Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing with ALMA.

Slides:



Advertisements
Similar presentations
ALMA Cycle 2 Capability Jongsoo Kim ALMA EA Korea node.
Advertisements

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The March to Early.
Molecular Gas and Dust in COSMOS Submillimeter Galaxies Caption: Left: 0.3 deg 2 map of a COSMOS field with AzTEC on ASTE at 1.1mm (Scott et al. 2008,
ALMA: MM Observing Considerations
A Search For Fragmentation in Starless Cores with ALMA Scott Schnee (NRAO) Hector Arce, Tyler Bourke, Xuepeng Chen, James Di Francesco, Michael Dunham,
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Definitive Science with Band 3 adapted from the ALMA Design Reference Science Plan (
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array EVLA Observations of.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
TMT Instrumentation Canadian capabilities and interests David Loop, NRC-HIA June 26, 2010.
The North America ALMA Science Center (NAASC) John Hibbard NA ARC Manager (NRAO/NAASC) National Research Council Canada ESO ALMA Community Meeting, Garching,
Star Formation Research Now & With ALMA Debra Shepherd National Radio Astronomy Observatory ALMA Specifications: Today’s (sub)millimeter interferometers.
ALMA Proposal Preparation and Submission Eelco van Kampen European ALMA Regional Centre (ESO, Garching) Thanks to Liz Humphrys, Andy Biggs and Paola Andreani.
ALMA During Early Science
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Multiwavelength Continuum Survey of Protostellar Disks in Ophiuchus Left: Submillimeter Array (SMA) aperture synthesis images of 870 μm (350 GHz) continuum.
ALMA Proposal Preparation and Submission Liz Humphreys European ALMA Regional Centre ESO, Garching Thanks to Andy Biggs, Paola Andreani, Eelco van Kampen.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing the Pluto.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Emmanuel Momjian (NRAO)
From Idea to ALMA Project James Di Francesco Herzberg Institute of Astrophysics North American ALMA Science Center (thanks to Mike Rupen, Gianni Comoretto.
ALMA Operations and the North American ALMA Science Center Al Wootten NRAO.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The ALMA Observing.
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Tools for the ALMA.
EA ARC Ken Tatematsu East-Asian ARC Manager. ARC organization Difference between ARCS: NA: concentrated in Charlottesville Europe: distributed in different.
Molecular Gas and Dust in SMGs in COSMOS Left panel is the COSMOS field with overlays of single-dish mm surveys. Right panel is a 0.3 sq degree map at.
A Search for Hydroxlyamine (NH 2 OH) Towards IRC+10216, Orion-S, Orion(KL), SgrB2(N), SgrB2(OH), W512M, W3(IRS5) R. L. Pulliam NRAO / North American ALMA.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The Expanded Very Large.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The ALMA Observing.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The ALMA Observing.
An I3 funded by the EU through FP6 Alastair G Gunn University of Manchester Jodrell Bank Observatory OPTICON BOARD MEETING – 11 th /12 th October 2004,
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array THE GBT PRIMOS PROJECT.
NRAO Users Committee Meeting May 20-21, National Radio Astronomy Observatory NRAO Users Committee Meeting – May 20-21, 2008 ALMA Operations Chris.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Extragalactic Source.
Catalogues: Each 850  m field was analyzed with the 2-D CLUMPFIND identification algorithm (Williams, de Geus & Blitz 1994; ApJ, 428, 693) to produce.
The North American ALMA Science Center North America’s ALMA Regional Center The North American ALMA Science Center acts as the gateway to ALMA for North.
The JCMT in the ALMA Era Surveying the Sub-millimetre Sky (Canada / Netherlands / Great Britain) Doug Johnstone NRC/HIA.
Molecular Clouds in in the LMC at High Resolution: The Importance of Short ALMA Baselines T. Wong 1,2,4, J. B. Whiteoak 1, M. Hunt 2, J. Ott 1, Y.-N. Chin.
Imaging Molecular Gas in a Nearby Starburst Galaxy NGC 3256, a nearby luminous infrared galaxy, as imaged by the SMA. (Left) Integrated CO(2-1) intensity.
64th International Symposium on Molecular Spectroscopy June , 2009 – Columbus, Ohio MOLECULAR SPECTROSCOPY AND THE ATACAMA LARGE MILLIMETER/SUBMILLIMETER.
ALMA Polarization Commissioning and Verification Status Kouichiro Nakanishi (Joint ALMA Observatory/NAOJ) on behalf of ALMA Polarization Commissioning.
SAGE meeting Socorro, May 22-23, 2007 EVLA Science Operations: the Array Science Center Claire Chandler NRAO/Socorro.
Early Science Specification and Expected Array Evolution Masao Saito EA ALMA Project Scientist EA PS Report1 2nd ALMA Users Meeting 2011/1/13.
Elizabeth Stanway - Obergurgl, December 2009 Lyman Break Galaxies as Markers for Large Scale Structure at z=5 Elizabeth Stanway University of Bristol With.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The ALMA Observing.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing with NRAO.
ALMA and the Call for Early Science The Atacama Large (Sub)Millimeter Array (ALMA) is now under construction on the Chajnantor plain of the Chilean Andes.
ALMA Science Examples Min S. Yun (UMass/ANASAC). ALMA Science Requirements  High Fidelity Imaging  Precise Imaging at 0.1” Resolution  Routine Sub-mJy.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array The Expanded Very Large.
ALMA’s Roots in Three Scientific Visions Paul Vanden Bout NRAO The Dusty & Molecular Universe – Paris 28/10/04.
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA Pipeline.
Possible Future Spectroscopic Star Formation Surveys James Di Francesco (National Research Council Herzberg)
ALMA Project Status Adrian Russell. Where is ALMA? El llano de Chajnantor ALMA.
Atacama Large Millimeter/ submillimeter Array - ALMA ASAC Charges For Oct 31 ASAC Report to ALMA Board Al Wootten JAO Interim Project Scientist.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array VLA Observations of.
An NSF Facility Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array.
THE ALMA ORION BAND 6 SCIENCE VERIFICATION DATA SPECTRAL LINE SURVEY - CONTENT AND DISCOVERY AVAILABLE FOR ALL SCIENCE Anthony J. Remijan ALMA Program.
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
High Redshift Galaxies/Galaxy Surveys ALMA Community Day April 18, 2011 Neal A. Miller University of Maryland.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Using CASA to Simulate.
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ngVLA: Reconfigurability.
The North America ALMA Science Center
Committee Charge Fred K.Y. Lo
Atacama Large Millimeter Array
Welcome to the 4th NAIC-NRAO School on Single Dish Radio Astronomy
Rick Perley National Radio Astronomy Observatory
Welcome K. Y. Lo Director, NRAO
Presentation transcript:

Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing with ALMA The NAASC: Canadian Roles James Di Francesco Millimetre Astronomy Group Herzberg Institute of Astrophysics National Research Council of Canada

2 Who are we? National Research Council of Canada (NRC): - the Government of Canada’s premier organization for research and development (est. 1916) - Herzberg Institute of Astrophysics (HIA): - Canada’s “national laboratory” for astronomy - oversees Canadian involvement in national telescopes: e.g., Gemini, JCMT, DAO, DRAO, and now ALMA - Canada’s premier instrumentation team: e.g., Altair, GMOS (Gemini), WIDAR correlator (EVLA), Band 3 Receiver suite (ALMA) - Canadian Astronomy Data Centre: e.g, Gemini, JCMT, DRAO, BLAST archives - located in Victoria, BC (DAO) and Penticton, BC (DRAO)

3 Who are we? Millimetre Astronomy Group (MAG): - provided support for JCMT users for over 20 years - located in Victoria, BC - many combined years of millimetre/submillimetre single-dish/interferometer experience - transitioning to support for ALMA users in N. America - 4 members involved in ALMA support at present MAG roles in ALMA: - helpdesk support - proposal preparation, data quality analysis & processing - astronomer-on-duty support in Chile - user documentation JCMT SCUBA image of Ophiuchus Me at the AOSPACS image of η CorviHARP image of L1340

4 The ALMA Early Science Primer 40 pages of useful information about ALMA Early Science, written in plain language for non-experts project led by NRC-HIA, after successful earlier version made for Hamilton 2008 ALMA workshop; many contributions by the NA, EU, and EA regional centers Contains concise descriptions of: - Early Science capabilities - proposals - examples of possible projects - interferometric concepts - expected data flow Available for the low, low price of $0.00 at the NRAO booth!

5 Primer Example: ALMA data of Pluto Premise: - study CO in Pluto’s atmosphere - constrain temperature of Pluto/Charon - constrain sizes of Nix & Hydra Strategies: - Bands 7 & 9 (850 & 450 μm) - continuum and CO 3-2 data - angular resolution: - 0.8” & 0.4” FWHM respectively - spectral resolution: - continuum: mode 70 (8 GHz width) - CO 3-2: mode 8 (0.21 km/s channels) Desired Sensitivities: - continuum: 0.03 & 0.12 mJy/beam, allows 5 σ detections of Nix & Hydra - line: 10 mJy km/s, CO 3-2 peak should be mJy in a line ~1 km/s wide 1.4 mm observations of Pluto & Charon from the SMA by Gurwell & Butler (2005) at 0.4” FWHM resolution, made using the most extended configuration of the SMA

6 Primer Example: ALMA data of Pluto Expected Observing Times (determined through ALMA sensitivity calculator in OT): - Continuum: Band 7 & 9 need 8.5 hr & 8.3 hr of exceptional weather respectively - Line: CO 3-2 needs only 4.3 hr - CO 6-5 needs higher sensitivity than available in ES and Nix & Hydra need wider array to be resolved: will wait until Full Operations for these projects

7 Other Canadian Tools for ALMA JCMT archive at CADC: - contains public processed data products of continuum and line observations over the last 20 years over Bands 6, 7 and 9 - Google “JCMT archive” SCUBA/SCUPOL Legacy Catalogues: - contains stacked, smoothed images of continuum data at 850 & 450 mm from SCUBA ( ), calalogue of ~6100 identified objects - contains polarimetric data of 85 regions observed with the SCUBA polarimeter Di Francesco et al. (2008) Matthews et al. (2009)

8 Summary As your North American partners, Canada will contribute to supporting both the American and Canadian astronomical communities for ALMA NA user support will also come from the Millimetre Astronomy Group at the Herzberg Institute of Astrophysics “Observing with ALMA: A Primer for Early Science” will help with your ALMA plans Early Science proposals may also benefit from public data in the JCMT Archive at the CADC, as well as the SCUBA and SCUPOL Legacy Catalogue data products (view from our parking lot)