Instrumentation on OIR Large Telescopes – A Case Study S. R. Kulkarni Caltech Optical Observatories.

Slides:



Advertisements
Similar presentations
Flow-down of Strategic Priorities to Annual and 5-year WMKO Plan Taft Armandroff Hilton Lewis September 18, 2009 Taft Armandroff Hilton Lewis September.
Advertisements

Subaru AO in future. Outline Overview of AO systems at Mauna Kea and in the world. Ongoing plan of AOS at Subaru and Mauna Kea. What’s in future.
1 Keck LGS AO Planning Workshop: Overview, Requirements & Schedule December 5, 2004.
RASC, Victoria, 1/08/06 The Future of Adaptive Optics Instrumentation David Andersen HIA.
Laser guide star adaptive optics at the Keck Observatory Adam R. Contos, Peter L. Wizinowich, Scott K. Hartman, David Le Mignant, Christopher R. Neyman,
All these Sky Pixels Are Yours The evolution of telescopes and CCD Arrays: The Coming Data Nightmare.
NGAO Companion Sensitivity Performance Budget (WBS ) Rich Dekany, Ralf Flicker, Mike Liu, Chris Neyman, Bruce Macintosh NGAO meeting #6, 4/25/2007.
All these Sky Pixels Are Yours The evolution of telescopes and CCD Arrays: The Coming Data Nightmare.
LGS AO Operations Transition: Introduction to Meeting April 15, 2005.
1 NGAO Instrumentation Studies Overview By Sean Adkins November 14, 2006.
The SOAR Telescope MSU’s Laboratory for Astronomical Discovery.
NGAO Science Instrument Reuse Part 2: Update and required feedback NGAO IWG Anna Moore, Sean Adkins NGAO Team Meeting January 22, 2007.
Keck Call for Proposals 2009A (Feb 1st - July 31st 2009) Deadline: 5pm, Mon 1st September 2008.
NGAO System Design Phase Management Report - Replan NGAO Meeting #6 Peter Wizinowich April 25, 2007.
Science Operations Plan NGAO - Meeting 10 D. Le Mignant W. M. Keck Observatory 09/17/2007.
NGAO 1-tier Draft Optical Relay Design P. Wizinowich 12/3/07.
Observing efficiency for NGAO 1.Definitions 2.Lessons learned a)Keck LGS AO “efficiency” b)Keck AO brute conclusion 3.Observing efficiency budget 4. Observing.
NGAO Status R. Dekany January 31, Next Generation AO at Keck Nearing completion of 18 months System Design phase –Science requirements and initial.
The Future of AO at Keck Sept 2004 Mike Brown, for the AOWG and Keck AO team.
A Handful of Topics. P200 Constituencies We re-negotiated our partnership agreements in CY2009 Long-standing partners JPL and Cornell are continuing as.
NGAO topical discussion: Observing Efficiency and Uptime Budgets Telecon Meeting 12/7 D. Le Mignant and E. Johansson 7 Dec Attendees; R. Campbell,
California Association for Research in Astronomy W. M. Keck Observatory NGAO Next-Generation Adaptive Optics System NGAO Uptime Budget Keck NGAO Meeting.
High Redshift Galaxies: Encircled energy performance budget and IFU spectroscopy Claire Max Sept 14, 2006 NGAO Team Meeting.
1 NGAO Science Instrument Reuse Part 1: NIRC2 NGAO IWG December 12, 2006.
Trade Study Report: NGAO versus Keck AO Upgrade NGAO Meeting #5 Peter Wizinowich March 7, 2007.
Telescope Errors for NGAO Christopher Neyman & Ralf Flicker W. M. Keck Observatory Keck NGAO Team Meeting #4 January 22, 2007 Hualalai Conference Room,
NGAO Controls Team Kickoff Meeting August 5, 2008 Erik Johansson.
The KPNO 4m “Mayall” Telescope Arjun Dey (NOAO). National Optical Astronomy Observatory Mission: provide the best ground-based astronomical capabilities.
Keck Observatory and The System: Astro2010 Activities Mike Bolte, Shri Kulkarni, Taft Armandroff Keck Strategic Planning Discussions September 18, 2009.
The evolution of ARC/3.5m Current ARC Partner Institutions University of Washington New Mexico State University Princeton University (until June 2014)
W. M. Keck Observatory Subaru Users’ Meeting
Next generation wide field AO (GLAO) and NIRMOS for Subaru Telescope.
U NIVERSITY of C ALIFORNIA O BSERVATORIES LICK · KECK · TMT University of California Observatories Director: Michael Bolte (UCSC) Associate Director: Ian.
