We present preliminary results of a simultaneous X‐ray/optical campaign of the proto‐typical LMXB Sco X‐1 at 1–10 Hz time resolution. Lightcurves of the high excitation Bowen/HeII emission lines were obtained through narrow interference filters with ULTRACAM, and these were cross‐correlated with X‐ray lightcurves. We find evidence for correlated variability, in particular when Sco X‐1 enters the Flaring Branch. The Bowen/HeII lightcurves lag the X‐ray lightcurves with a light travel time which is consistent with reprocessing in the companion star
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco...
We present simultaneous X-ray (RXTE) and optical (ULTRACAM) narrow-band ( Bowen blend/He II and near...
We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco...
We present simultaneous high time resolution (1-10 Hz) X-ray and optical observations of the persist...
Sco X-1 has been the subject of many multiwavelength studies in the past, being the brightest persis...
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the Rossi X-Ray Tim...
We present a multi-wavelength study of the low-mass X-ray binary Sco X-1 using Kepler K2 optical dat...
We analyze Rossi X-ray Timing Explorer (RXTE) Proportional Counter Array (PCA) data of the transient...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
Spectroscopically, tidal disruption events (TDEs) are characterized by broad (∼104 km s−1) emission ...
Phase-resolved VLT spectroscopy of the bursting Low Mass X-ray Binaries 4U 1636-536/V801 Ara and 4U ...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco...
We present simultaneous X-ray (RXTE) and optical (ULTRACAM) narrow-band ( Bowen blend/He II and near...
We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco...
We present simultaneous high time resolution (1-10 Hz) X-ray and optical observations of the persist...
Sco X-1 has been the subject of many multiwavelength studies in the past, being the brightest persis...
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the Rossi X-Ray Tim...
We present a multi-wavelength study of the low-mass X-ray binary Sco X-1 using Kepler K2 optical dat...
We analyze Rossi X-ray Timing Explorer (RXTE) Proportional Counter Array (PCA) data of the transient...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
Spectroscopically, tidal disruption events (TDEs) are characterized by broad (∼104 km s−1) emission ...
Phase-resolved VLT spectroscopy of the bursting Low Mass X-ray Binaries 4U 1636-536/V801 Ara and 4U ...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...