'Observing time' diaporamas de présentation

PISCO and ATCA Follow-on for SPT Clusters

PISCO and ATCA Follow-on for SPT Clusters. Antony A. Stark Smithsonian Astrophysical Observatory 18 May 2007. P arallel I mager for S outhern C osmology O bservations (PISCO): A Multiband Imager for Magellan. Antony Stark Smithsonian PI Christopher Stubbs Harvard PI

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Part I: General scheme of Subaru observing time and SSP Part II: SSP plan with FMOS

Part I: General scheme of Subaru observing time and SSP Part II: SSP plan with FMOS. Part 1 Subaru Strategic Programme. K. Ohta Kyoto Univ. June, 22, 2009 Oxford. Observing time category with FMOS. GTO (20 nights for FMOS builders) General open use - normal program: up to 5 nights

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Science Operations

Science Operations. Phil Edwards. 14 November 2016. Astronomy and space science. Outline. ATCA A Rorschach test Parkes Mopra Tidbinbilla ASKAP LBA 2017APR Feedback Now with added science highlights!. ATCA. ATCA forum convened last week to discuss rapid response observations

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An Introduction to Simdata

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Calvin-Rehoboth Robotic Twin Telescopes

Calvin-Rehoboth Robotic Twin Telescopes. Deborah Haarsma, Larry Molnar, David Van Baak (Calvin College) http://www.calvin.edu/observatory. Project Description. Goal: Give undergraduate students direct access to the physical universe, both eye-at-the-eyepiece and their own CCD images.

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Japanese VLBI programs, East Asian VLBI Network and Space VLBI;VSOP-2

Japanese VLBI programs, East Asian VLBI Network and Space VLBI;VSOP-2. H.Kobayashi(NAOJ) 2011, Jan., 27 Future of VLBA. First VLBI experiments between Korea and Japan(2001-2003). VY CMa SiO(J=2->1) 86 GHz. Shibata et al, 2003. VSOP ( 1997-2005)

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Fast Transient Detection with the (e)-EVN

Fast Transient Detection with the (e)-EVN. Andrew Siemion. Zsolt Paragi. Aard Keimpema. Commensal Fast Transient Detection with Interferometers and Possibilities for the (e)-EVN. Andrew Siemion. Zsolt Paragi. Aard Keimpema. Coherent emission mechanisms - physics of particle acceleration.

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How to Write a Convincing Technical Justification

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SOFIA SCIENCE UTILIZATION POLICIES Pamela M. Marcum SOFIA Project Scientist SSSC Feb 19, 2010

SOFIA SCIENCE UTILIZATION POLICIES Pamela M. Marcum SOFIA Project Scientist SSSC Feb 19, 2010. OVERVIEW. The purpose of this discussion is to give a overview of what the SOFIA Program-level policies are regarding data rights and observing policies.

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The Spitzer Legacy Program Lessons Learned T. SOIFER

The Spitzer Legacy Program Lessons Learned T. SOIFER. Spitzer Legacy Principles. Fundamental Principles of (Spitzer) Legacy Science Program Large coherent science investigations, not reproducible by any reasonable number or combination of smaller GO programs

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Multiwavelength Continuum Survey of Class 0/I disks in Ophiuchus

Science Goal: To observe the variation in the dust SED between disks We will observe the dust continuum emission from all 28 Class 0/I disks in the Ophiuchus molecular cloud identified by c2d (Enoch et al. 2009) Receivers: Bands 3, 6, 7 & 9 (110, 230, 345 and 690 GHz)

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