The 6dF VPH Upgrade and other instrumental issues Will Saunders, Martin Ostreich, Allan Lankshear, Brendan Jones, Mick Kanonczuk, Kristin Fiegert, John.

Slides:



Advertisements
Similar presentations
© Smart Fibres Ltd SmartScan FBG Interrogator Features and Benefits.
Advertisements

1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
SALT RSS-NIR MID-TERM REVIEW MAY 20 & 21, 2009 ANALYTIC OPTICS KENNETH NORDSIECK UNIVERSITY OF WISCONSIN.
1 WHT 2 Degree Field Forward Cass, Prime Focus correctors, multi-object spectrographs David King Institute of Astronomy University of Cambridge Science.
Strecher, compressor and time structure manipulation
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
Spectral Resolution and Spectrometers
Echelle Spectroscopy Dr Ray Stathakis, AAO. What is it? n Echelle spectroscopy is used to observe single objects at high spectral detail. n The spectrum.
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
9/24/05LDP Prism description A Low Dispersion Prism for IMACS f/2 (LDP) A lower dispersion element affords more slits per mask at the expense of resolution.
RAVE MEETING BALTIMORE May 2008 Status of the 3 rd 6dF field plate and the new RAVE observing support model. Q.A.Parker (AAO/Mac.Uni) Fred Watson (AAO)
Spectral Resolution and Spectrometers A Brief Guide to Understanding and Obtaining the Proper Resolution of the 785 Raman System.
Spectroscopic Reference Design Options D. L. DePoy Texas A&M University.
Spectroscopic Data ASTR 3010 Lecture 16 Textbook Ch. 11.
Laser guide star adaptive optics at the Keck Observatory Adam R. Contos, Peter L. Wizinowich, Scott K. Hartman, David Le Mignant, Christopher R. Neyman,
Modern Correctional Facilities Need:  Robust and Reliable Data Management  Efficient data entry and manipulation  Versatile Professional Report Generation.
AURA New Initiatives Office S.C. Barden, M. Liang, K.H. Hinkle, C.F.W. Harmer, R.R. Joyce (NOAO/NIO) September 17, 2001 Instrumentation Concepts for the.
Prismswww.edmundoptics.com Right AngleEquilateralPentagonalDove.
An Echidna-style positioner for DESpec
The SKA Molonglo Prototype (SKAMP) Project SKA Meeting - April 2006 Anne Green.
An Echidna-style positioner for DESpec Will Saunders 8 March 2011.
Astronomical Spectroscopy
Spectroscopy Techniques and Projects at 1.2-m UK Schmidt Telescope
AAOmega: a scientific and optical overview Will Saunders 1 Terry Bridges 2, Peter Gillingham 1, Roger Haynes 1, Greg A. Smith.
VOLUME-PHASE HOLOGRAPHIC GRATINGS FOR ASTRONOMICAL SPECTROGRAPHS James A. Arns, Willis S. Colburn, & Mark Benson (Kaiser Optical Systems, Inc.) Samuel.
Optical Design for an Infrared Multi-Object Spectrometer R. Winsor, J.W. MacKenty, M. Stiavelli Space Telescope Science Institute M. Greenhouse, E. Mentzell,
6dF Data Release 2 The good, the bad and the ugly Will Saunders AAO 27/04/05.
AAOmega: a Multi-purpose Fiber-fed Spectrograph for the AAT Greg Smith 1 Will Saunders 1 Terry Bridges 2, Vladimir Churilov 1,
Instruments without optics: an integrated photonic spectrograph Joss Bland-Hawthorn & Anthony Horton Anglo-Australian Observatory Ground-based and Airborne.
Astronomical Instrumentation Often, astronomers use additional optics between the telescope optics and their detectors. This is called the instrumentation.
Progress Report on the 6dF Galaxy Survey Heath Jones Redshifts and Redshift Completeness Results and Planned Data Releases Observations and Sky Coverage.
AAO Fibre Instrument Data Simulator 10 October 2011 ROE Workshop 2011 Michael Goodwin Tony Farrell Gayandhi De Silva Scott Smedley Australian Astronomical.
This page is intentionally blank. A new view of the Universe VIII Fred Watson (and the RAVErs) April 2005 A new view of the Universe VIII Fred Watson.
SPECTROSCOPIC DIAGNOSTIC COMPLEX FOR STUDYING PULSED TOKAMAK PLASMA Yu. Golubovskii, Yu. Ionikh, A. Mestchanov, V. Milenin, I. Porokhova, N. Timofeev Saint-Petersburg.
2009 Aug 20 — SAC update WFOS/MOBIE1 WFOS/Multi-Object Broadband Imaging Echellette MOBIE Team, to date: PI / optical designer: Rebecca Bernstein Project.
