LBC-Blue pre-commissioning LBC-Blue LBC-Blue –E Giallongo (PI) Rome: diPaola, Pedichini, Speziali, Testa, Gallozzi Rome: diPaola, Pedichini, Speziali,

Slides:



Advertisements
Similar presentations
GSMT Control Workshop Tucson, September 11-12, 2001 Pointing Control for a giant segmented mirror telescope Patrick Wallace Rutherford Appleton Laboratory.
Advertisements

CMSC 2006 Orlando Active Alignment System for the LSST William J. Gressler LSST Project National Optical Astronomy Observatory (NOAO) Scott Sandwith New.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
1 Laser Beam Coherence Purpose: To determine the frequency separation between the axial modes of a He-Ne Laser All sources of light, including lasers,
LBT AGW units Design Review Mar.2001 General Concept Performance specifications and goals The off-axis unit The mechanical support structure The control.
ENERGY a proposal for a Multi-channel Cmos Camera F. Pedichini, A. Di Paola, R. Speziali INAF Oss. Astr. Roma h e-
Etendue is inversely proportional to survey time for a very wide-field survey; it is scaled so that IWI is 100. VISTA and UKIRT/ WFCAM have large gaps.
WFS Preliminary design phase report I V. Velur, J. Bell, A. Moore, C. Neyman Design Meeting (Team meeting #10) Sept 17 th, 2007.
SDW20051 Vincent Lapeyrère LESIA – Observatoire de Paris Calibration of flight model CCDs for CoRoT mission.
The Camera and Photography
CAMERAS AND LENSES The Essential Reference Guide for Filmmakers.
Agile: A Time-Series CCD Photometer to Study Variables Anjum Mukadam, Russell Owen, Ed Mannery University of Washington, Seattle.
1 LBT Web Services and Scheduler We present several LBT web tools to plan organize and schedule observations. Authors: Stefano Gallozzi Diego Paris Adriano.
NEO Research Project in Korea Wonyong Han 1, Yong-Ik Byun 2, Hong-Suh Yim 1, Young-Jun Choi 1, Hong-Kyu Moon 1 & NESS Team 1 Korea Astronomy and Space.
Michigan/MIKE Fiber System (MMFS) – Update Apr 2005.
Advanced Concepts & Science Payloads Office Eddicam/EST MeetingPage 1 CCD Procurement Schedule driven Review off-the shelf availability Specific mode of.
SPECTROSCOPIC DIAGNOSTIC COMPLEX FOR STUDYING PULSED TOKAMAK PLASMA Yu. Golubovskii, Yu. Ionikh, A. Mestchanov, V. Milenin, I. Porokhova, N. Timofeev Saint-Petersburg.
Presentation EddiCam consortium, FF, Madrid 13/06/2002 Eddington programmatic status Fully approved by SPC as part of ESA’s science program as project.
STATUS REPORT OF FPC SPICA Task Force Meeting March 29, 2010 MATSUMOTO, Toshio (SNU)
PACS IIDR 01/02 Mar 2001 FPFPU Alignment1 D. Kampf KAYSER-THREDE.
NIRCam ETU Testing at LMATC, Palo Alto Kailash C. Sahu.
Astrophotography The Basics. Image Capture Devices Digital Compact cameras Webcams Digital SLR cameras Astronomical CCD cameras.
Telescope Guiding with a HyViSI H2RG Used in Guide Mode Lance Simms Detectors for Astronomy /2/09.
MARS Design Review PP-1 Requirements Definition Performance: –Tip/Tilt error < 0.06″ rms mirror coordinates 0.12″ rms image coodinates 0.28″ fwhm image.
Telescope Integration and Tests Tuesday Afternoon.
FLAO system test plan in solar tower S. Esposito, G. Brusa, L. Busoni FLAO system external review, Florence, 30/31 March 2009.
NIRSpec Operations Concept Michael Regan(STScI), Jeff Valenti (STScI) Wolfram Freduling(ECF), Harald Kuntschner(ECF), Robert Fosbury (ECF)
SAM PDR1 S OAR Adaptive Module LGS LGSsystem Andrei Tokovinin SAM LGS Preliminary Design Review September 2007, La Serena.
