The North America Array Technology Development and the Realization of the SKA-High Steven T. Myers NRAO 14 May 2009 USSKA Consortium Meeting Washington,

Slides:



Advertisements
Similar presentations
SKA New Technology Demonstrator Ray Norris CSIRO Australia Telescope National Facility.
Advertisements

SADC HPC Workshop, 2 Dec 2013, Cape Town
5-6 May 2009 AWG Meeting LAX1 Technology Development Project US contributions to global.
SKA South Africa Overview Thomas Kusel MeerKAT System Engineering Manager April 2011.
22 May 2008Lynn Baker USSKA Consortia Meeting Washington, DC1 Project Manager, Responsibilities and Tasks –Coordination between groups within the TDP –Promote.
C. ChandlerEVLA Advisory Committee Meeting September 6-7, Scientific Commissioning Plan Claire Chandler.
EVLA Early Science: Shared Risk Observing EVLA Advisory Committee Meeting, March 19-20, 2009 Claire Chandler Deputy AD for Science, NM Ops.
Transition from SKADS to PrepSKA Richard Schilizzi Lisbon, 3 October 2008.
New Mexico Symposium – 19 Oct S. T. Myers The Radio Synoptic Survey Telescope (RSST) A Square Kilometer Array Concept Steven T. Myers National Radio.
Chicago 3 in Washington, DC – 14 Sep S. T. Myers The Radio Synoptic Survey Telescope (RSST) Steven T. Myers National Radio Astronomy Observatory.
High Sensitivity VLBI Sheperd Doeleman MIT Haystack Observatory.
The Expanded Very Large Array: Phase I Science and Technical Requirements Rick Perley NRAO - Socorro.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Meeting Summary Richard.
The Square Kilometre Array: an update Steve Rawlings UoOxford and PrepSKA Coordinator Richard Schilizzi SKA Program Development Office Japan, November.
EVLBI and the Australian SKA Pathfinder (ASKAP) Prof. Steven Tingay Curtin University of Technology Perth, Australia 7th eVLBI workshop SHAO, 2008 June.
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
AAs in PEP Jan Geralt Bij de Vaate. PEP Project Execution Plan for the pre construction phase of the SKA Consortium to be formed AA-low ready for construction.
Moscow presentation, Sept, 2007 L. Kogan National Radio Astronomy Observatory, Socorro, NM, USA EVLA, ALMA –the most important NRAO projects.
EVLA Software Bryan Butler. 2007May22EVLA SAGE Meeting2 Requirements and Goals of EVLA Software Maximize scientific throughput of the instrument At a.
Arecibo Frontiers – 12 Sep Beyond the Frontiers: The Road From Arecibo to The Radio Synoptic Survey Telescope (RSST) Steven T. Myers National Radio.
Answers from the Working Group on AGN and jets G. Moellenbrock, J. Romney, H. Schmitt, V. Altunin, J. Anderson, K. Kellermann, D. Jones, J. Machalski,
Time domain science and LSST follow ‐ up in South Africa (+ SKA) Stephen Potter South African Astronomical Observatory.
SAGE meeting Socorro, May 22-23, 2007 EVLA Science Operations: the Array Science Center Claire Chandler NRAO/Socorro.
P. NapierEVLA Advisory Committee Meeting September 8-9, EVLA Advisory Committee Project Overview P. Napier, Project Manager Management, Schedule,
Large Area Surveys - I Large area surveys can answer fundamental questions about the distribution of gas in galaxy clusters, how gas cycles in and out.
P.NapierEVLA Advisory Committee, 11 June EVLA Phase II Implementation/Funding P. Napier.
P.NapierEVLA Advisory Comm, 14 Dec 2004 Project Overview Peter Napier, EVLA Project Manager Status 2003 Committee Response.
June 3,4 2010Lynn Baker USSKA Consortia Washington, DC1 TDP / AWG Update Lynn Baker USSKA Consortia Meeting Washington DC June 3,4, 2010.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing with NRAO.
ALMA Science Examples Min S. Yun (UMass/ANASAC). ALMA Science Requirements  High Fidelity Imaging  Precise Imaging at 0.1” Resolution  Routine Sub-mJy.
The North America Array Technology Development and the Realization of the SKA-High Steven T. Myers & Jim Ulvestad NRAO 15 Oct 2009 USSKA Consortium Meeting.
The SKA: Next Week, the Next 3 Years & Beyond Jim Cordes, Cornell University 24 August 01  Concepts  Science Goals & Payoffs  Configurations, Modes.
UlvestadEVLA Advisory Committee Meeting September 6-7, Future EVLA Operations Jim Ulvestad.
Future Radio Interferometers Jim Ulvestad National Radio Astronomy Observatory.
New Worlds, New Horzions, New Science – 09 Mar S. T. Myers Cosmological Galaxy Surveys: The Molecular Perspective Steven T. Myers (NRAO) *National.
An NSF Facility Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Gustaaf van MoorselEVLA Advisory Committee Meeting December 14-15, 2004 EVLA Computing End-to-end (E2e) software.
Rick PerleyEVLA Phase II Definition Meeting Aug 23 – 25, The Expanded Very Large Array Phase II Baseline Plan and Constraints.
Square Kilometre Array eInfrastructure: Requirements, Planning, Future Directions Duncan Hall SPDO Software and Computing EGEE 2009.
WIDAR Correlator Options and Potential Craig Walker NRAO Socorro U.S. VLBI Technical Coordination Meeting May 14-15, 2007.
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ngVLA: Reconfigurability.
Imaging issues Full beam, full bandwidth, full Stokes noise limited imaging Algorithmic Requirements: –PB corrections: Rotation, Freq. & Poln. dependence,
Bryan Butler EVLA Computing Division Head
Concepts for a Next-Generation VLBA
EVLA Basic Operations Jim Ulvestad
The Megamaser Cosmology Project
EVLA Project Peter Napier
VLA/VLBA INTEGRATION With appropriate outfitting, the VLA+NMA+VLBA could be one integrated instrument covering all resolutions from arcminutes to well.
Jim Cordes Cornell University
Shared Risk Observing Claire Chandler EVLA SSS Review, June 5, 2009
VLA to EVLA Transition Plan
Gustaaf van Moorsel September 9, 2003
Software Requirements
Shared Risk Science with the EVLA
SKADS White Paper - Technologies -
DVA1 as Part of the Dish Verification Program (DVP) Washington, DC P
SKA PEP - Dish Array WP5 Phase 1 Dishes with Single Pixel Feed Systems
Observatory Science Operations
A Draft Funding Model for the SKA
EVLA Algorithm Research & Development
EVLA Operations Jim Ulvestad
Observatory Science Operations
Correlator Growth Path
Joseph Lazio & Namir Kassim Naval Research Laboratory
Future Radio Interferometers
EVLA Construction Status
VLA EXPANSION PROJECT Correlator Issues.
Transition Observing and Science
Rick Perley NRAO - Socorro
Science with the Pathfinders and the Route to the SKA
Presentation transcript:

The North America Array Technology Development and the Realization of the SKA-High Steven T. Myers NRAO 14 May 2009 USSKA Consortium Meeting Washington, DC

The North America Array is... ● Technology development and prototyping program for the SKA-high component – Fully part of US and International SKA program – Some NRAO specific aspects ● Concept development for the expansion and incorporation of the EVLA/VLBA as the “SKA- high”, sited in North America – SKA-high siting proposal in – Astro2020 and construction in 2022+

Decadal Activity ● Subject of RFI response to RMS Program Prioritization Panel (Myers et al.) ● Components: – NRAO participation in SKA-mid precursors and pathfinders, such as MeerKAT and ATA – Continue and expand SKA TDP (TDP-II), extending to SKA-high antenna evaluation and NAA preparatory R&D – Construct a NAA Prototype Antenna Station connected to EVLA, develop SKA-high costing model and NAA site concept

NAA/SKA-high Science Goals ● Mostly taken from Astro2010 Science White Papers, broken down into those 5 areas – CFP: megamasers (dark energy, BH masses), weighing dark matter (lensing), – GCT: imaging galaxies in early Universe (lines, continuum), – PSSF: protoplanetary disks – SSE: super-star clusters and supernovae, SNe and GRB, obscured pulsars and motions – TGN: local group motions

High-Level “Design” ● SKA-high goals – GHz top-level spec – A/T = 5000 m 2 /K (~20 x EVLA) ● NAA concept – 1-50 GHz capability ● “core” 5-45 GHz, three 3:1 bands – At least 10 x EVLA sensitivity ● 5 x EVLA on NM baselines – Grow from EVLA + VLBA + GBT +ATA?

TDP-II ● 3 years ( ) $13450K ● Goals: – Continue and expand SKA TDP-I – Evaluate TDP/PrepSKA antennas for higher frequency operations to guide SKA-high design – NAA concept development and initial SKA-high systems design – Design for NAA Prototype Antenna Station and site choice

TDP-II Components 1. Antenna Evaluation 2. Data Transmission 3. Digital Signal Processing 4. Digitization 5. Monitor & Control 6. Wideband Feed/Receiver 7. Algorithms, Computing, Software 8. SKA-high/NAA Concept Design

NAA Prototype Antenna Station ● 4 years ( ) $17800K ● NAA-PAS Goals: – 1 year detailed design – 3 year prototype construction and evaluation – Develop SKA costing model – Develop NAA site proposal for SKA-high CFP (in 2018 or later) – Preparation for SKA-high Astro2020 proposal – Preparation for SKA-high construction 2022+

NAA Timeline ● 2009 – Form NRAO SKA Program Office ● 2010 – NRAO-MeerKAT collaboration start ● 2011 – Submit TDP-II NSF proposal ● 2012 – Begin TDP-II ● 2015 – Complete TDP-II ● 2015 – NAA-PAS decision point, proposal ● 2016 – NAA-PAS production readiness ● 2018 – NAA-PAS construction complete ● 2019 – NAA-PAS testing complete, A2020

Other aspects ● NRAO SKA Program Office ● NRAO MeerKAT collaboration (w/MOU) ● Possible NRAO ATA collaboration ● Connection to SKA-mid – Augment antenna evalution in (probably 1yr of extra TDP-II ~ $4M) – Testing using NAA-PAS + EVLA ● Revisit SKA-high science case ~ – next decade “knowledge explosion”

Comments and Issues ● Science case – room for improvement! – new cases, e.g. the CO Cosmic Web ● TDP-II scope and organization – intent: organized as TDP-I with USSKA – more direct NRAO involvement/funding – international participation? – need to propose in 2011 (or 2010) ● NRAO and SKA and NAA (also Fred's talk) – EVLA personnel available after 2012

Supplementary Slides ● FYI

NAA Proposed Cost Breakdown ● Table 7.1 from PPP submission (Myers et al.)

SKA Timeline ● SKA “official” timeline – TDP-I and PrepSKA complete – EVLA, ASKAP, MeerKAT complete – 2013 SKA-mid infrastructure emplacement – 2018 SKA-mid Phase 1 complete – SKA-high site selection – SKA Astro2020 preparation – SKA-high start – 2023 SKA-mid complete