activity
19982002
most citedThe census of cataclysmic variables in the ROSAT Bright Survey

82 citations · 137 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph2002★ 82 cited

The census of cataclysmic variables in the ROSAT Bright Survey

A. D. Schwope, H. Brunner, D. Buckley +5

We give an identification summary and results of polarimetric, photometric and spectroscopic follow-up observations of new, X-ray bright cataclysmic variables. These were identifie…

astro-ph2000★ 9 cited

High Speed Phase-Resolved 2-d UBV Photometry of the Crab pulsar

A. Golden, A. Shearer, R. M. Redfern +5

We report a phase-resolved photometric and morphological analysis of UBV data of the Crab pulsar obtained with the 2-d TRIFFID high speed optical photometer mounted on the Russian…

astro-ph2000

The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS sources with PSPC countrate CR > 0.2 s-1

A. D. Schwope, G. Hasinger, I. Lehmann +7

We present a summary of an identification program of the more than 2000 X-ray sources detected during the ROSAT All-Sky Survey (Voges et al. 1999) at high galactic latitude, |b| >…

astro-ph1998★ 44 cited

The ROSAT BRIGHT survey: I. Identification of an AGN sample with hard ROSAT X-ray spectra

J. -U. Fischer, G. Hasinger, A. D. Schwope +5

The ROSAT Bright Survey (RBS) aims to completely optically identify the more than 2000 brightest sources detected in the ROSAT all-sky survey at galactic latitudes |b| > 30 degr (e…

astro-ph1998★ 1 cited

A Search for the Optical Counterpart of PSR B1951+32 in the Supernova Remnant CTB 80

Creidhe O'Sullivan, A. Shearer, M. Colhoun +8

Using time-resolved two-dimensional aperture photometry we have put upper limits on the pulsed emission from two proposed optical counterparts for PSR B1951+32. Our pulsed upper li…

astro-ph1998★ 1 cited

Pulsed optical emission from Geminga

A. Shearer, A. Golden, S. Harfst +9

We present optical data which shows that G", the optical counterpart of the gamma-ray pulsar Geminga, pulses in B with a period of 0.237 seconds. The similarity between the optical…