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20002007
most citedMultiwavelength Observations of Markarian 421 in March 2001: an Unprecedented View on the X-ray/TeV Correlated Variability

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astro-ph2007220 cited

Multiwavelength Observations of Markarian 421 in March 2001: an Unprecedented View on the X-ray/TeV Correlated Variability

G. Fossati, J. H. Buckley, I. H. Bond +26

(Abridged) We present a detailed analysis of week-long simultaneous observations of the blazar Mrk421 at 2-60 keV X-rays (RXTE) and TeV gamma-rays (Whipple and HEGRA) in 2001. The…

astro-ph2005

Time-resolved observations of the short period CV SDSS J123813.73-033933.0

S. V. Zharikov, G. H. Tovmassian, R. Napiwotzki +2

We observed a new and poorly studied cataclysmic variable (CV) SDSS J123813.73-033933.0 to determine its classification and binary parameters. Simultaneous time-resolved photometri…

astro-ph2004

Time-resolved observations of the short period CV SDSS J123813.73-033933

S. V. Zharikov, G. H. Tovmassian, V. Neustroev +2

We present simultaneous spectral and photometric observations of SDSS J123813.73-033933.0. From Ha radial velocity measurements we determined the orbital period of the system to be…

astro-ph2003

The distance and radius of the neutron star PSR B0656+14

W. F. Brisken, S. E. Thorsett, A. Golden +1

We present the result of astrometric observations of the radio pulsar PSR B0656+14, made using the Very Long Baseline Array. The parallax of the pulsar is pi = 3.47 +- 0.36 mas, yi…

astro-ph2003

Measuring the Absolute Height and Profile of the Mesospheric Sodium Layer using a Continuous Wave Laser

D. J. Butler, R. I. Davies, R. M. Redfern +2

We have developed and tested a novel method, based on LIDAR, of measuring the height and profile of the mesospheric sodium layer using a continuous wave laser. It is more efficient…

astro-ph2000

A 2.14 ms Candidate Optical Pulsar in SN1987A

J. Middleditch, J. A. Kristian, W. E. Kunkel +10

We have monitored Supernova 1987A in optical/near-infrared bands from a few weeks following its birth until the present time in order to search for a pulsar remnant. We have found…