We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco X-1 at 1-10 Hz time resolution. Lightcurves of the high excitation Bowen/Hell emission lines and a red continuum at lambda(c) similar to 6000 angstrom were obtained through narrow interference filters with ULTRACAM, and these were cross-correlated with simultaneous RXTE X-ray lightcurves. We find evidence for correlated variability, in particular when Sco X-1 enters the Flaring branch. The Bowen/Hell lightcurves lag the X-ray lightcurves with a light travel time which is consistent with reprocessing in the companion star while the continuum lightcurves have shorter delays consistent with reprocessing in the accretion disc
The Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma-Ray Observatory co...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...
We present preliminary results of a simultaneous X‐ray/optical campaign of the proto‐typical LMXB Sc...
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 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...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at t...
Bright, short duration X-ray flares from accreting compact objects produce thin, dust scattering rin...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
The Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma-Ray Observatory co...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...
We present preliminary results of a simultaneous X‐ray/optical campaign of the proto‐typical LMXB Sc...
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 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...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at t...
Bright, short duration X-ray flares from accreting compact objects produce thin, dust scattering rin...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
The Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma-Ray Observatory co...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
We analyze a large collection of RXTE archive data from 1997 April to 2003 August of the bright X-ra...