0000000000620306

AUTHOR

P. Dubath

showing 2 related works from this author

The INTEGRAL/SPI response and the Crab observations

2004

The Crab region was observed several times by INTEGRAL for calibration purposes. This paper aims at underlining the systematic interactions between (i) observations of this reference source, (ii) in-flight calibration of the instrumental response and (iii) the development and validation of the analysis tools of the SPI spectrometer. It first describes the way the response is produced and how studies of the Crab spectrum lead to improvements and corrections in the initial response. Then, we present the tools which were developed to extract spectra from the SPI observation data and finally a Crab spectrum obtained with one of these methods, to show the agreement with previous experiments. We …

[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics - Instrumentation and Detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]INTEGRAL/SPIAstrophysics (astro-ph)instrumental responseFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]CrabAstrophysicscalibration
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TheINTEGRALspectrometer SPI: performance of point-source data analysis

2005

The performance of the SPI point-source data analysis system is assessed using a combination of simulations and of observations gathered during the first year of INTEGRAL operations. External error estimates are derived by comparing source positions and fluxes obtained from independent analyses. When the source detection significance provided by the SPIROS imaging reconstruction program increases from ∼10 to ∼100, the errors decrease as the inverse of the detection significance, with values from ∼10 to ∼1 arcmin in positions, and from ∼10 to ∼1 per cent in relative flux. These errors are dominated by Poisson counting noise. Our error estimates are consistent with those provided by the SPIRO…

Statistical noisePoint sourceInstrumentationdata analysis -gamma raysPoisson distribution01 natural sciencesNoise (electronics)[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesakeSignal-to-noise ratioOptics0103 physical sciencesSpurious relationship010303 astronomy & astrophysicsinstrumentationPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryAstronomy and AstrophysicsComputational physicsobservationsSpace and Planetary SciencesymbolsDeconvolutionbusinessmiscellaneous -methodsMonthly Notices of the Royal Astronomical Society
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