Subaru/FMOS Commissioning: Brief history & current status Naoyuki Tamura Instrument scientist Subaru Telescope, NAOJ Expected performance Observation “A.
January 25, 2005GRETINA 2004 Review1 GRETINA 2004 Annual Review Steve Virostek Lawrence Berkeley National Lab Mechanical System.
20 October 2008LBT Q Eng/SW Review0 PCS – Pointing Control Subsystem Michele De La Peña.
AST3-1 photometry from Dome A Bin Ma, Peng Wei, Yi Hu, Zhaohui Shang NAOC AST3
The Prime Focus Imaging Spectrograph Design and Capabilities
The Active Optics System S. Thomas and the AO team.
1 BROOKHAVEN SCIENCE ASSOCIATES Storage Ring Commissioning Samuel Krinsky-Accelerator Physics Group Leader NSLS-II ASAC Meeting October 14-15, 2010.
1 Optical observations of asteroids – and the same for space debris… Dr. D. Koschny European Space Agency Chair of Astronautics, TU Munich Stardust school.
Oct 26, 2007SALT Workshop UKZN1 Robert Stobie Prime Focus Imaging Spectrograph Science Rationale Modes –Fabry-Perot Spectral Imaging –Grating Spectroscopy;
Digital Camera TAVITA SU’A. Overview ◦Digital Camera ◦Image Sensor ◦CMOS ◦CCD ◦Color ◦Aperture ◦Shutter Speed ◦ISO.
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.
Web Image Simulator Stefano Gallozzi & LBC Team Copyright © 2003.
System Performance Metrics and Current Performance Status George Angeli.
Robo-AO Overview: System, capabilities, performance Christoph Baranec (PI)
In Photography, there is an Exposure Triangle (Reciprocity Theory) Aperture – size of the iris opening, how much light come into the “window” Shutter Speed.
Observations with AMBER  General overview  P2VM  OB preparation with P2PP P2PP / OB / templates Available templates for observation procedure Typical.
Stacy Kopso, M.Ed., R.T.(R)(M).  Xray photon loses energy and changes direction  Responsible for most of the scatter that fogs the image  Related to.
The Field Camera Unit Results from technical meeting S. Scuderi INAF – Catania.
THEMIS Prototype Imager [ initial field testing ].
The Prime Focus Imaging Spectrograph for the Southern African Large Telescope: Operational Modes Chip Kobulnicky – Instrument Scientist, University of.
Motion tracking TEAM D, Project 11: Laura Gui - Timisoara Calin Garboni - Timisoara Peter Horvath - Szeged Peter Kovacs - Debrecen.
MagIC Upgrade for High-Speed Photometry Jim Elliot, MIT Magellan SAC
LBC-OB Gui User Interface v 2.0 Stable Stefano Gallozzi & LBC-Team Stefano Gallozzi & LBC-Team © Copyright 2007.
Single Object Spectroscopy and Time Series Observations with NIRSpec
Diagnostic Radiology II X-ray Tubes. Anode angle Anode angle defined as the angle of the target surface with respect to the central ray in the x-ray field.
NIRSpec Time Series Observations
Calibration meeting summary
“ Who will I blame my mistakes on. ” Dr
Relative Spectral Response and Flat Fields with Internal Calibration Lamps Luisa M. Lara IAA-CSIC Granada (SPAIN)
Single Object & Time Series Spectroscopy with JWST NIRCam
IR Detector - Test cryostat : Machining
JWST NIRCam Time Series Observations
Chris Willott, Loic Albert, René Doyon, and the FGS/NIRISS Team
ESAC 2017 JWST Workshop JWST User Documentation Hands on experience
ESAC 2017 JWST Workshop NIRSpec MSA Planning Tool (MPT)
Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph
The Pixel Hybrid Photon Detectors of the LHCb RICH
MIRI Observing Templates
Karen Meech Institute for Astronomy TOPS 2003
Echidna: current status and expected performance
MIRI Low Resolution Spectroscopy
Deep Sky Imaging with SharpCap
Presentation transcript:

