Astronomical Instrumentation at Texas A&M Jennifer Marshall Darren DePoy.

Slides:



Advertisements
Similar presentations
White Dwarfs in the HET Dark Energy Experiment Bárbara G. Castanheira The University of Texas at Austin Universität Wien 17 th European White Dwarf Workshop.
Advertisements

1 Astronomical Observational Techniques and Instrumentation RIT Course Number Professor Don Figer Telescopes.
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
DESpec spectrographs Jennifer Marshall Darren DePoy Texas A&M University.
Calibration for LHAASO_WFCTA Yong Zhang, LL Ma on behalf of the LHAASO collaboration 32 nd International Cosmic Ray Conference, Beijing 2011.
Spectroscopic Reference Design Options D. L. DePoy Texas A&M University.
 Michael J. Sholl 1, Mark R. Ackerman 2, Chris Bebek 3, Robert Besuner 1, Arjun Dey 4, Jerry Edelstein 1, Patrick Jelinsky 1, Michael L. Lampton 1, Michael.
All these Sky Pixels Are Yours The evolution of telescopes and CCD Arrays: The Coming Data Nightmare.
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
All these Sky Pixels Are Yours The evolution of telescopes and CCD Arrays: The Coming Data Nightmare.
Astronomical Research at TAMU Faculty Future facilities and projects.
The SOAR Telescope MSU’s Laboratory for Astronomical Discovery.
HETDEX Spectrographs R&D for DESpec Jennifer Marshall Texas A&M University.
KDUST Supernova Cosmology
Telescopes and Astronomical Observations Ay16 Lecture 5 Feb 14, 2008.
Astronomical Spectroscopy
The Photometric Calibration of the Dark Energy Survey D. L. Tucker 1, S. S. Allam 1, J. T. Annis 1, R. Armstrong 2, J. P. Bernstein 3, E. Bertin 4, D.
X-ray Optical microwave Cosmology at KIPAC. The Survey 5000 square degrees (overlap with SPT and VISTA) Five-band (grizY) + VISTA (JHK) photometry to.
The KPNO 4m “Mayall” Telescope Arjun Dey (NOAO). National Optical Astronomy Observatory Mission: provide the best ground-based astronomical capabilities.
1 Korean Activities in IR Space Missions - Past, Current and Future - Woong-Seob Jeong 1 on behalf of Korean Infrared Astronomy Group 1 KASI, Korea Ramada.
Chapter 6: The Tools of the Astronomer. Telescopes come in two general types Refractors use lenses to bend the light to a focus Reflectors use mirrors.
AAO Fibre Instrument Data Simulator 10 October 2011 ROE Workshop 2011 Michael Goodwin Tony Farrell Gayandhi De Silva Scott Smedley Australian Astronomical.
Further Advancements of the PARI Optical Ridge Telescopes for Education and Public Outreach M. W. Castelaz, J. D. Cline Pisgah Astronomical Research Institute.
Sternberg Astronomical Institute of Lomonosov Moscow State University.
Calibration Plan for Early DES Data
Spectrophotometer Prof.Dr. Moustafa M. Mohamed Vice Dean Faculty of Allied Medical Science Pharos University in Alexandria, EGYPT.
High Resolution Echelle Spectrograph for Chinese Weihai 1m Telescope. Leiwang, Yongtian Zhu, Zhongwen Hu Nanjing institute of Astronomical Optics Technology.
15 October Observational Astronomy Direct imaging Photometry Kitchin pp ,
THE DARK ENERGY SURVEY Science Goals: Perform a 5000 sq. deg. survey of the southern galactic cap Map the cosmological density field to z=1 Constrain the.
Dark Energy Probes with DES (focus on cosmology) Seokcheon Lee (KIAS) Feb Section : Survey Science III.
Dark Energy and Large Synoptic Survey Telescope Precision Calibration Apparatus: Calibrating the Throughput and Response of Astronomical Instrumentation.
John Peoples for the DES Collaboration BIRP Review August 12, 2004 Tucson1 DES Management  Survey Organization  Survey Deliverables  Proposed funding.
is transparent ERAU Astronomical Observatory Meade inch Schmidt Cassegrain Reflecting Telescope.
DECam Daily Flatfield Calibration DECam calibration workshop, TAMU April 20 th, 2009 Jean-Philippe Rheault, Texas A&M University.
Office of Science U.S. Department of Energy DETF Recommendations I 2.1Science (Charge questions 1, 2, 7) Andy Albrecht & Nicholas Suntzeff 2.1.2Comments.
The Photometric Calibration of the Dark Energy Survey D. L. Tucker 1, S. S. Allam 1, J. T. Annis 1, R. Armstrong 2, J. P. Bernstein 3, E. Bertin 4, D.
Australia’s Path to a Giant Telescope Matthew Colless MNRF Symposium 7 June 2003.
Calibration of the LSST Camera Andy Scacco. LSST Basics Ground based 8.4m triple mirror design Mountaintop in N. Chile Wide 3.5 degree field survey telescope.
Image Processing: Critical to Hubble Discoveries
1 Followup to Filters & Calibration Strategy Workshop: Calibration Douglas L. Tucker DES Calibration Workshop 13 June 2008.
1 The DES Calibrations Effort Douglas L. Tucker (DES Calibrations Scientist) DES NSF/DOE Review, 8-9 June 2009 The DES Calibrations Effort has connections.
The Large Synoptic Survey Telescope: The power of wide-field imaging Michael Strauss, Princeton University.
The View from NSF Very Wide Field Surveys in the Light of Astro2010 Space Telescope Science Institute June Nigel Sharp 1.
1 Calibration Screen Development Claire Cramer Brian Stalder Gautham Narayan Christopher Stubbs Department of Physics Harvard University Claire Cramer.
1 DECam in Chile Intro to Dark Energy Survey & DECam Project Status of arrivals in Chile Instrument checkout in Chile Schedule for first light.
Science with Giant Telescopes - Jun 15-18, Instrument Concepts InstrumentFunction range (microns) ResolutionFOV GMACSOptical Multi-Object Spectrometer.
Goals for HETDEX Determine equation of state of Universe and evolutionary history for dark energy from 0
Mountaintop Software for the Dark Energy Camera Jon Thaler 1, T. Abbott 2, I. Karliner 1, T. Qian 1, K. Honscheid 3, W. Merritt 4, L. Buckley-Geer 4 1.
LSST Photometric Calibration D. Burke SLAC/KIPAC DOE SLAC Program Review June 6-7, 2006.
Douglas Tucker (FNAL)Joint DOE/NSF Review, January Global Photometric Calibrations Douglas L. Tucker (FNAL) Joint DOE/NSF Review of DES
ISWG - December 7, Destiny, The Dark Energy Space Telescope.
Michael Allen. MooSci  MooSci is a device that uses scintillation measurements from the Moon to reconstruct the ground layer turbulence profile.  This.
1 Astronomical Observational Techniques and Instrumentation Professor Don Figer Telescopes.
DESpec in the landscape of large spectrographic surveys Craig Hogan University of Chicago and Fermilab.
NIRSpec - the JWST Multi-Object Spectrograph P. Ferruit (ESA), S. Arribas (CSIS), S. Birkmann (ESA), T. Böker (ESA), A. Bunker (Oxford), S. Charlot (IAP),
Hobby-Eberly Telescope Dark Energy Experiment The upgraded HET.
Li, Ting Texas A&M University DePoy, Darren Texas A&M University Burke, David SLAC Kessler, Richard University of Chicago Marshall, Jennifer Texas A&M.
Cosmic Program and Users in the Fermilab Dark Energy program Brenna Flaugher Fermilab Institutional Review Feb
DECam Spectrophotometric Calibration DECam calibration workshop, TAMU April 20 th, 2009 Jean-Philippe Rheault, Texas A&M University.
The GMT Project The Giant Magellan Telescope (GMT)
The EUSO-SPB mission Valentina Scotti INFN Sezione di Napoli.
The upgraded HET Hobby-Eberly Telescope Dark Energy Experiment.
Calibration Status for the GOME Instrument
Harvard graduate student Arti Garg hunting dark matter (microlensing candidates) with the Magellan telescope (Above) The PanSTARRS telescope atop the volcano.
Detectors of the New Projects at NAOC
LSST Photometric Calibration
Astronomical Observational Techniques and Instrumentation
Makmal Fizik Angkasa Research Activities and Projects in Space Physics Lab Prof. Dr. Mohd. Zambri Zainuddin Makmal Fizik Angkasa Jabatan Fizik.
Observational Astronomy
Sci. 1-3 Telescopes- then and Now Pages 18-23
Presentation transcript:

