M2FS: Michigan/Magellan Fiber System. M2FS (Michigan/Magellan Fiber System) Fiber-fed MOS w/2 independent and identical spectrograph arms 256 total fibers.

Slides:



Advertisements
Similar presentations
M2FS SAC UpdateMarch 18, 2012 System Overview: M2FS Spectrograph Two independent, identical channels Each fed by 128 fibers Each with LoRes and HiRes modes.
Advertisements

MMIRS 1 MMIRS MMT and Magellan Infrared Spectrograph Brian McLeod.
1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
1 WHT 2 Degree Field Forward Cass, Prime Focus correctors, multi-object spectrographs David King Institute of Astronomy University of Cambridge Science.
 Cambridge  9 Sep 2012  ASz  The GMT-Consortium Large Earth Finder (G-CLEF): A Versatile, Optical Echelle Spectrograph for the GMT Andrew Szentgyorgyi.
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
PRIME FOCUS CAGE AND CONCEPTUAL DESIGN FOR CAMERA CORRECTOR PRIME FOCUS “BLANCO 2.1dF” SPECIFICATIONS - STRUCTURAL STABILITY - FOCUSING -CALIBRATION -
21/22 September 2002IMACS update1 IMACS: Inamori-Magellan Areal Camera and Spectrograph Magellan SAC Status Report 21/22 September 2002 Boston, MA.
Keck I Cassegrain ADC: Preliminary Design Overview UCO/Lick Observatory 15 October 2003.
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.
An Echidna-style positioner for DESpec
Compare and Contrast SONG and LCOGT Tim Brown Sep 17, 2011 Charleston College/SONG4 FTN, Rob Ratkowski.
The “Cobra” Fiber Positioner, the WFMOS Design, and Potential lessons for DESpec Michael Seiffert, Jet Propulsion Laboratory Richard Ellis, Caltech DESpec.
Lab5 Production Status: Optics and RBX integration Pawel de Barbaro U. of Rochester.
MMT Magellan Infrared Spectrograph ( MMIRS ) P.I. Brian McLeod Warren R. Brown SAO/CfA.
Michigan/MIKE Fiber System (MMFS) – Update Apr 2005.
SIAMOIS, kickoff meeting, Paris, may, SIAMOIS: optical test bench BOSS (Banc Optique SiamoiS) Pernelle Bernardi Observatoire de Paris-Meudon,
The Michigan/Magellan Fiber System (M2FS): An MRI Instrument Development Proposal to NSF.
M agellan I namori K yocera E chelle Rebecca BernsteinU. Michigan Steve ShectmanCarnegie Observatories Steve GunnelsParagon Engineering Stefan MochnackiU.
Corner Raft Test Station Kirk Arndt, Ian Shipsey Purdue University LSST Camera Workshop SLAC Sept , 2008.
18/19 January 2003IMACS SAC meeting update1 IMACS: Inamori-Magellan Areal Camera and Spectrograph Magellan SAC Status Report 18/19 January 2003 OCIW, Pasadena,
Magellan F/5 System Status A.Szentgyorgyi/SAO/30 Apr 2005.
Presentation EddiCam consortium, FF, Madrid 13/06/2002 Eddington programmatic status Fully approved by SPC as part of ESA’s science program as project.
August 2 and 3, 2010 Project Cost, Schedule, Risk and Contingency Jay Elias.
ZTFC 12-segment field flattener (and related) options R. Dekany 07 Aug 2012.
17/18 May 2003IMACS SAC meeting update1 IMACS: Inamori-Magellan Areal Camera and Spectrograph Magellan SAC Status Report 17/18 May 2003 Univ. of Michigan,
Magellan F/5 System Status A.Szentgyorgyi/SAO/25 Sept 2004.
Spectroscopic Observations (Massey & Hanson 2011, arXiv v2.pdf) Examples of Spectrographs Spectroscopy with CCDs Data Reduction and Calibration.
High Resolution Echelle Spectrograph for Chinese Weihai 1m Telescope. Leiwang, Yongtian Zhu, Zhongwen Hu Nanjing institute of Astronomical Optics Technology.
Telescope Integration and Tests Tuesday Afternoon.
Upgrade plan of the MOA 1.8-m telescope F. Abe MOA collaboration 19 Jan. 2009, 13th Microlensing Paris.
INSTRUMENTATION/ OID / L. Pasquini/ 1 ____________________________________________________________ FLAMES COORDINATION AND INTERFACES. FIELD CORRECTOR.
Magellan F/5 System Status A.Szentgyorgyi / Ann Arbor 25 Sept 2005.
