ESAC_3_24_05.ppt Gamma-ray Large Area Space Telescope – exploring the high-energy universe.

Slides:



Advertisements
Similar presentations
Gamma-ray Mapping of the Interstellar Medium and Cosmic Rays in the Galactic Plane with GLAST Yasushi Fukazawa 1, T. Kamae 1,2, T. Ohsugi 1, T. Mizuno.
Advertisements

Blazar Science Group report, August 31, 2005 Gamma-ray Large Area Space Telescope Coordinators: P. Giommi & B. Lott Report on the “Blazar and Other AGN”
EGRET unidentified sources and gamma-ray pulsars I. CGRO mission and the instrument EGRET and it’s scientific goals II. Simple introduction of EGRET sources.
Science Drivers for the Next Generation VHE Telescope(s?) G. Sinnis with much help from C. Dermer, J. Buckley, H. Krawczynski, S. LeBohec, R. Ong, M. Pohl,
Gamma-ray Astronomy Missions, and their Use of a Global Telescope Network.
SLAC, 7 October Multifrequency Strategies for the Identification of Gamma-Ray Sources Marcus Ziegler Santa Cruz Institute for Particle Physics Gamma-ray.
GLAST Large Area Telescope - OperationsDOE Review, 15 June GLAST Large Area Telescope Operations Review Rob Cameron Instrument Science Operations.
GLAST LAT Project – Collaboration MeetingAugust, 2005 Science Group Reports 1 GLAST Large Area Telescope: Collaboration Meeting August 26, 2005 Pulsar,
GLAST LAT ProjectGraduate Student Orientation, Sep 22, 2005 E. do Couto e Silva 1 Gamma ray Large Area Space Telescope (GLAST) Eduardo do Couto e Silva.
Gamma-ray Large Area Space Telescope IEEE Nuclear Science Symposium Wyndham El Conquistador Resort, Puerto Rico October , 2005 The Gamma Ray Large.
Gamma-ray Astronomy (The Short Story…). The Big Picture l Whole sky glows l Extreme environments l Probes of the Universe CGRO/EGRET All Sky Map.
GLAST LAT Project 1S. Ritz Discussion: To Where From Here? DC1 Closeout Meeting February 13, 2004 S. Ritz Gamma-ray Large Area Space Telescope.
GLAST LAT Project July 19, 2005 E. do Couto e Silva 1/17 Science Verification Analysis and Calibration GLAST Large Area Telescope Eduardo do Couto e Silva.
GLAST LAT Project DOE Mini-review 12 October 2004 S. Ritz 1 IntroductionS. Ritz Technical and Production StatusL. Klaisner Instrument Science Operations.
Julie McEnery1 GLAST: Multiwavelength Science with a New Mission Julie Mc Enery Gamma-ray Large Area Space Telescope.
SLAC, 7 October Multifrequency Strategies for the Identification of Gamma-Ray Sources Marcus Ziegler Santa Cruz Institute for Particle Physics Gamma-ray.
Eduardo do Couto e Silva - ATC/LM Colloquium, June How many neutralinos are there? Expansion of universe Depletion of neutralinos Creation of neutralinos.
1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting.
GLAST LAT Project ISOC Peer Review - March 2, 2004 Section Gamma-ray Large Area Space Telescope GLAST Large Area Telescope ISOC Peer Review 7.2.
GLAST Large Area Telescope - OperationsDOE Review, 15 June GLAST Large Area Telescope Operations Review Rob Cameron Instrument Science Operations.
SLAC DoE Review June 14-16, 2005 GLAST Large Area Telescope Overview Elliott Bloom SLAC - KIPAC Stanford University.
Exploring the High Energy Universe where Particle Physics and Astrophysics Collide Prof. Lynn Cominsky Sonoma State University GLAST Education and Public.
JD1 rationale Catherine Cesarsky, Diego Torres, Stefan Wagner.
ESAC_3_24_05.ppt 1 GLAST: Large Area Telescope - LAT Status and Schedule - Multiwavelength Needs: Discussion with AAAC in October Peter F. Michelson Stanford.
ICHEP 04 - August 16-22, 2004, Beijing Monica Pepe – INFN Perugia 1 Gamma-ray Large Area Space Telescope High Energy Gamma Physics with GLAST Monica Pepe.
Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach.
1 Arecibo Synergy with GLAST (and other gamma-ray telescopes) Frontiers of Astronomy with the World’s Largest Radio Telescope 12 September 2007 Dave Thompson.
The role of GLAST in multiwavelength observations of bright TeV blazars D. Paneque J.Chiang, B. Giebels, V. Lonjou, B.Lott,
Outline: Introduction into the problem Status of the identifications Summary Identification of Very high energy gamma-ray sources.
Igor V. Moskalenko Stanford University on behalf of the Fermi LAT Collaboration and the Fermi mission RESULTS FROM THE FIRST MONTHS OF THE FERMI GAMMA-RAY.
Imaging Compact Supermassive Binary Black Holes with VLBI G. B. Taylor (UNM), C. Rodriguez (UNM), R. T. Zavala (USNO) A. B. Peck (CfA), L. K. Pollack (UCSC),