FMOS Overview Oxford, 22nd June FMOS: Fibre Multi-Object Spectrograph Logical successor to 2dF Logical successor to 2dF Wide-Field IR spectroscopy.
Observational Techniques Workshop 19 April 2001 Fred Watson, Anglo-Australian Observatory (with thanks to Karl Glazebrook and Terry Bridges) Observational.
This page is intentionally blank. A new view of the Universe II Fred Watson, AAO April 2005 A new view of the Universe II Fred Watson, AAO April 2005.
High Resolution Echelle Spectrograph for Chinese Weihai 1m Telescope. Leiwang, Yongtian Zhu, Zhongwen Hu Nanjing institute of Astronomical Optics Technology.
Near Infrared Spectro-polarimeter (NIRSP) Conceptual Design Don Mickey Jeff Kuhn Haosheng Lin.
Optical Aeronomy Calibration Facility CEDAR WORKSHOP JUNE, 2007 Jeff Baumgardner, Center for Space Physics Boston University.
Astronomical Spectroscopy Notes from Richard Gray, Appalachian State, and D. J. Schroeder 1974 in “Methods of Experimental Physics, Vol. 12-Part A Optical.
Multiplexed High Res Spectroscopy at Keck – J. Cohen (PI), H. Epps (Optical Design), M. Rich (Project Scientist) Keck instruments for optical spectroscopy.
Science large collection of science cases for seeing improved imaging and spectroscopy also demand on diffraction limited imaging and spectroscopy (Italians)
NIRSpec Operations Concept Michael Regan(STScI), Jeff Valenti (STScI) Wolfram Freduling(ECF), Harald Kuntschner(ECF), Robert Fosbury (ECF)
6dFGS Workshop, Epping 11 July 2003 Fred Watson (and the RAVErs) 6dFGS Workshop, Epping 11 July 2003 Fred Watson (and the RAVErs)
INSTRUMENTATION/ OID / L. Pasquini/ 1 ____________________________________________________________ FLAMES COORDINATION AND INTERFACES. FIELD CORRECTOR.
JGR 19 Apr Basics of Spectroscopy Gordon Robertson (University of Sydney)
Eusoballoon optics test Baptiste Mot, Gilles Roudil, Camille Catalano, Peter von Ballmoos Test configuration Calibration of the light beam Exploration.
NEXT GENERATION OPTICAL SPECTROGRAPH FOR NOAO Samuel Barden, Charles Harmer, Taft Armandroff, Arjun Dey, and Buell Jannuzi (National Optical Astronomy.
The FMOS Facility for the SUBARU telescope Gavin Dalton Oxford/RAL.
The Prime Focus Imaging Spectrograph Design and Capabilities
Objective Our goal is to create a radically inexpensive spectrometer for educational purposes using a Raspberry Pi. The prototype is housed in a black.
Oct 26, 2007SALT Workshop UKZN1 Robert Stobie Prime Focus Imaging Spectrograph Science Rationale Modes –Fabry-Perot Spectral Imaging –Grating Spectroscopy;
6dF workshsopATNF May 30th dF: Observing, data reduction & dataflow Q.A.Parker Macquarie University/AAO.
THE INTEGRATED PHOTONIC SPECTROGRAPH MULTIPLE OFF-AXIS INPUTS AND TELESCOPE RESULTS Nick Cvetojevic 1,2, Nemanja Jovanovic 1,2, Joss Bland-Hawthorn 3,
The 6dF Galaxy Survey - The First Year Will Saunders Anglo-Australian Observatory.
System Performance Metrics and Current Performance Status George Angeli.
Experiments and Design of a wavelength calibration procedure for MOSFIRE Principal Investigator: David Guerrero, Cal Poly SLO Research Advisor: Ian McLean,
The 6dF Galaxy Survey - The Target Samples Will Saunders Anglo-Australian Observatory.
Electron Spectrometer: Status July 14 Simon Jolly, Lawrence Deacon 1 st July 2014.
Performance and sensitivity of Low Resolution Spectrographs for LAMOST Zhu Yongtian, Hou Yonghui, Hu Zhongwen Wang Lei, Wang Jianing.
The Prime Focus Imaging Spectrograph for the Southern African Large Telescope: Operational Modes Chip Kobulnicky – Instrument Scientist, University of.
Sept 16, 2005Ast 920 Meeting 21 Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph Meeting 2 Intro; VPH Grating Spectroscopy Ken Nordsieck.
1 GREAT spectrograph and plugplate discussion Ian Parry Institute of Astronomy Cambridge University UK.
Concepts for a high resolution multi-object spectrograph for galactic archeology on the Anglo-Australian Telescope Samuel C. Bardena, Joss Bland-Hawthornb,
Really Basic Optics Instrument Sample Sample Prep Instrument Out put
Calibration of the Cosmic Origins Spectrograph
An IFU slicer spectrometer for SNAP
Fraunhofer diffraction from Circular apertures:
Presentation transcript:

