activity
19982008
most citedThe O-C diagram of the subdwarf B pulsating star HS2201+2610: detection of a giant planet?

1 citations · 1 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph2008

Towards Asteroseismology of PG1605+072

A. Tillich, U. Heber, S. J. O'Toole +2

We present our attempt to characterise the frequency spectrum of the bright V 361 Hya star PG1605072 from atmospheric parameter and radial velocity variations through a spectros…

astro-ph2007

Six New ZZ Ceti Stars from the SPY and the HQS Surveys

B. Voss, D. Koester, R. Østensen +3

We report on the discovery of six new ZZ Ceti stars. They were selected as candidates based on preparatory photometric observations of objects from the Hamburg Quasar Survey (HQS),…

astro-ph20071 cited

The O-C diagram of the subdwarf B pulsating star HS2201+2610: detection of a giant planet?

R. Silvotti, S. Schuh, R. Janulis +9

In this article we present the O-C diagram of the hot subdwarf B pulsating star HS2201+2610 after seven years of observations. A secular increase of the main pulsation period, Pdot…

astro-ph2001

Multiwavelength observations revealing the outbursts of the two soft X-ray transients XTE J1859+226 and XTE J1118+480

S. Chaty, C. A. Haswell, R. I. Hynes +9

We report here on multiwavelength observations of the two new soft X-ray transients (SXTs) XTE J1859+226 and XTE J1118+480, which we observed with HST/RXTE/UKIRT. For XTE J1118+480…

astro-ph1998

Three photometric methods tested on ground-based data of Q 2237+0305

I. Burud, R. Stabell, P. Magain +5

The Einstein Cross, Q~2237+0305, has been photometrically observed in four bands on two successive nights at NOT (La Palma, Spain) in October 1995. Three independent algorithms hav…

astro-ph1998

High resolution optical and near-IR imaging of the quadruple quasar RX J0911.4+0551

I. Burud, F. Courbin, C. Lidman +10

We report the detection of four images in the recently discovered lensed QSO RX J0911.4+0551. With a maximum angular separation of 3.1", it is the quadruply imaged QSO with the wid…