Astronomical Instrumentation at Texas A&M Jennifer Marshall Darren DePoy

TAMU Instrumentation The Department of Physics and Astronomy at Texas A&M University has built a new astronomical instrumentation lab –Three years old –Led by Darren DePoy Mission: to design and build astronomical instrumentation to support Dark Energy and Cosmology observations Partner in DES, LSST, HETDEX/HET, GMT

DECam for DES Dark Energy Survey –Led by Fermilab –DECam: Large new camera for CTIO 4m telescope DePoy is Project Scientist for DECam TAMU is involved in calibration efforts for DECam –DECal –aTmCam

Projection optics Screen Fiber bundle Spectro meter Light source Mono chromator Photodiode DECal for DES Calibration system for DECam: Flat field screen Daily flat field system –LED flat field lamps Spectrophotometric calibration system –Long fiber bundle –Monochromator (with spectrometer monitor) –Monitor photodiodes

aTmCam for DES aTmCam is an atmospheric monitoring camera Goal: produce <1% photometry by monitoring sky during DES observations pressureozonewater aerosol ‘cannon’ mask with wedge prism and narrowband filters

VIRUS for HETDEX VIRUS is a new instrument for HET to support HETDEX survey –150+ channel fiber-fed spectrograph –>33, ” fibers – nm coverage at R~700

GMACS for GMT Texas A&M is a founding partner in the Giant Magellan Telescope Recently completed a one-year design study of GMACS –Wide field multi-object optical spectrograph

MooSci for GMT We have built a lunar scintillometer called MooSci for GMT site testing Used to test site before and after top of mountain is removed

Antarctic instrumentation We are interested in collaborating in projects for Antarctica/Dome A –We have begun discussions with Teledyne regarding purchasing detectors for KDUST –We could also help with camera design/testing