The 6dF VPH Upgrade and other instrumental issues Will Saunders, Martin Ostreich, Allan Lankshear, Brendan Jones, Mick Kanonczuk, Kristin Fiegert, John Stevenson, Chris McCowage, Bob Dean, Peter Gillingham, Tony Farrell, Keith Shortridge, Brendan Jones, Mick Kanonczuk, Darren Stafford, John Collins, Fred Watson, Malcolm Hartley, Paul Cass, Ken Russell, Dionne James AAO 11/07/03

VPH Upgrade Volume-Phase Holographic gratings offer many advantages for astronomy - Efficient (90% vs 60%) Can specify dispersion and blaze Reduced pupil relief - smaller and slower optics Cheap, robust, large sizes available, multiple suppliers Can tune blaze in use (Prototype for AAOmega) BUT must articulate camera as well as grating

6dFGS Gratings Only 300 resolution elements on CCD - impossible to achieve required wavelength coverage (3900A-7600A) and resolution (~5A) in one hit Hence two gratings, two settings per field Need very rapid grating change =>Pair of gratings at same grating angle on a slide 580V gives 5A fwhm - just good enough for D n -σ. 425R gives 8A fwhm - shorter integration times, and can use twilight.

Results of VPH Upgrade No conflict with AAT use of 316R Much better PSF everywhere More constant PSF, especially across the chip Much more uniform throughput along the slit Not much gain in peak efficiency - gratings only 70% peak efficiency due to loss to zeroth order at such low dispersion Restricted range of other gratings now available: 580V, 425R, 1201B, 1516R, 1700I

Other instrumental issues - Fibre breakages Continues to be a major problem. Several fibres lost, per field plate, per lunation (improving?). Typically running with live fibres. Repairs very slow, difficult and risky. Often running with one field-plate at ~75% efficiency. Additional wear and tear from RAVE survey. All repaired fibres now jacketted with polyimide sleave. Positioning tolerances increased. Robot parking supervised. Other ideas?

Acquisition Guide fibres especially fragile (stripped). No way to repair in original design. Much of first 18 months of survey running with 3 or 2 incomplete (or scrambled!) guide bundles. Very serious effect on S/N and uniformity. Complete redesign and rebuild last year. Breakage rate reduced by sleeving. Now complete set of guide bundles. Guide fibres still oversized at 100μm. Have 75μm available but not high priority.

Camera oil contamination There is oil contamination in 6dF camera, from vacuum pump. Leads to progressive oil contamination of field-flattening lens during each lunation. Complete strip-down very lengthy and risky process. Maybe slow improvement with heat-jacketting?

Robot ‘comm2’ overhaul Complete hardware and software overhaul last year. Full maintenance schedule laid down and implemented. Robot reliability now very good. Configure also much improved (but slower!).