GLAST Science and Opportunities Seattle AAS Meeting, January 2007 Enhancing GLAST Science Through Complementary Radio Observations Jim Ulvestad Paper
Introduction to gamma-ray astronomy GLAST-Large Area Telescope Introduction to GLAST Science New way of studying astrophysics Schedule of GLAST project.
Julie McEnery1 Data Challenge II Logo by Stefano Ciprini.
GLAST LAT ProjectCDR/CD-3 Review May 12-16, 2003 Document: LAT-PR-01967Section 1 Introduction & Science Overview 1 GLAST Large Area Telescope: Introduction.
ESAC_3_24_05.ppt 1 GLAST Development Status, Science Opportunities and Multiwavelength Needs, Interagency Coordination Peter F. Michelson Stanford University.
1 GLAST Gamma-ray Large Area Space Telescope P. Michelson GLAST LAT Spokesperson Stanford University for the GLAST LAT Collaboration.
National Aeronautics and Space Administration November 23, Gamma-ray Large Area Space Telescope (GLAST) Kevin Grady, Project Manager Steven Ritz,
Blazars: VLBA and GLAST Glenn Piner Whittier College.
A Catalog of Candidate High-redshift Blazars for GLAST
GLAST LAT Project DOE/NASA Review, March 31, GLAST Large Area Telescope: Lowell A. Klaisner Stanford Linear Accelerator Center Project Manager
1 S. Ritz Data Policies & GO Program Status GUC August 2004.
Julie McEnery1 Data Challenge II. Julie McEnery2 Seth Digel, Diego Torres & Olaf Reimer on high-latitude molecular clouds, SNRs, XRBs, OB associations,
1 Stepping in everyone’s toes ( but for a good cause….) Eduardo do Couto e Silva Software Meeting – January 2001.
First GLAST Symposium Planning 1 GLAST The Gamma-ray Large Area Space Telescope First GLAST Symposium Planning Users Committee Meeting 7 May 2006 P.F.
Pulsars: The radio/gamma-ray Connection Prospects for pulsar studies with AGILE and GLAST Synergy with radio telescopes –Timing and follow-up –Radio vs.
ESAC_3_24_05.ppt 1 GLAST Large Area Telescope Overview and Science Update Peter F. Michelson Stanford University GLAST User’s Committee.
Launch The Gamma-ray Large Area Space Telescope (GLAST) S. Ritz (GSFC, Project Scientist), J. Grindlay (Harvard, Users Committee Chair), C. Meegan (MSFC,
Peter F. Michelson LAT Principal Investigator Fermi User Group Meeting August 28, 2009.
GLAST LAT SpacePart06 April BejingClaudia Cecchi Gamma-ray Large Area Space Telescope High Energy Gamma Rays Physics with GLAST Claudia Cecchi.
GLAST Mission: Status and Science Opportunities Peter F. Michelson Stanford University Gamma-ray Large Area Space Telescope.
1 Fermi Gamma-ray Space Telescope Users Group Meeting 6 February 2009 Mission Status Update (since the phonecall) and Issues S. Ritz, J. McEnery.
Peter F. Michelson Stanford University Principal Investigator, Large Area Telescope Collaboration on behalf of the Fermi LAT Collaboration.
GLAST Large Area Telescope – ISOC Overview and StatusDOE Annual Review, 13 June GLAST Large Area Telescope Instrument Science Operations Center.
GLAST LAT Project DC2 Software Workshop, GSFC, June 27-29, Analytical Objectives for Science Tools for DC2 for DC2 S. W. Digel Stanford Linear Accelerator.
1 Fermi Gamma-ray Space Telescope Large Area Telescope Multiwavelength Notes (mostly LAT) Dave Thompson Fermi LAT Multiwavelength Coordinator.
Fermi Gamma-ray Space Telescope Searches for Dark Matter Signals Workshop for Science Writers Introduction S. Ritz UCSC Physics Dept. and SCIPP On behalf.
Population Studies of the Unidentified EGRET Sources In collaboration with A. V. Olinto, V. Pavlidou, C. Brown, and B. D. Fields Image Credit: EGRET Team/NASA/Honeywell.
Monitoring GLAST Operations: Building tracking displays for the LAT Instrument Science Operations Center By Christina Ketchum.
Gamma-ray Large Area Space Telescope: Physics Goals and Instrument Status Jennifer Carson SLAC/KIPAC for the GLAST LAT collaboration GLAST lifetime: 5+5.
07/12/061 Modeling a Black Hole Fill in your information here. Fill in your information here.
GLAST Large Area Telescope:
A Search for Blazars among the Unidentified EGRET Gamma-Ray Sources.
Reports from Science Groups
GLAST : Exploring the High Energy Universe where Particle Physics and Astrophysics Collide Prof. Lynn Cominsky Sonoma State University GLAST Education.
Proposal for LAT Year 1 Data Release Plan
GLAST Dark Matter & New Physics Working Group
Data Challenge 2: Aims and Status
March ’05 Face to Face Meeting Introduction
GLAST Large Area Telescope Instrument Science Operations Center
Presentation transcript:

ESAC_3_24_05.ppt Gamma-ray Large Area Space Telescope – exploring the high-energy universe

2 Gamma-ray Large Area Space Telescope ► flight hardware now arriving at SLAC for instrument integration  4 flight towers installed ► Schedule:  instrument assembly complete: December 2005  instrument environmental tests complete: May 2006  LAT delivery to Spectrum-Astro (General Dynamics) for integration with spacecraft: May 2006  GLAST Launch: August 31, 2007

3 LAT Schedule

4 Critical path to ship LAT to Spectrum Astro

5 Flight Hardware Integration Flight Tracker in Cleanroom at SLAC Flight Calorimeter Preparation of flight grid for TCS integration LAT Integration stand with PAP ready for proof test

6 First Flight Tower in I&T

7 First Integrated Tower – Muon Candidate Event Calorimeter crystals Tracker planes XZ projection YZ projection

8 Gamma-ray Candidate Event

9 Two Towers in Grid

10 First 2-tower events

11 First 2-tower events

12 Interest in GLAST Mission is growing ► At all mission levels, including Conferences, Workshops. ► Multiwavelength survey initiatives underway ─VLA monitoring for a large sample of flat-spectrum, compact sources ─VLBA Imaging and Polarimetry Survey proposed to obtain a set of reference images for 1000 potential LAT sources in advance of GLAST launch ─Northern and Southern hemisphere radio pulsar timing campaigns in support of GLAST mission ─optical and radio monitoring of LAT AGN ► Broad and growing interest COS-B EGRET GLAST ??? Publications & Conference Proceedings pre-launch total

13 Science Groups of LAT Collaboration  groups responsible for analysis and writing papers GroupPrincipal Responsibilities 1. Catalogs Prepare comprehensive LAT catalog for publication, after 1, 2, and 5 years (nominal), including cross-identifications when known. 2. Diffuse (Galactic & Extragalactic) and Molecular Clouds Generate Galactic diffuse model for delivery to community (GSSC) and provide periodic updates; study mass tracers and CR density in individual clouds; Analysis of the residual isotropic gamma-ray emission (after accounting for LAT sources and Galactic diffuse) including its spectra and angular fluctuations; assess contributions from various source classes 3. Blazars & Other AGNs Analysis of spectra and time variability of LAT-detected blazars and other types of AGNs; modeling of spectra (e.g. SSC model) including effects of EBL; study evolution with redshift 4. Pulsars, SNRs & Plerions Construct phase-resolved “light curves” and spectra for LAT-detected radio pulsars; search for periodic emission in other sources, including unidentified sources; identify SNRs and plerions and model spectra of these sources 5. Unidentified Sources, Population Studies, & Other Galaxies Coordinate deep multi-wavelength studies of the error boxes of the unidentified GLAST sources and correlate with potential counterpart populations; determine the heterogeneity of the population and correlate with source characteristics \(e.g. time variability; spectral index, etc.) Search for emission from other galaxies, particularly nearby galaxies such as M31, ULRGs, and from clusters of galaxies; determine source spectra and/or set upper limits 6. Dark Matter and Exotic Physics Search for signatures of dark matter, extra dimensions (e.g. KK graviton decay), quantum gravity dispersion effects, etc. 7. Gamma-Ray Bursts Construct LAT GRB catalogs; determine burst spectra, including time evolution; coordinate joint analysis of bursts with GBM 8. Sources in the Solar System Solar flares; lunar emission; … 9. Calibration and Analysis Methods Pre-flight performance of the LAT and on-orbit calibration and performance (1) Monte Carlo model of LAT; event reconstruction and background rejection methods; (2) astrophysical data analysis methods (e.g. likelihood analysis; time series analysis; source spectral analysis, cross-correlation methods, etc.)

P. F. Michelson GLAST LAT SSAC Meeting: March 15, Science Group Coordinators GroupCoordinators 1. CatalogsSeth Digel (SU-SLAC); Isabelle Grenier (CEA/Saclay) 2. Diffuse (Galactic & Extragalactic) and Molecular Clouds Seth Digel (SU-SLAC); Isabelle Grenier (CEA/Saclay) 3. Blazars & Other AGNsPaolo Giommi (ASDC); Benoit Lott (IN2P3–Bordeaux) 4. Pulsars, SNRs & PlerionsRoger Romani (Stanford); David Thompson (GSFC) 5. Unidentified Sources, Population Studies, & Other Galaxies Patrizia Caraveo (IFC, CNR); Olaf Reimer (Stanford) 6. Dark Matter and Exotic PhysicsElliott Bloom (SU-SLAC); Aldo Morselli (INFN–Rome) 7. Gamma-Ray BurstsJay Norris (GSFC); Nicola Omodei (INFN-Pisa); N. Kawai (start 07; sabbatical at SU 08-09) 8. Sources in the Solar SystemGerry Share (NRL) 9. Calibration and Analysis MethodsWilliam Atwood (UCSC); Steve Ritz (GSFC) Eduardo do Couto e Silva (SU-SLAC, start ~07) ► science coordinator telecons: ~ every two weeks