The INTEGRAL Science Data Centre (ISDC)
By T. Courvoisier, Roland Walter, V. Beckmann, A. Dean, P. Dubath, R. Hudec, P. Kretschmar, Sandro Mereghetti, T. Montmerle, Nami Mowlavi and 10 more. 2001
290 citations recorded by the source corpus.
The INTEGRAL Science Data Centre (ISDC) provides the INTEGRAL data and means to analyse them to the scientific community. The ISDC runs a gamma ray burst alert system that provides the position of gamma ray bursts on the sky within seconds to the community. It operates a quick-look analysis of the data within few hours that detects new and unexpected sources as well as it monitors the instruments. The ISDC processes the data through a standard analysis the results of which are provided to the observers together with their data.
Subfields: Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/bf245b7c072d3cd3f45ed9f9b9f80fb417395d47
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Citations in the corpus
- Positron annihilation spectrum from the Galactic Centre region observed by SPI/INTEGRAL (2004, methodology): “For our analysis we use only single and PSD events and when available we use consolidated data provided by INTEGRAL Science Data Center (ISDC, Courvoisier et al, 2003).”
- OMC: An Optical Monitoring Camera for INTEGRAL Instrument description and performance (2003, methodology): “The data are received at the Integral Science Data Center (Courvoisier et al. 2003), where they are completely processed in an automatic way.”
- Discovery of Luminous Pulsed Hard X-Ray Emission from Anomalous X-Ray Pulsars 1RXS J1708–4009, 4U 0142+61, and 1E 2259+586 by INTEGRAL and RXTE (2006, methodology): “Most of the INTEGRAL data reduction in this study was performed with the Offline Scientific Analysis (OSA) version 4.1 distributed by the INTEGRAL Science Data Centre ( ISDC; see, e.g., Courvoisier et al. 2003).”
- Unveiling Supergiant Fast X-Ray Transient Sources with INTEGRAL (2006, methodology): “The reduction and analysis of the ISGRI data have been performed by using the INTEGRAL Offline Scientific Analysis (OSA) v.4.2 available to the public through the INTEGRAL Science Data Centre ISDC (Courvoisier et al. 2003).”
- THE FOURTH IBIS/ISGRI SOFT GAMMA-RAY SURVEY CATALOG (2009, methodology): “After removal of pointings flagged as Bad Time Intervals (BTI) by the Science Data Centre (Courvoisier et al. 2003) this number is reduced to 39548 science windows of good quality data.”
- Probing clumpy stellar winds with a neutron star (2007, methodology): “The ISGRI data are reduced using the INTEGRAL Offline Scientific Analysis (OSA) version 6.0 software publicly released by the INTEGRAL Science Data Centre (Courvoisier et al. 2003).”
- SPI observations of the diffuse ^60Fe emission in the Galaxy (2007, background): “…predesignated targets, with a fixed orientation for intervals of typically ∼2000 s (referred to as pointings), which are successively arranged as a standard pattern of neighbouring pointings 2◦ apart (dithering), and covering target region of interest for improved imaging (Courvoisier et al. 2003).”
- The INTEGRAL/IBIS scientific data analysis (2003, methodology): “The specific procedure for the IBIS data analysis starts from the data files obtained with the Integral Science Data Center (ISDC) (Courvoisier et al. 2003) preprocessing and performs a number of analysis steps which are hereafter described for the IBIS standard and photon-photon modes and the ISGRI”
- INTEGRAL observations of recurrent fast X-ray transient sources (2005, methodology): “The reduction and analysis of the IBIS/ISGRI data have been performed by using the INTEGRAL Offline Scientific Analysis (OSA) v.4.1 available to the public through the INTEGRAL Science Data Centre ISDC (Courvoisier et al. 2003).”