A visible-light AO system for the 4.2 m SOAR telescope A. Tokovinin, B. Gregory, H. E. Schwarz, V. Terebizh, S. Thomas.
IXYZ Frank Marshall NASA/GSFC 25 April 2012 April 25, 20121Implementing Portals of the Universe.
Telescopes World Tour 2005, continued…. (1888) Near San Jose, CA James Lick made money in real estate Lick telescope a real pyramid… 36-inch Lick Obs.
Laser Dye Performance A.Jaqueline Mena University of Hawai’i- Hilo W.M. Keck Observatory Mentor: Kenny Grace Advisor: Jason Chin Funding provided through.
IRCS+AO188 decommission? Yosuke Minowa. IRCS AO assisted NIR imager and spectrograph Wavelength coverage: – 1-5 micron (Aladdin III 1024x1024 InSb array)
European small and medium sized telescopes Paul Murdin Particle Physics & Astronomy Research Council.
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)
Early scientific goals for the MMT’s multi-laser-guided adaptive optics Michael Lloyd-Hart, Thomas Stalcup, Christoph Baranec, N. Mark Milton, Matt Rademacher,
is transparent ERAU Astronomical Observatory Meade inch Schmidt Cassegrain Reflecting Telescope.
Scientific Strategic Plan The Process Fall 2008: SSC and Observatory Management began activities to revise the SSP Previous SSP from 2003, last.
5.1 Optical Observatories 5.1 a: Observatory Sites: One limitation: the time needed for optics to reach equilibrium shape when exposed to severe temperatures.
1 R. D. Gehrz 67th International Symposium on Molecular Spectroscopy, Columbus, OH, June 21, 2012 The Stratospheric Observatory for Infrared Astronomy.
Hunting youngest Type Ia SNe in the intermediate Palomar Transient Factory Yi Cao (Caltech) On behalf of the intermediate Palomar Transient Factory collaboration.
From Pan-STARRS to PTF Wing-Huen Ip Institutes of Astronomy and Space Sciences National Central University Nov. 25, 2011 Sun-Moon Lake, Taiwan.
FELT 1 Study of the capability and configuration of a fixed mirror Extremely Large Telescope (FELT) Low cost path to large telescope Primary concern is.
ALTAIR: Access to Large Telescopes for Instruction and Research Chair: Larry Ramsey (14 members, 8.5L, 2S, 3.5U) Report: Submitted Mar 9, 2009
Mega Telescopes of the 21 st Century Evolution in the Ground-Space Synergy Dr. Marc Postman (STScI) & Richard Ellis (Caltech) James Webb Space Telescope.
Some Thoughts on Ground Layer Adaptive Optics & Adaptive Secondary Mirrors for Keck P. Wizinowich 9/15/14 1.
Keck Observatory Overview Peter Wizinowich W. M. Keck Observatory AOSC May 31, 2004.
1 Earth’s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth’s atmosphere can absorb certain.
Followup Observations in the Swift Era S. R. Kulkarni California Institute of Technology.
Tools that help us see Celestial Objects Gr. 9 science exploration unit.
Telescopes Telescopes only have a few jobs: 1)Point to a particular point on the sky 2)Collect lots of light and focus it onto a detector 3)Follow the.
Z Knight W.M. Keck Observatories Research Supervisor: Al Conrad Home Institution: University of Hawai'i at Hilo A Graphical User Interface for NIRC2 Asteroid.
Incoming instruments. New instruments IMACS MOEMultiobject echellette LDSS upgradeMultiobject optical spectroscopy CorMASSLow-res visiting NIR spectrograph.
1 W. M. Keck Observatory Update Randy Campbell Photo Credit: Subaru Telescope 28 May 2005 UT.
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
Big Bear Solar Observatory Some ground-based technology developments that will propel solar physics Phil Goode for Jeff Kuhn Big Bear Solar Observatory.
Future Blanco Instrumentation and how to get it…
Lecture 14 AO System Optimization
Keck Observatory Status
Science Priorities and Implications of Potential Cost Savings Ideas
Laser(s) for Keck Observatory’s Next Generation AO (NGAO) System
NGAO Uptime Budget Keck NGAO Meeting #2 Tuesday, November 14, 2006
NGAO Trade Study GLAO for non-NGAO instruments
Presentation transcript:

