P.R. Young, G. Del Zanna, H.E. Mason, G.A. Doschek, J.L. Culhane, H. Hara STFC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire, OX11 0QX, U.K. University College London, Department of Space and Climate Physics, Holmbury St. Mary, Dorking, Surrey, UK DAMTP, Centre for Mathematical Sciences, Cambridge, UK Code 7670, Naval Research Laboratory, Washington, DC 20375-5352, USA National A...

Nobuyuki IWAMOTO1,∗, Toshitaka KAJINO, Grant J. MATHEWS, Masayuki Y. FUJIMOTO and Wako AOKI National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan The Graduate University for Advanced Studies, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA Department of Physics, Hokkaido Univ...

P. R. Young, G. Del Zanna, H. E. Mason, K. P. Dere, E. Landi, M. Landini, G. A. Doschek, 1STFC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfor 2University College London, Department of Space and Climate Physics, 3DAMTP, Centre for Mathematical Sciences, 4George Mason University, 4400 University Dr., Fairfax 5Artep, Inc at Naval Research Laboratory, 4555 Overlook Ave. S.W., 6Code 7670, Na...

Taro MATSUO, Hiroshi SHIBAI, and Mitsunobu KAWADA Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 [email protected], [email protected], [email protected] Makoto HATTORI and Izumi S. OHTA Graduate School of Science, Tohoku University, 6-3 Aoba, Aramaki, Aoba-ku, Sendai 980-8578 [email protected], [email protected] and Hirosh...

a The Sudbury Neutrino Observatory (SNO) has unique capabilities as a supernova detector. In the event of a galactic supernova there are opportunities, with the data that SNO would collect, to constrain certain intrinsic neutrino properties significantly, to test details of the various models of supernova dynamics, and to provide prompt notification to the astronomical community through the Sup...

An interferometer system for use at the 2.34 meter Vainu Bappu Telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur, to obtain speckle-grams of astronomical objects in the visible wavelength, has been developed. Laboratory tests of resultant intensity distributions due to a point source, with phase modulation screens, as well as the images obtained using this interferometer at th...

We present the results of an intermediate resolution (∼ 2 Å) spectroscopy of a sample of 37 candidate Lyα blobs and emitters at redshift z = 3.1 using the DEIMOS spectrograph on the 10 m Keck telescope. The emission lines are detected for all the 37 objects and have variety in their line profiles. The Lyα velocity widths (FWHM) of the 28 objects with higher quality spectra, measured by fitting ...