Madison, May 20, 2009 Tom Gaisser1 IceCube Collaboration Overview & Response to 2008 SAC Report.

Slides:



Advertisements
Similar presentations
The IceCube Neutrino Telescope Kyler Kuehn Center for Cosmology and AstroParticle Physics The Ohio State University Novel Searches for Dark Matter CCAPP.
Advertisements

IceCube.
Search for Extremely-high Energy Cosmic Neutrino with IceCube Chiba Univ. Mio Ono.
The IceCube High Energy Telesope The detector elements Expected Sensitivity Project Status Shigeru Yoshida Dept. of Physics CHIBA Univ. ICRC 2003.
Neutrino Astronomy at the South Pole David Boersma UW Madison “New Views of the Universe” Chicago, 10 December 2005.
LSU 07/07/2004Communication1 Communication & Documentation Project Management Unit – Lecture 8.
AIDA is co-funded by the European Commission within the Framework Programme 7 Capacities Specific Programme, Grant Agreement AIDA status report.
IceCube a kilometer-scale deep-ice observatory in Antarctica Olga Botner Uppsala university, Sweden Neutrino 2004, June 14-19, icecube.wisc.edu.
1. Introduction 2. IceCube Detector 3. Neutrino Detection Principles 4. Status of the Construction and Performance 5. Summary IceCube neutrino
Per Olof Hulth Stockholm university1 NSF Review March 25-27, 2003 Introductory remarks Per Olof Hulth Stockholm university.
A km 3 Neutrino Telescope: IceCube at the South Pole Howard Matis - LBNL for the IceCube Collaboration.
Alexander Kappes LTP/PSI Colloquium Paul Scherrer Institut, 30. Sept Neutrinos on the rocks – Astronomy at the South Pole with IceCube.
IceCube S Robbins University of Wuppertal Moriond - “Contents and Structures of the Universe” La Thuile, Italy, March 2006 Outlook for Neutrino Detection.
Astronomy & Astrophysics Advisory Committee (AAAC) May 11, 2006 Vladimir Papitashvili Antarctic Sciences Section Office of Polar Programs National Science.
A. Karle UW Madison 1. 2 Why neutrino astronomy? Astrophysical Accelerators Neutrinos allow for observation of ‘hidden regions’ of cosmic accelerators.
Frontiers in Contemporary Physics: May 23, 2005 Recent Results From AMANDA and IceCube Jessica Hodges University of Wisconsin – Madison for the IceCube.
First Results from IceCube Physics Motivation Hardware Overview Deployment First Results Conclusions & Future Plans Spencer Klein, LBNL for the IceCube.
Neutrino Astronomy at the South Pole David Boersma UW Madison Lake Louise Winter Institute Chicago, 23 February 2006.
SAC/PAP March 1, 2007Analysis plans IceCube analysis plans, Outline of presentation Initial emphasis on atmospheric neutrinos Use IceCube filter requests.
John Peoples for the DES Collaboration BIRP Review August 12, 2004 Tucson1 DES Management  Survey Organization  Survey Deliverables  Proposed funding.
CIPANP 2006K. Filimonov, UC Berkeley From AMANDA to IceCube: Neutrino Astronomy at the South Pole Kirill Filimonov University of California, Berkeley.
The Status of IceCube Mark Krasberg University of Wisconsin-Madison RICH 2004 Conference, Playa del Carmen, Mexico Dec 3, 2004.
Kara Hoffman, the University of Maryland. the Antarctic Muon and Neutrino Array.
News from the South Pole: Recent Results from the IceCube and AMANDA Neutrino Telescopes Alexander Kappes UW-Madison PANIC ‘08 November 2008, Eilat (Israel)
Searching for Quantum Gravity with AMANDA-II and IceCube John Kelley November 11, 2008 PANIC’08, Eilat, Israel.
Neutrino Astronomy at the South Pole Searches for astrophysical high-energy neutrinos with IceCube Kurt Woschnagg UC Berkeley Miami 2012 Lago Mar, Ft Lauderdale,
COSMO/CosPA 2010 Searches for the Highest Energy Neutrino with IceCube Searches for the Highest Energy Neutrino with IceCube Aya Ishihara ( Fellow) (JSPS.
B.Baret Vrije Univertsiteit Brusse l Vrije Universiteit Brussel, Belgium The AMANDA – IceCube telescopes & Dark Matter searches B. Baret on behalf of the.
IceCube a new window on the Universe Muons & neutrinos Neutrino astronomy IceCube science Status & plans Tom Gaisser for the IceCube Collaboration Arequipa,
