under CFR 125.4(13) -- data approved for public disclosure." 19 Sept, 2002TIPS – WFC3 Status 1 -UVIS.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA SMOV4 Requirements Review Cosmic Origins Spectrograph Scott D. Friedman STScI 30 July 2003.

Slide 1 of 5 COS Monthly Status Review David Soderblom STScI

COS PIPELINE CDR Jim Rose July 23, 2001OPUS Science Data Processing Space Telescope Science Institute 1 of 12 Science Data Processing

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 17 September 2002.

Click to Change Title Here is a text box to present information in paragraph format, instead of bulleted lists. We’ve left space to the right for an image.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Pipeline Critical Design Review July 2001.

WFC3 COS 5 th COS/WFC3 FSW/GS Splinter Meeting Baggett - 03 April 2002 Slide 1 of 8 SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA 5 th COS/WFC3.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA Cosmic Origins Spectrograph Hubble Mission Status Review Charles D. (Tony) Keyes Last Review:

The Status of HST/COS and HST/STIS Cristina Oliveira 8/12/14COS and STIS Cal Workshop1 SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA.

WFC3 PIPELINE CDR Jim Rose October 16, 2001OPUS Science Data Processing Space Telescope Science Institute 1 of 13 Science Data Processing

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.

COS OPUS/HDA CDR Daryl Swade July 23, 2001Keywords and Associations Space Telescope Science Institute 1 of 14 Keywords and Associations.

23-Nov-1999STScI Projects Monthly Status Review1 of 8 SpaceTelescopeScienceInstitute COS Status Report for period December, 1998 to November, 1999 Tony.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 24 October 2007.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS TAGFLASH System Requirements Review CALCOS Requirements Philip E Hodge 14 December 2005.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA TIPS / COS 17 January 2002.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 15 September 1999.

Cosmic Origins Spectrograph November 13, 2003 Page 1 “Data contained herein is exempt from ITAR regulations under CFR 125.4(13) -- data approved for public.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 22 April 2002.

Keyes – 1 February 2000 : Slide 1 of 6 COS Monthly Status Review v OP-01 updates and revisions – STScI and IDT schedule and agenda for continuing COWG.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA COS Monthly Status Review 22 January 2003.

1 COS SI Testing and Delivery SI formally delivered to HSTP in May  N 2 purge alignment and NUV throughput testing pre- and post-ship  No effective alignment.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA TIPS Cosmic Origins Spectrograph 20 September 2001.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA Cosmic Origins Spectrograph HST Quarterly Review – Instrument Status Charles D. (Tony) Keyes.

Cosmic Origins Spectrograph Monthly Status Review 17 April 2001 Charles D.(Tony) Keyes Page 1 of 10 Synopsis Role: STScI supports COS science operations.

Cosmic Origins Spectrograph Monthly Status Review 19 June 2001 Charles D.(Tony) Keyes Page 1 of 10 Synopsis Role: STScI supports COS science operations.

SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA TIPS / COS 27 June 2002.

Characterization of the Post-Launch Line Spread Function of COS

Single Object & Time Series Spectroscopy with JWST NIRCam

JWST NIRCam Time Series Observations

COS FUV Flat Fields and Signal-to-Noise Characteristics

Calibration of the Cosmic Origins Spectrograph

Presentation transcript:

HST Quarterly Review Page 1 Space Telescope Science Institute 15 October 2003 SI Status: COS STScI COS Program Activity SubprojectSTScI Activity Instrument Development IDT/STScI MOU I & T Ball (Thermal-Vac support) Commanding and Scheduling System OP-01 Ops bench testing Pipeline and Calibration keyword development pipeline development SM4 planning User Support COS ETCs Instr. Handbook development COS activities are a traditional-mode, new HST instrument development project coordinated with IDT led by PI Jim Green (Colorado) STScI supports COS science operations by leading development of “front- end” (operations) and “back-end” (OPUS/MAST/calibration) ground system and user support functions..

HST Quarterly Review Page 2 Space Telescope Science Institute 15 October 2003 SI Status: COS STScI Support of COS Thermal-Vacuum Testing COS Initial Alignment and Verification Thermal-Vac at Ball: 25 June-10 July COS Thermal-Vacuum Science Calibration at Ball: 22 Sep-21 Oct  NUV testing complete; FUV commences 10 Oct STScI Thermal-Vac planning and participation  Close coordination of STScI support activities with IDT  All STScI COS Instrument Scientists provide onsite support for SI operation, data- taking, and analysis  Keyes, Sembach, Leitherer, Friedman, and Bohlin stand multiple-day shifts during initial alignment and science calibration Thermal-Vacuum activities; Hartig will “float”  Hartig provides onsite optical alignment support  Per STScI/COS IDT MOU STScI provides OPUS processing, conversion to FITS, and HDA-archival of all COS Thermal-Vacuum data  Processed approximately 520 datasets from initial alignment and verification activities  Processed approximately 1200 science calibration datasets to date STScI post-test analysis activities  Repeatability monitor (Friedman): no anomalies in verification testing  Flat fields (Bohlin): verified 1% flatfield and 1% rms per pixel in extracted absorption line spectrum  Keyword processing anomalies (Sembach, Keyes, Friedman, Hartig, Hodge)

HST Quarterly Review Page 3 Space Telescope Science Institute 15 October 2003 SI Status: COS STScI Ground Systems and User Support Activities STScI scheduling system  Flat field commanding updates implementation and local testing completed  Bench testing of timing and commanding for all FUV and NUV exposure modes except target acquisition completed  Coordinated parallels now in requirements definition Delivered updated Cycle 13 COS mini-Handbook (Sembach); includes post-verification updates Spectroscopic APT/ETC implementation underway SMOV4 requirements defined (Friedman, Keyes); reviewed and approved by HSTP Supported SM4 BEA review (Keyes) STScI COS Bright Object Protection checking software for user support (ROBOT) development underway

HST Quarterly Review Page 4 Space Telescope Science Institute 15 October 2003 SI Status: COS Sample COS FUV Spectrum “A” Segment Note: segment “B” (not shown) records remaining half of bandpass Internal PtNe calibration lamp (no distortion correction)

HST Quarterly Review Page 5 Space Telescope Science Institute 15 October 2003 SI Status: COS Internal PtNe calibration lamp Sample COS NUV Spectrum Note: 3 stripes are not continuous in wavelength

HST Quarterly Review Page 6 Space Telescope Science Institute 15 October 2003 SI Status: COS Initial NUV External Flatfield Results (September 2003) COS G185M NUV P-flat (Bohlin) 1.36% Poisson rms Pixel (cross-dispersion) Pixel (dispersion) Intrinisic detector scatter (1  3.25%) within the 100x100 pixel box shown in dashed lines 20, ,000 counts per pixel in each stripe C B A Pixel (dispersion)

HST Quarterly Review Page 7 Space Telescope Science Institute 15 October 2003 SI Status: COS Initial NUV External Flatfield Results (September 2003) rms deviation from unity ratio characterizes S/N Normalized ratio of first half of exposure to second half (Friedman)

HST Quarterly Review Page 8 Space Telescope Science Institute 15 October 2003 SI Status: COS TA1 Image (NUV) Double pinhole aperture 1” (~40 pixels) separation Dispersion (pixels) Cross Dispersion (pixels) Images are clearly resolved Initial Spatial Resolution Results (July 2003)