activity
19982003
most citedThe PROOF Distributed Parallel Analysis Framework based on ROOT

34 citations · 34 across the 1 of their papers we have counts for

collaborators

6 papers

physics.data-an200334 cited

The PROOF Distributed Parallel Analysis Framework based on ROOT

Maarten Ballintijn, Rene Brun, Fons Rademakers +1

The development of the Parallel ROOT Facility, PROOF, enables a physicist to analyze and understand much larger data sets on a shorter time scale. It makes use of the inherent para…

astro-ph2000

Spectral analysis of multi mode pulsating sdB stars II. Feige 48, KPD 2109+4401 and PG 1219+534

U. Heber, I. N. Reid, K. Werner

Three members of the new class of pulsating sdB stars (sdBV or EC 14026 stars) are analysed from Keck HIRES spectra using line blanketed NLTE and LTE model atmospheres. Atmospheric…

astro-ph2000

Kinematics and morphology of the Narrow-Line Region in the Seyfert galaxy NGC1386

J. Rossa, M. Dietrich, S. J. Wagner

We present a high spatial and spectral resolution 2-D echelle spectrogram of the Narrow-Line Region in the Seyfert 2 galaxy NGC1386. This Seyfert galaxy was observed with CASPEC in…

astro-ph2000

The enigmatic soft X-ray NLS1 RX J0134.2-4258

D. Grupe, K. M. Leighly, H. -C. Thomas +1

We report the discovery and analysis of the follow-up ROSAT pointed observation, an ASCA observation and optical and radio observations of the enigmatic Narrow-Line Seyfert 1 galax…

astro-ph1998

The effect of metallicity on the Cepheid P-L relation, from a Baade-Wesselink analysis of SMC Cepheids

Jesper Storm, Bruce W. Carney, Anne M. Fry

We present results based on a Baade-Wesselink analysis of Cepheids in the Small Magellanic Cloud. The Baade-Wesselink analysis provides individual luminosities for these metal-poor…

astro-ph1998

Discovery of the secondary star of the HgMn binary kappa Cancri

T. Ryabchikova, O. Kotchoukhov, G. Galazutdinov +2

A careful investigation of a CCD spectrum of the SB1 system kappa Cnc in the spectral region 3800 A - 8000 A resulted in the discovery of the lines of the secondary star. We then a…