IceCube and AMANDA: Neutrino Astronomy at the South Pole Brennan Hughey February 22nd, 2007.
1 Jan Conrad (CERN) GLAST Lunch, 09. Mar. 2006, Jan Conrad (KTH) The AMANDA neutrino telescope: Results from GRB and dark matter searches Jan Conrad (KTH,
The IceCube Neutrino Observatory is a cubic kilometer detector at the geographic South Pole. We give an overview of searches for time-variable neutrino.
Jan 16, 2004Tom Gaisser 1.3 Cost & schedule review The IceTop component of IceCube Area--solid-angle ~ 1/3 km 2 sr (including angular dependence of EAS.
KEK, Feb 27, 2006Tom Gaisser1 Cosmic-ray physics with IceCube IceTop the surface component of IceCube.
XIX European Cosmic Ray Symposium Firenze (Italy) Neutrino Astronomy and Cosmic Rays at the South Pole Latest.
Science Advisory Committee March 30, 2006 Jim Yeck IceCube Project Director IceCube Construction Progress.
David Seckel, IceTop Baseline Review, Madison, Dec. 4, 2003 IceTop Baseline Review Dec. 4, Madison WI.
IPPOG masterclass working group May 15, Building an IceCube Collaboration outreach activity Inspired by the International Masterclasses for hands-
IceCube: Status and Results
IceCube project Shigeru Yoshida Dept. of Physics, Chiba University.
Searching for Quantum Gravity with AMANDA-II and IceCube John Kelley IceCube Collaboration University of Wisconsin, Madison, U.S.A. October 27, 2008 KICP.
Icecube Neutrino Observatory at the South Pole Kirill Filimonov, University of California, Berkeley, for the IceCube Collaboration.
Nov 30, 2003Tom Gaisser The IceTop component of IceCube Perspective from the South Pole.
Alexander Kappes (E. Strahler, P. Roth) ECAP, Universität Erlangen-Nürnberg for the IceCube Collaboration 2009 Int. Cosmic Ray Conf., Łódź,
U.S. Department of Agriculture eGovernment Program February 25, 2003 USDA Presidential Initiatives Meeting Chris Niedermayer, USDA eGovernment Executive.
I Taboada, GA Tech High-energy neutrino astronomy with IceCube Ignacio Taboada Georgia Institute of Technology for the IceCube collaboration Madison, NDM.
South Pole Astro April 4, 2011 Tom Gaisser1 125 m Cosmic-ray physics with IceCube IceTop is the surface component of IceCube as a three-dimensional cosmic-ray.
1 Particles and Nuclei International Conference (PANIC05) Santa Fe, NM (U.S.A.) October 24 th, from Quark n.36, 02/01/04 Neutrino.
08/2006Julia Becker, Universität Dortmund TeV particle astrophysics, Madison Julia Becker for the IceCube collaboration August 2006 by the AMANDA experiment.
IceCube Neutrino Telescope Astroparticle Physics at the South Pole Brendan Fox Pennsylvania State University for the IceCube Collaboration VLVNT08 - Very.
Search for Ultra-High Energy Tau Neutrinos in IceCube Dawn Williams University of Alabama For the IceCube Collaboration The 12 th International Workshop.
High-energy Neutrino Astrophysics with IceCube Neutrino Observatory
Albrecht Karle University of Wisconsin - Madison for the IceCube Collaboration IceCube Current status, recent results and future prospects.
Dark Matter Searches with AMANDA and IceCube Catherine De Clercq for the IceCube Collaboration Vrije Universiteit Brussel Interuniversity Institute for.
1 IceCube Christian Spiering for the IceCube Collaboration EPSC, Cracow July 2009.
Downgoing Muons in the IceCube experiment: Final presentation for Phys 735, Particle, Prof. Sridhara Dasu L.Gladstone 2008 Dec 3.
Measuring the total neutrino cross section using the IceCube detector
SAC/PAP Review UW-Madison March 1-2, 2007
IceCube Construction Endgame
Governance and Collaboration By-Laws
Julia Becker for the IceCube collaboration
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Lake Louise Winter Institute 2009 Erik Strahler University of Wisconsin-Madison.
Simulation in IceCube Science Advisory Committee Meeting Paolo Desiati
IC40 Physics Run Preparations
IceCube Neutrino Telescope Astroparticle Physics at the South Pole
Status and prospects of the IceCube Neutrino Telescope
The IceCube Neutrino Telescope
AMANDA-II Point Source Search Results
M&O Homework Questions
Preliminary Project Execution Plan
Presentation transcript:

Madison, May 20, 2009 Tom Gaisser1 IceCube Collaboration Overview & Response to 2008 SAC Report

Madison, May 20, 2009 Tom Gaisser2 Calendar (Spring 2009) M&O “Lessons Leearned” workshop – February 3,4 Pole season ends – February 12 MREFC PY8 Funding Request submitted - February 12 Planning meeting at NSF – February 20 Software and Computing Advisory Panel – March IceCube/RPSC Planning Meeting – March 25 April 1: Project Year 8 begins, initial MREFC PY8 funding awarded Deep Core/86 string end-game plan submitted April 1 M&O proposal submitted April 7 Transition to IC59 – April ? Collaboration meeting – April 28 – May 2 Annual review at NSF – May 6-7 ICRC papers due May 15 (extended to May 22) Science Advisory Committee – May Future: IOFG ?

Madison, May 20, 2009 Tom Gaisser3 Outline 1.Successful season 19 strings (inc. 1 st deep core) 19 IceTop stations 2.Status report in response to SAC 2008 comments on Support for physics analysis Support for M&O of IceCube 3.Responses to specific recommendations of SAC 2008 on Analysis plans Publications Detector optimization R&D Data handling 4.Future SAC meetings

Madison, May 20, 2009 Tom Gaisser4 19 holes & strings in 50 days! L

Madison, May 20, 2009 Tom Gaisser5 38 IceTop tanks installed, filled, frozen & commissioned before station closing

Madison, May 20, 2009 Tom Gaisser6

Madison, May 20, 2009 Tom Gaisser7 Support for physics analysis The Committee was glad to see that real physics analysis is now starting using the IceCube data but would like to understand in the future how the analysis will be organized and how sufficient manpower will be gathered to cover all of the physics opportunities. MREFC ramp-down removes central support for young scientists. It is imperative that funding be secured for the next several years to allow this group to participate in the physics program of IceCube. If funding for 15 of these individuals can be obtained, the US effort can be brought to a healthy number, 28 scientists and 27 students plus faculty. –We recommend that the IceCube collaboration consider submitting a new coordinated supplemental grant proposal to empower the universities to play a leading role in IceCube physics program

Madison, May 20, 2009 Tom Gaisser8 Status of base grants & MOUs Annual NSF review was May 6, 7 –See executive summary report on docushare U.S. base grants being negotiated now Program officers using MOUs as guide to needed funding levels –Current round of proposals from U.S. groups Base grants receiving significant increases Somewhat less than requested M&O proposal assumes increased level in base grants –New institutions are getting support MOUs available by link / handout

