Simulation of ALMA. observation of SZ. decrement. in Perseus cluster. Bubble profiles ... we hope. LWA, eLOFAR. mm. VLBI. ALMA. GLAST. VSOP-2. EVLA. eMERLIN ...
Raw data formats depend on the waveband. Radio complex visibilities in u-v plane ... Lots of new facilities: XMM-Newton, Chandra, INTEGRAL, eMERLIN, GAIA, ALMA, ...
SAGE Science Advisory Group for EVLA K. Y. Lo SAGE Purpose/History Science Advisory Group for the EVLA formed by the Director to advise the NRAO on optimizing the ...
Science with the SKA: A Next Generation World Radio Observatory (AR ... Canadian aerostat. US Large N. Australian Luneburg Lenses. Dutch fixed planar array (cf. ...
Produce a deployment plan for the full SKA and a detailed costed system ... Y3 report detailing performance and cost data for composite MeerKat antenna. 36. CO ...
2. Key science programs ( level 0'): defined and disseminated ... Cherenkov radiation from neutrino interactions in lunar regolith (0.2 - 1GHz) SKA ...
... submission, and handling of ... submitted manually or chosen dynamically (think of Barry Clark for the VLA) ... Led by Sanjay Bhatnagar, Steve Myers ...
a lens or a mirror collects the light & brings it to a focus. a spectrograph separates the different frequencies. 3 ... In an interferometer, the correlator ...
www.merlin.ac.uk/e-merlin. Fibre connection to telescopes; ... MERLIN. Chandra. Main sequence and evolved stars novae, ... July 2006: MERLIN shutdown for ...
Galaxies Through CosmicTime. 2. Star-formation, AGN, or ? ... See through gas and dust. Morphology/Tb (resolution) Spectra (a -0.4 indicates AGN) (S a ?a) ...
Many nifty targeted, special-interest surveys. Canadian Galactic Plane Survey (CGPS) ... Archive reports BW, time on source, and theoretical rms noise (what you could ...
RadioNet FP6 runs until 31/12/08, 20 months. proposal ... Overall aim is focused, realistic and concrete ... Do some special tricks or non-standard processing ...
And it is still not up to speed with the instruments available ... test observations made with WSRT-VLA-MERLIN baselines (Rioja et al. 1997, Porcas ...
uJy sensitivity; 50-150 mas resolution key science driver for e-MERLIN ~1500 sources for deep 1.5 GHz field. AG, VO tools already essential for multi-l ...