6-7 October 2001Inamori-Magellan Areal Camera & Spectrograph 1 IMACS: Inamori-Magellan Areal Camera and Spectrograph Magellan SAC Status Report 6-7 October.
The Study of IFU for the Li Jiang 2.4m Telescope ZHANG Jujia 张居甲 Yun Nan Astronomical Observatory. CAS Sino-French IFU Workshop Nov Li Jiang.
Opto-Mechanics for SNAP at UM
The Prime Focus Imaging Spectrograph Design and Capabilities
13-14 April 2002Inamori-Magellan Areal Camera & Spectrograph 1 IMACS: Inamori-Magellan Areal Camera and Spectrograph Magellan SAC Status Report April.
1 Space Telescope Science Institute JWST S&OC JWST S&OC Contract Peter Stockman TIPS March 20, 2003.
Keck Observatory in the TMT Era Keck Strategic Planning meeting September 18, 2009.
Magellan Telescopes Instrumentation: A Critical Assessment of Current Status.
Oct 17, 2001SALT PFIS Preliminary Design Review1 Southern African Large Telescope Prime Focus Imaging Spectrograph Mechanical Mechanism Design Michael.
Binospec - Next Generation Optical Spectrograph for the MMT
Oct 24, 2006SSWG1 Robert Stobie Prime Focus Imaging Spectrograph Status On-telescope throughput analysis Ghost analysis Repair plan Status of other current.
DBSP-R Upgrade Progress Review The DBSP-R Team DBSP-R Progress Review.
9/24/05MagE Update SAC meeting Developments with MagE Complete layout of Spectrograph structure and camera by B. Bigelow –Structure will be all anodized.
The 6dF Galaxy Survey - The First Year Will Saunders Anglo-Australian Observatory.
Science with Giant Telescopes - Jun 15-18, Instrument Concepts InstrumentFunction range (microns) ResolutionFOV GMACSOptical Multi-Object Spectrometer.
Wide field telescope using spherical mirrors Jim Burge and Roger Angel University of Arizona Tucson, AZ Jim
Page 1HMI/AIA Science Meeting – February 13, 2006 HMI Instrument Status HM/AIA Science Meeting February 13, 2006 Barbara Fischer HMI Deputy Program Manager.
Apr 29, 2003SSWG1 Prime Focus Imaging Spectrograph Status Passed CDR- moving into fabrication phase Mechanism design complete: fabrication drawing packages.
Astronomical Observational Techniques and Instrumentation
Magellan Telescopes Observatory Report Personnel Accomplishments Observing Statistics Common Problems Work in Progress.
MMIRS Status A.Szentgyorgyi/SAO 30 April Imaging 7 x 7 arcmin FOV 0.2 arcsec pixels Y,J,H & K wavelength coverage Spectroscopy Multislit (4’ x 7’)
1 Harvard-Smithsonian Center for Astrophysics Magellan SAC 9/04 MMIRS Status Report Brian McLeod.
GMT’s Near IR Multiple Object Spectrograph - NIRMOS Daniel Fabricant Center for Astrophysics.
Status of LAMOST ZHAO Yongheng National Astronomical Observatories of China.
MMIRS 1 Harvard-Smithsonian Center for Astrophysics Magellan SAC 9/05 MMIRS Status Upate Presented by A. Szentgyorgyi P.I. B. McLeod.
F/5 telescope work Secondary mirror polishing (SOML) Secondary mount support controls Active optics controls Flat field screen & lamps Telescope baffles.
NIRSpec - the JWST Multi-Object Spectrograph P. Ferruit (ESA), S. Arribas (CSIS), S. Birkmann (ESA), T. Böker (ESA), A. Bunker (Oxford), S. Charlot (IAP),
MagIC Upgrade for High-Speed Photometry Jim Elliot, MIT Magellan SAC
CASE spectrograph Spectrograph Optical Specifications
ComCam Hardware and Interfaces James Howard ComCam CAM LSST 2017 Project & Community Workshop 2017 Aug 15.
Prime Focus Imaging Spectrograph Status
Agenda ComCam planning and scheduling (James & Jacques) CCS & CCS-TCS Interface (Tony) Software to use ComCam Software to get data out of ComCam (Mike)
Telescope Assembly, Integration and Verification (AIV) WBS 04C. 14 J
ComCam Hardware and Interfaces James Howard ComCam CAM LSST 2017 Project & Community Workshop 2017 Aug 15.
Prime Focus Imaging Spectrograph Status
Optics Alan Title, HMI-LMSAL Lead,
Presentation transcript:

