activity
19972013
most citedCharacterization of Large Volume 3.5 x 8 inches LaBr3:Ce Detectors

109 citations · 208 across the 7 of their papers we have counts for

collaborators

7 papers

physics.ins-det2013★ 109 cited

Characterization of Large Volume 3.5 x 8 inches LaBr3:Ce Detectors

A. Giaz, L. Pellegri, S. Riboldi +18

The properties of large volume cylindrical 3.5 x 8 inches (89 mm x 203 mm) LaBr3:Ce scintillation detectors coupled to the Hamamatsu R10233-100SEL photo-multiplier tube were invest…

cond-mat.mtrl-sci2012★ 25 cited

Picosecond dynamics of hot carriers and phonons and scintillator non-proportionality

A. Kozorezov, J. K. Wigmore, A. Owens

We have developed a model describing the non-proportional response in scintillators based on non-thermalised carrier and phonon transport. We show that the thermalization of e-h di…

physics.ins-det2011★ 8 cited

Synchrotron radiation studies of spectral response features caused by Te inclusions in a large volume coplanar grid CdZnTe detector

Conny C. T. Hansson, Alan Owens, Francesco Quarati +3

We report preliminary results from a synchrotron radiation study of Te inclusions in a large volume single crystal CdZnTe (CZT) coplanar-grid detector. The experiment was carried o…

astro-ph1999★ 2 cited

BeppoSAX broad-band observations of Gamma Cassiopeiae

A. Owens, T. Oosterbroek, A. N. Parmar +3

We report broad-band X-ray measurements of the Be star Gamma Cassiopeiae by the BeppoSAX X-ray astronomy satellite. The observations took place on 1998 July, 18-23. The 0.1-200 keV…

astro-ph1999★ 5 cited

A BeppoSAX observation of the massive X-ray binary 4U1700-37

A. P. Reynolds, A. Owens, L. Kaper +2

A 0.5-200 keV BeppoSAX spectrum of the non-pulsating high-mass X-ray binary 4U1700-37 is presented. The spectrum is well characterized by the standard accreting pulsar model of an…

astro-ph1998★ 2 cited

The absorption properties of gamma-ray burst afterglows measured by BeppoSAX

Alan Owens, M. Guainazzi, T. Oosterbroek +14

We present an analysis of the X-ray absorption properties of 6 gamma-ray burst (GRB) afterglows measured with BeppoSAX. Between 8 hrs and 20 hrs after the initial GRB trigger, indi…