Instrumentation on OIR Large Telescopes – A Case Study S. R. Kulkarni Caltech Optical Observatories

Workhorse Instruments – Optical Imagers & Spectrographs – NIR Imagers & Spectrographs and so on Specialized Instruments – Polarimeters, Rapid spectroscopy,.. Adaptive Optics & related instruments “Mega” instruments – Very powerful capabilities (e.g. PFS, GPI, NGAO)

Motivation Cost of workhorse instruments is increasing much faster than inflation The cost of Adaptive Optics facility (let alone instruments) is significant The cost of mega instruments is now approaching that of the telescope itself

Issues: Prioritization & Opportunity Costs Given a fixed budget how to prioritize instrumentation – New instruments versus Upgrades – Which instruments should be built? Mega-instrument – Say cost of a mega instrument is $50M – Per night usage is $50M/N where N=total number of nights – Inversely the opportunity cost of Mega instruments is significant both in money and nights

A CASE STUDY: ANALYZE THE OUTPUT OF THE KECK TELESCOPES

Keck Telescopes Keck I, commissioned in 1993 [$93M] Keck II, commissioned in 1996[$73M] Other than thermal-IR Keck has a complement of instruments from blue to NIR

The Instruments NIRC NIRC2 NIRSPEC OSIRIS MOSFIRE LRIS HIRES ESI DEIMOS KCWI

Keck AO Facility We have LGS AO on both telescopes. NIRC2 is at Keck II OSIRIS at Keck I Continuous upgrades (Center Launch, NIR Tip- tilt, wavefront controller upgrades etc)

Primary data Use the publications which are listed on the WM Keck site – This list is due to Peggi Kamisato and Taft Armandroff.

Top papers by citations

LIGHT CURVES

Some Conclusions It takes about five years for an instrument to peak The usable lifetime of instruments, if not upgraded, is 10 years Optical instruments seem to be more productive and have more impact than NIR (with and without AO) instruments Upgrades increase the productivity of instruments at very low cost

ARE BUILDERS WELL RECOGNIZED?

COST & VALUE OF A NIGHT

CASE STUDY: THE VERY LARGE ARRAY

Should a new all-sky survey be undertaken by the VLA?

NVSS & FIRST FIRST NVSS

Survey returns NVSS and FIRST started off with linear returns for five years and another decade to reach peak fluxes NVSS is returning three times more citations than the typical mix of programs A second sky survey is eminently reasonable and should be undertaken rapidly

DISCUSSION FOR THE AUDIENCE

Mega Instruments & Surveys Mega-instruments are powerful but also expensive. – eg. HSC, PFS, BigBOSS, GPI, SPHERE Once built must be used extensively – Presumably the science returns demand it Age of Surveys – Even PTF can keep Palomar and Keck quite busy – Let alone HSC – Let alone GAIA – Let alone planned radio surveys

Lack of Followup telescopes Mega-instruments remove telescopes from routine use Surveys demand extensive follow up But no new telescopes are being contemplated ……