M2FS: Michigan/Magellan Fiber System

M2FS (Michigan/Magellan Fiber System) Fiber-fed MOS w/2 independent and identical spectrograph arms 256 total fibers + manual plug plates 128 Fibers per Arm HiRes (R=18-34k) and LoRes (R~ ) Modes (can be used independently on separate arms) Single and multi-order spectroscopy supported in HiRes Mode 30 arcmin diameter FoV (fully accessible to all fibers) Aperture size = 1.2 arcsec (diam) Minimum fiber spacing = 12 arcsec (center-center) Any fiber can be deployed to any position in field Target position lead-time is about 4-6 weeks to fabricate plates. 1 km/s precision anticipated at V=21-22 for late-type stars. LoRes targets to V=24-25 within aperture. Target M2FS delivery date to Magellan: Apr-Jun 2012 Science operations aimed to start in 2012B semester Prototype robotic positioner planned and full automated plugging may be possible by 2014 pending funding.

Project Status: Fibers Fiber construction is proceeding full-time at UM. 418 Fibers have completed first construction stage (10 ft tubing with end hypos, apppropriately epoxied) Polishing underway; eight-fiber polisher built for this purpose. Initial interferometric tests => flat to <1/4 wave. All fiber ends to be AR coated (first test run went well); tested interferometrically (thanks Gabor Furesz); tested for FRD performance. Goal: 256 prime science fibers + >64 science spares + 20 acquisition fibers. Tetris ends under design and trying to find vendors. Finding vendors for ferrules is proving hard. Modulo ferrules: Construction/Testing by end of June; all fiber parts by end of September.

Project Status: Prime Optics Optical Design Review passed July Echelle gratings in hand. All M2FS major transmissive spectrograph optics ordered through AR coating. CaF2 blanks shipped to opticians (OSI for asphere and HJOL) Assuming no breakage, all prime optical elements in hand by Oct/Nov. Triplet construction in Jan/Feb Wide-Field Corrector optics pending order with formal appro- val from NSF. M2FS telecentrator from MMFS. DECOMISSIONS MMFS. Mechanical design to be completed by Sep Lenses to be completed by Nov/Dec. Construction/Mouting of all optics by end of Mar/Apr 2012.

M2FS Wide-Field Corrector

Project Status: Mechanical Fiber mount largely a copy of MMFS, even to use some parts. Mechanical design of major spectrograph components underway: o Grating exchange stage and grating mounts. o Prime optics mounts (largely derivative from PFS). o CCD dewar mount bulkhead which also supports the filter exchanger, fiber-locator system, shutter, fiber cradle. o Design of fiber shoe and fiber end mounts underway. Conceptual design for calibration unit/FLS projector in the secondary cage in place. To work closely with LCO on design and testing/deployment. Construction and testing at OCIW. Design Review in August. Fabrication of principal compo- nents from Aug 2011-Feb 2012 at OCIW and UM shops.

Echelle Grating Fiber Injection Cam/Coll Optics LoRes Grating CCDs Spectrograph 1 Spectrograph 2 Magellan Elevation Ring

Project Status: Electronic E2V CCDs to arrive in May 2011; IT will install in dewars at OCIW. Design/performance goals just now beginning in earnest. Surprising number of controls: o Grating tilts, azimuth (echelle only) x 2 o Grating stage translation x 2 o Filter position, vertical and insertion x 2 o Fiber locator system mirror insertion x 2 o Shutter x 2 o Spectrograph focus (derivative from PFS) x 2 o Fiber slit assemblies x 16 o CCD control x 2 o Guider focus, SH periscope optics, SH camera o Guide camera o Calibration lamps, FLS projector Initial controls meeting on Apr 29 (Friday) to identify issues, people, software demands and basis for a realistic schedule.

Project Status: Performance