Chad Edwards; Ph.D. in particle physics in 1984, started first real job at JPL ... Geostationary orbit above Atlantic Ocean, downlink to White Sands, New Mexico ...
Enhanced data delivery and science support desired for all astronomers, but ... Robust maintenance of aging infrastructure (buildings, antennas, railroad) is required ...
(Lecture 10, Synthesis Imaging II, p. 187; Cornwell & Fomalont) Basic theory. Some choices ... errors tend to be relatively unimportant at dynamic ranges 1000 or so ...
... as being critical in acceleration and collimation of relativistic cosmic jets ... Image jet collimation within 200 Schwarzschild radii of a number of nearby black ...
Several small initiatives recommended by the committee span both ground and space. ... up-take (G. Djorgovski, P. Pinto, M. Donahue, J. Ulvestad, F. Hill, B. Wilkes) ...
... might be best candidates to harbor binary BHs. 8. U. Ulvestad & Ho 2001 ... radio binary BHs? ... Birth of stellar-mass BHs in starburst/merger galaxies such ...
Tenth Summer Synthesis Imaging Workshop. University of New ... Brighten and deflect. Gomez et al. 2000. 26. Where Most X-rays & ?-rays Are Emitted. clouds ...
Focus on project deliverables, without losing sight of a ... Disbanded international consortium. AIPS 'Project' is no more, but AIPS code base remains ...
Work Breakdown Structure (WBS) 6.01 Project Management. 6.02 System Integration and ... CE probably too high for Operations Budget to cover over next few years. ...
Title: The Expanded Very Large Array Author: AOCPub Last modified by: tromero Created Date: 8/20/2001 2:45:28 PM Document presentation format: On-screen Show
... other AGN in June with the ATCA at high resolution (22 GHz) ... VLBI can provide high resolution images but unless careful only over small fields of view. ...
Need much better sensitivity to get near Cas A power, or to observe many more modest starbursts ... needs lots of long(ish) baselines, and frequencies above a ...
Title: Pulsar Powerhouse: The Center of the Crab Nebula Author: M Bietenholz Last modified by: michael Created Date: 1/4/1980 12:41:10 AM Document presentation format
AGN Unification-1 History The present status Aims and objectives Review the arguments that led to unified schemes. Outline the different schemes, their strengths and ...
Wide range of frequency bands, 0.3-86 GHz, frequency agility ... Nearby, low-luminosity AGNs may be a GLAST 'sleeper' Mrk 421, 501. M87, N4151. Nearby GRBs? ...
The Radio-Loud/Radio-Quiet Dichotomy of AGN. Brandon Kelly. Astro 596. History ... 1963- Maarten Schmidt realized that bright optical point source associated with ...
To increase science impact and throughput via improved quality of data and ... ideas, clarifying objectives/task definitions, communicating across sites more ...
Time of day. Season. Year ~ sunspot number. If trial array ... Fails, pick another ... R. Becker, A. Brown, M. Elvis, S. Kurtz, A. Sarma, N. Vogt, R. Zavala ...
Radio jets reflect the accretion history of black holes in the universe. ... Black holes stand out with high brightness temperature compact flat-spectrum radio cores. ...
... x 5' region, so yield integrated spectral properties on ~200 pc spatial scales. Individual 8-m UTs will give angular resolution of 0.2' (spatial scales of 3 pc) ...
NVO Study of Super Star Clusters in Nearby Galaxies. Ben Chan, Chris Hanley, ... a plot of the magnitude of the brightest cluster in a galaxy vs. the log of the ...
NEXT SPACE VLBI MISSION, ASTRO-G (VSOP-2) AND ITS SPECTRUM MANAGEMENT ASTRO-G Project (JAXA) Y. Murata JAXA) HALCA and VSOP (1997-2005) VSOP with HALCA The first ...
... 1 Galaxies. Steve Kraemer (Catholic Univ. of America) Properties of Seyfert Galaxies ... All galaxies with central bulges harbor supermassive black holes: ...
Harry Ferguson. Wes Traub. David Spergel. Mike Shara ... Craig Hogan Chuck Bennett (GSFC) Sterl Phinney Michael Turner (NSF) Rene Ong Jacob van Zyl (JPL) ...
Special Astrophysical Observatory (SAO) of the Russian Academy of Sciences. WWW page: ... MPFS=MultiPupil Fiber Spectrograph. Spatial sampling: 0.5', 0.75', 1.0' ...
... energies from X-ray to radio, and including images, object lists, and ... Chandra X-ray image (SAO/CXC) USC/ISI. ROSAT image (GSFC/HEASARC) UW-Madison/NCSA ...
NASA s Beyond Einstein Program: An Architecture for Implementation Committee Charge Assess the five proposed Beyond Einstein missions (Constellation-X, Laser ...
tude des noyaux actifs de galaxies en interf rom trie optique : ... Ce serait l'instrument id al pour l' tude du c ur des noyaux actifs de galaxies ...
VLBA Observations of EGRET Blazars. Why were some strong radio quasars detected by EGRET while others like 3C345 were not? ... EGRET VLBA observations (1994-1997) ...