'Scuba 2' presentation slideshows

Cornell-Caltech Atacama Telescope (CCAT)

Cornell-Caltech Atacama Telescope (CCAT). Rationale and science drivers Telescope Site Instruments Estimated performance Project schedule. A timely convergence of Science, Technology, and Opportunity Many sources emit most of their energy in the FIR/submm

670 views • 51 slides

The JCMT Nearby Galaxies Legacy Survey

The JCMT Nearby Galaxies Legacy Survey. Chris Wilson McMaster University 1. Survey design and goals 2. Science results. The JCMT Nearby Galaxies Legacy Survey team. C. Wilson, F. Israel, S. Serjeant (coordinators)

415 views • 32 slides

476 views • 30 slides

Distant galaxies

Distant galaxies. Eelco van Kampen, Institute for Astrophysics, Innsbruck, and Institute for Astronomy, Edinburgh with Jim Dunlop, John Peacock, Will Percival, Miller Crawford, Susie Scott (Edinburgh), And Chris Rimes (Colorado). Semi-numerical galaxy formation. Ingredients:.

438 views • 29 slides

Simulating Proto-clusters utilizing the Austrian Grid

Michaela Lechner Eelco van Kampen Daniel Clarke Simon Ostermann Manchester, May 2007. Simulating Proto-clusters utilizing the Austrian Grid. Institute of Astro- and Particle Physics Distributed and Parallel Systems Group Institute for Computer Science.

352 views • 27 slides

394 views • 26 slides

Dust-Obscured Galaxies (DOGs)

439 views • 24 slides

The JCMT Nearby Galaxies Legacy Survey

The JCMT Nearby Galaxies Legacy Survey. Chris Wilson McMaster University 1. Survey design and goals 2. Science results 3. Future surveys. The JCMT Nearby Galaxies Legacy Survey team. C. Wilson, F. Israel, S. Serjeant (coordinators)

382 views • 24 slides

Boulder

2. Boulder. A New Generation Submillimetre Camera for the James Clerk Maxwell Telescope. NIST Presentation. 2. Outline: Project summary Management plan and costs CoDR and Board outcomes Pre-select phase Agenda for this week. Boulder.

360 views • 24 slides

The Atmospheric Emission Signal as seen with SHARC-II

The Atmospheric Emission Signal as seen with SHARC-II. Alexander van Engelen University of British Columbia. Who am I?. Working with: Douglas Scott (UBC) Andy Gibb (UBC) Tim Jenness (JAC, Hilo HI) Dennis Kelly (UK ATC, Edinburgh) on the data reduction pipeline software for SCUBA-2

286 views • 20 slides

ETS meeting 01/17/08

332 views • 19 slides

CCAT and Star formation

CCAT and Star formation. Derek Ward-Thompson Cardiff University CCAT meeting 13/09/06. Where we are. The greatest advance SCUBA has given to star formation studies is wide-field sub-mm astronomy. SCUBA-2 will give us an even greater lead in this area. JCMT will close in 2012.

264 views • 17 slides

Strumentazione sub-mm/mm pre-ALMA

Strumentazione sub-mm/mm pre-ALMA. APEX SCUBA & SCUBA-2 IRAM SMA CSO OVRO, BIMA ? CARMA NMA. APEX : A tacama P athfinder EX periment. Location: Llano de Chajnantor (Chile, 5000 m) Antenna modified copy of US ALMA prototype MPIfR=50% Onsala Sp. Obs=23% ESO=27%

331 views • 16 slides

Allen et al. (2005)

Johnstone et al. (2000). Allen et al. (2005). Tracing Dense Core Structure with NH 3. Oph B2. NH 3 (1,1) int. intensity (GBT). 850 m m continuum (JCMT). NH 3 emission shows excellent (but not perfect) correspondence with dust continuum emission. Tracing Dense Core Structure with NH 3.

376 views • 15 slides

Allen et al. (2005)

Johnstone et al. (2000). Allen et al. (2005). Tracing Dense Core Structure with NH 3. Oph B2. NH 3 (1,1) int. intensity (GBT). 850 m m continuum (JCMT). NH 3 emission shows excellent (but not perfect) correspondence with dust continuum emission. Tracing Dense Core Structure with NH 3.

277 views • 15 slides

The JCMT in the ALMA Era

The JCMT in the ALMA Era. Surveying the Sub-millimetre Sky (Canada / Netherlands / Great Britain). Doug Johnstone NRC/HIA. A New Suite of Instruments. Faster bolometer array (SCUBA2) Continuum mapping at multiple wavelengths Ancillary devices (polarimeter, FTS)

258 views • 14 slides

Boulder

Boulder. SCUBA-2: The next generation submillimetre camera for the James Clerk Maxwell Telescope. 2. Top Level Requirements. 2. Summary of main requirements. A fully-sampled image plane covering at least 8 arcmin-square. Per-pixel sensitivity of < 65 and 320mJy/  Hz at 850 and 450 m.

289 views • 12 slides

SCUBA Polarization results: 1998-1999

SCUBA Polarization results: 1998-1999. Jane Greaves, Joint Astronomy Centre, Hawaii. with special thanks to: Wayne Holland, Tim Jenness, David Berry and Antonio Chrysostomou. SCUBA Polarimeter at the JCMT.

204 views • 9 slides

CCD-style imaging for the JCMT

CCD-style imaging for the JCMT. SCUBA-2 technology. To fill an 8 ? 8 arcmin field-of-view of the JCMT requires many thousands of pixels!. ? Conventional bolometer technology is impractical!. We need:. ? the ability to construct large format detector arrays.

101 views • 9 slides

3. Science Case

75 views • 1 slides