Madison, May 20, 2009 Tom Gaisser9 Univ Alabama, Tuscaloosa Univ Alaska, Anchorage UC Berkeley UC Irvine Clark-Atlanta University U Delaware / Bartol Research Inst Georgia Tech University of Kansas Lawrence Berkeley National Lab University of Maryland Ohio State University Pennsylvania State University University of Wisconsin-Madison University of Wisconsin-RiverFalls Southern University, Baton Rouge Univ Alabama, Tuscaloosa Univ Alaska, Anchorage UC Berkeley UC Irvine Clark-Atlanta University U Delaware / Bartol Research Inst Georgia Tech University of Kansas Lawrence Berkeley National Lab University of Maryland Ohio State University Pennsylvania State University University of Wisconsin-Madison University of Wisconsin-RiverFalls Southern University, Baton Rouge  Universität Mainz Humboldt Univ., Berlin DESY, Zeuthen Universität Dortmund Universität Wuppertal MPI Heidelberg RWTH Aachen  Universität Mainz Humboldt Univ., Berlin DESY, Zeuthen Universität Dortmund Universität Wuppertal MPI Heidelberg RWTH Aachen Uppsala University Stockholm University Uppsala University Stockholm University Chiba University Chiba University Universite Libre de Bruxelles Vrije Universiteit Brussel Université de Mons-Hainaut Universiteit Gent Universite Libre de Bruxelles Vrije Universiteit Brussel Université de Mons-Hainaut Universiteit Gent Univ. of Canterbury, Christchurch University of Oxford University Utrecht The IceCube Collaboration: 33 institutions, ~250 authors EPFL Lausanne

Madison, May 20, 2009 Tom Gaisser10 Collaboration head count & FTE 33 Institutions –Faculty 62 (31 U.S., 33 non-U.S.) –Post-docs, etc. 57 (41 U.S., 16 non-U.S.) –Ph.D. students: 86 (33 U.S., 53 non-U.S.) –Total active: 207 (105 U.S., 102 non-U.S.) FTE breakdown (scientists only) –FTE in M&O: 45.5 (26* U.S., 19.5 non-U.S.) *26 U.S. includes 6 FTE requested in M&O proposal –FTE in Analysis 53 ( 24 U.S., 29 non-U.S.)

Madison, May 20, 2009 Tom Gaisser11 Collaboration resources in M&O Distributed Management and Funding Model (FY12 FTE) Distributed Management and Funding Model (FY12 FTE) FY12 (FTE) Oct'11 - Sep'12 Total US Europe & Asia Pacific In Kind (FTE) Total In Kind (FTE) M&O Core (FTE) US Base Grants (FTE) 2.1 PROGRAM MANAGEMENT DETECTOR OPERATIONS & MAINTENANCE COMPUTING AND DATA MANAGEMENT TRIGGERING AND FILTERING DATA QUALITY, RECONSTRUCTION & SIMULATION TOOLS In-kind Effort Still To Be Distributed Grand Total (FY12 FTE) ~ 5 FTE still on MREFC Requested

Madison, May 20, 2009 Tom Gaisser12 M&O support It is now imperative to provide the M&O funding so that the physics potential of the experiment can be exploited. Since this is an international experiment, other countries should also be providing their fair share of M&O support. –The Committee requests that the M&O funding plan be fully described at the next meeting and that the IceCube collaboration work with the NSF and other country agencies to assure that the M&O tasks are fully covered in a fair and adequate division.

Madison, May 20, 2009 Tom Gaisser13 Status of M&O Proposal submitted April 7 –Request support for 5 years starting 2010 –Review panel May 7 / 8 –MOU coordinated with M&O task list Emphasis on distribution of effort across the collaboration –Status report in Jim Yeck’s talk next on agenda

Madison, May 20, 2009 Tom Gaisser14 Analysis plans Recommendation 1.We recommend that each analysis topic establishes its own set of necessary tasks to be completed and clear milestone dates for their execution. 2.We would further suggest that by the time of our next meeting the Committee is presented with much more information on the plans for assessing systematic uncertainties for each of the main upcoming topics for the next 1- 2 years…. 3.Experimental cross checks, validation, and error assessment often require most of the effort. Responses – see Elisa Resconi’s presentation as analysis coordinator 1.Working group wiki’s 2.Systematic uncertainties a main focus of analysis phone calls & wiki and of calibration phone calls & wiki 3.L2a story as an example

Madison, May 20, 2009 Tom Gaisser15 IceCube Analysis & Ph.D. Theses Matrix (numbers in boxes indicate number of active Ph.D. theses; colored boxes indicate institutional activity in area) May 2009

IceCube overall Analysis Contribution Matrix (numbers in boxes indicate FTE effort on Ph.D. thesis work, preparation of papers, etc.) May 2009

Madison, May 20, 2009 Tom Gaisser17 Presentations at conferences Recommendation –The Committee would also recommend to the Collaboration to aggressively disseminate IceCube results in topical conferences. Response –ICRC papers –Speakers’ committee web page

