GALAXY EVOLUTION OPTICAL AND IR SURVEYS Lucia Pozzetti INAF Osservatorio Astronomico di Bologna.
F. Genova, Open Archive Forum, 02/05/141 On-line information in astronomy From networking to a virtual observatory.
The multi-wavelength context of the future gamma-ray instruments: X-rays T. Dotani 1), A. Bamba 2), T. Fujinaga 3,1) 1) ISAS/JAXA 2) Aoyama Gakuin Univ.
Dr. O.N. CHAUBEY Dr. R. CHANDRA. INDIAN NEWSPAPERS IN ENGLISH: GENESIS BENGAL GAZETTE OR CALCUTTA GENERAL ADVERTISER IN 1780; The Times of India in 1838.
Probing the Radio Counterpart of Gamma-ray Flaring Region in 3C 84 Hiroshi Nagai (National Astronomical Observatory of Japan) In collaboration with Monica.
Stephen C.-Y. Ng HKU. Outline What are pulsar wind nebulae? Physical properties and evolution Why study PWNe? Common TeV sources, particle accelerators.
Luke Drury Dublin Institute for Advanced Studies Luke Drury Dublin Institute for Advanced Studies Particle Acceleration in the Universe.
P.Coppi, Yale ? AGN à la Blandford, cont. [ What Worked, What Didn’t, and What Next? ]
Chandra Calibration Status Recent releases Current Calibration projects Cross-Calibration between Chandra and other X-ray telescopes Revisions.
I. Balestra, P.T., S. Ettori, P. Rosati, S. Borgani, V. Mainieri, M. Viola, C. Norman Galaxies and Structures through Cosmic Times - Venice, March 2006.
CfA Oct 8 2003 Determining the Cosmic Distance Scale with Galaxy Clusters Erik Reese University of California, Berkeley.
Chandra X-Ray Observatory CXC Paul Plucinsky EPI Cal 2010 1 Update on ACIS Operations I.New Patch for ACIS Flight SW II.Control of the ACIS FP temperature.
![P.Coppi, Yale ? AGN à la Blandford, cont. [ What Worked, What Didn’t, and What Next? ]](https://static.fdocuments.in/doc/330x215/56649d3f5503460f94a18bb8/pcoppi-yale-agn-a-la-blandford-cont-what-worked-what-didnt-and.jpg)