LBC-Blue pre-commissioning LBC-Blue LBC-Blue –E Giallongo (PI) Rome: diPaola, Pedichini, Speziali, Testa, Gallozzi Rome: diPaola, Pedichini, Speziali, Testa, Gallozzi Arcetri/Padova/Bologna: Ragazzoni (co-PI), Barufollo, Diolaiti Arcetri/Padova/Bologna: Ragazzoni (co-PI), Barufollo, Diolaiti Trieste: Smareglia, Gasparo Trieste: Smareglia, Gasparo –field of view, filters –taking data: preparing & executing the observations Two pre-commissioning runs this year: Two pre-commissioning runs this year: –Summer (May – mid-July) –Fall (mid-Sept to present) leading up to LBC-Blue commissioning late October

Opto-mechanical Design

LBC-Blue: focal plane x 4608 pix ‘science’ chips x 4608 pix ‘science’ chips –0.23”/pxl (7.85’ x 17.7’ per chip) –separated by 80 pxl (18”) gaps –~ 27’ x 27’ field of view x 2048 pix ‘technical’ chips x 2048 pix ‘technical’ chips –first 256 lines masked to be used without shutter (~frame transfer CCDs) –fast readout: 1.2s for the 256x2048 area –1’ x 7.85’ field of view –for guiding & active optics all behind shutter & filter all behind shutter & filter from “LBC Blue Channel: The CCD Camera” (Giallongo (PI), Speziali, diPaola, Pedichini, Ragazzoni (co-PI)& LBC team)

Wavelength coverage Filters intended (8/channel at one time) Filters intended (8/channel at one time) –LBC-Blue: Bessel U,B,V Bessel U,B,V Sloan g’, r’ (u’ to be added) Sloan g’, r’ (u’ to be added) –LBC-Red: Bessel V, R, mod-I Bessel V, R, mod-I Sloan r’,z’ (i’ to be added) Sloan r’,z’ (i’ to be added) NB 910nm/30nm fwhm (under consideration) NB 910nm/30nm fwhm (under consideration) Sensitivities Sensitivities –ETC gives 5  -1hr for 0.9” seeing, 1.8” SW aperture, no moon, airmass = 1.3: B~27.1, U~25.4, V~26.9 B~27.1, U~25.4, V~26.9 First light image at B consistent with estimate from ETC. First light image at B consistent with estimate from ETC. –Estimates only! to be measured during commissioning…

Preparing Observing Blocks   OB tool runs on Linux & Windows (Gallozzi)   set pointing, position angle   configure Blue & Red channel: dither pattern, exposure time, Nexp   Writes out xml file

Executing Observing Blocks LBC Control SW:   Runs from firefox browser   Uploads OB   Executes observation   Interfaces with TCS: slews, obtains rotator trajectory, dithers   Guiding for exposures longer than a given threshold (~30sec)   Technical chip exposures 2,4,8,…sec taken   Automatically searched for stars; when sufficient stars found, starts guiding

Focus & Collimation   Slew to target   Execute OB to move M1 down by 0.8mm (60pxl pupil)   Obtain 15-20s image using a ~1000 line window of chip 2   Analyze with IDL algorithm (Barufollo & Ragazzoni):   Automatically finds bright isolated pupils   computes Zernike coefficients   sends the results to the TCS/PSF which adjusts mirror position & forces   2-3 iterations to achieve focus & collimation   Frequency of focus/collimation? TBD, depends on accuracy of collimation lookup table

Summer (May to mid-July) pre-commissioning CCD Controllers (Pedichini, Skytech) CCD Controllers (Pedichini, Skytech) –Returned from Rome/Skytech –Source of pickup noise tracked down and eliminated Decreased image transfer time (diPaola & Smareglia) Decreased image transfer time (diPaola & Smareglia) –105s total: 26 s readout (41 s readout & demultiplexing) 26 s readout (41 s readout & demultiplexing) transfer from LBC CMU to archive and from transfer from LBC CMU to archive and from LBC archive to user machine LBC archive to user machine Development of single extra-focal image analysis algorithm (Barufollo & Ragazzoni) Development of single extra-focal image analysis algorithm (Barufollo & Ragazzoni) MAT (4” rms) and LBC (7.6” rms) pointing models MAT (4” rms) and LBC (7.6” rms) pointing models First collimation lookup table made First collimation lookup table made –Mirror position (x,y,z,rx,ry) vs elevation for about a dozen datapoints. Outstanding Issues in mid-July: Outstanding Issues in mid-July: –rotator cable chain buckling –Focal plane tilt (100 microns) which had existed since fall 2005.

Fall (Sept – late Oct) pre-commissioning New rotator cable chain installed New rotator cable chain installed Fixed focal plane tilt Fixed focal plane tilt –Shimmed rotator flange by 0.38mm Guiding works Guiding works Tasks for the next two weekends: Tasks for the next two weekends: –Refinement of collimation lookup table –Refinement of pointing models (MAT and LBC) –Refinement of active optics code (Oct 19-22) LBC-Blue Commissioning to begin October 23 LBC-Blue Commissioning to begin October 23

Quantum Efficiencies from Pedichini F., Speziali, R., Diolaiti, E., Ragazzoni, R. 2002, “The Large Binocular Camera of LBT: The focal plane detectors”, (in later document, one blue chip differs; QE for this one 1-8% lower but similar shape)