Madison, May 20, 2009 Tom Gaisser18 Presentations at meetings - two examples Spring APS meeting (May 2-5, 2009) –Teresa Montaruli, “Recent results from IceCube” –I. Taboada, “Neutrino messengers from GRBs” –M. Baker, “Neutrino Point Source Searches with iceCube 22 String Configuration” –Laura Gladstone, “Observation of the Moon Shadow in the IceCube 40 string detector” –D. Besson, “Updates on IceCube's Radio Frequency extension” –D. Rocco Seasonal Variations of the Atmospheric Muon Flux in IceCube –R. Abbasi Large scale cosmic rays anisotropy as observed with IceCube 31 st International Cosmic Ray Conference (July 8-15, 2009) –Biennial –Major conference of particle astrophysics Auger, TA, etc Gamma-ray telescopes Neutrino astronomy –Total of 36 submitted: 19 talks; 17 posters with complementarity of posters/talks

Madison, May 20, 2009 Tom Gaisser19 First 3 months of 2009

Madison, May 20, 2009 Tom Gaisser20 Papers Recently published or accepted –Solar flare paper ApJ 689 No 1 (2008 December 10) L65-L68 –IceCube DAQ paper Nuclear Instruments and Methods in Physics Research A 601 (2009) 294–316 –AMANDA 7 year point source search Phys. Rev. D 79, (2009).) + events posted on webPhys. Rev. D 79, (2009).) –AMANDA 7 year atmospheric neutrinos PRD, Accepted –IC22 WIMP search, PRL, accepted In process –IC9 analysis of GRB B responding to reviewsIC9 analysis of GRB B –Sound speed paper out to collaborationSound speed paper –IC22 Point Source Paper out to collaborationIC22 Point Source Paper –IceCube PMT Paper almost readyIceCube PMT Paper

Madison, May 20, 2009 Tom Gaisser21 Papers (cont’d) Expected soon –GRB search(es), northern hemisphere –AMANDA cascades –IC40 Moon shadow –IC40 point source search Needed –CR anisotropy paper –IceCube atmospheric neutrinos –IceTop technical description paper Including performance –Atmospheric paper based on in-ice & IceTop rates –IceCube performance paper –Primary energy spectrum/composition

Madison, May 20, 2009 Tom Gaisser22 Detector optimization Recommendation on Deep Core (1 st priority) –Deep Core is a good idea; SAC endorses it 1.Provide info on angular resolution and background rejection 2.Put some High QE DOMs on central standard IceCube string 3.Decommission AMANDA –Response: 1-3 all done. See deep-core proposal, deep core talk next on agenda Recommendation: placement of outer strings 1.Try for further optimization of location of strings 2.Insure no negative impact on physics goals –Response: Optimized map; studies underway (see Karle’s talk)

Madison, May 20, 2009 Tom Gaisser23 Approach to R&D Recommendations 1.Take advantage of IceCube holes (unique opportunity) 2.May require seeking funding 3.Stronger engagement of Collaboration in R&D activities ICB review; milestones; progress reports 4.Develop plan for possible future use of drill Response: 1.R&D status reports on agenda in afternoon 2.Hoffman career grant features radio 3.Combined R&D working group established K. Helbing, chair; coordinate with M&O Improved focus and coordination of activities

Madison, May 20, 2009 Tom Gaisser24 Data handling Recommendations: –Develop more effective data compression to cope with high data rate –NSF roadmap for satellite bandwidth –Reorient simulations from MREFC to physics –Plan regular computing upgrades for data warehouse –Data challenge: signal insertion into data stream Responses: –Talks after lunch by Blaufuss/Hanson, Merck, Braun

Madison, May 20, 2009 Tom Gaisser25 Use of S.A.C. The Committee hopes that the comments of the SAC group are helpful for the IceCube program and encourages the collaboration to think about how the SAC can best be used in the future. We would like to arrange meetings so that more of the collaboration scientists are involved. –Two possibilities: Set SAC meeting to overlap with end of collaboration meeting SAC members attend some of collaboration meeting Some of both