Monte-Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis
arXiv:astro-ph/0610118 · doi:10.1093/pasj/59.sp1.S113
Abstract
We have developed a framework for the Monte-Carlo simulation of the X-Ray Telescopes (XRT) and the X-ray Imaging Spectrometers (XIS) onboard Suzaku, mainly for the scientific analysis of spatially and spectroscopically complex celestial sources. A photon-by-photon instrumental simulator is built on the ANL platform, which has been successfully used in ASCA data analysis. The simulator has a modular structure, in which the XRT simulation is based on a ray-tracing library, while the XIS simulation utilizes a spectral "Redistribution Matrix File" (RMF), generated separately by other tools. Instrumental characteristics and calibration results, e.g., XRT geometry, reflectivity, mutual alignments, thermal shield transmission, build-up of the contamination on the XIS optical blocking filters (OBF), are incorporated as completely as possible. Most of this information is available in the form of the FITS (Flexible Image Transport System) files in the standard calibration database (CALDB). This simulator can also be utilized to generate an "Ancillary Response File" (ARF), which describes the XRT response and the amount of OBF contamination. The ARF is dependent on the spatial distribution of the celestial target and the photon accumulation region on the detector, as well as observing conditions such as the observation date and satellite attitude. We describe principles of the simulator and the ARF generator, and demonstrate their performance in comparison with in-flight data.
19 pages with 8 figures, accepted for publication in PASJ Vol 58, Suzaku special issue
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- First Detection of Ar-K Line Emission from the Cygnus Loop
- Investigating the outskirts of Abell 133 with Suzaku and Chandra observations
- Detection of pure warm-hot intergalactic medium emission from a Mpc long filament in the Shapley supercluster using X-ray spectroscopy
- Suzaku and Fermi view of the supernova remnant 3C 396
- Initial state of the recombining plasma in supernova remnant W 28
- Discovery of annular X-ray emission centered on MAXI J1421-613: Dust-scattering X-rays?
- Discovery of Diffuse Hard X-Ray Emission from the Vicinity of PSR J1648-4611 with Suzaku
- Suzaku Observations of the old pulsar wind nebula candidate HESS J1356-645
- Origin of the low-temperature plasma in the Galactic center X-ray emission
- Suzaku Observations of the Supernova Remnant N23 in the Large Magellanic Cloud
- A Possible Supernova Remnant high above the Galactic Disk
- X-ray Eclipse Diagnosis of the Evolving Mass Loss in the Recurrent Nova U Scorpii 2010
- Broadband X-ray Spectral Study of Nuclear Structure in Local Obscured Radio Galaxies
- Multi-epoch X-ray spectral analysis of Centaurus A: revealing new constraints on iron emission line origins
- Exploring Hot Gas at Junctions of Galaxy Filaments with Suzaku
- X-ray Development of the Classical Nova V2672 Ophiuchi with Suzaku
- X-ray study of extended emission around M86 observed with Suzaku
- The New Primary X-ray Component Confirmed in the Seyfert I Galaxy IC4329A
- Suzaku observation of a high entropy cluster Abell 548W
- Suzaku Observation of Diffuse X-Ray Emission from a Southwest Region of the Carina Nebula
- A Search for a Contribution from Axion-Like Particles to the X-Ray Diffuse Background Utilizing the Earth's Magnetic Field
- Matched-filtering Line Search Methods Applied to Suzaku Data
- Spatial Power Spectral Analysis of the Suzaku X-ray Background
- Suzaku and Chandra Observations of CIZA J1700.83144, a Cluster of Galaxies in the Zone of Avoidance
- The Modulating Optical Depth of Photoelectric Absorption Edge with Pulse Phase in Accretion-Powered X-ray Pulsars
- Discovery of an Overlapping Cluster in Abell 1674 Field with Suzaku
- The Supernova Remnant G284.31.8 and Its Relation to the Gamma-ray Binary 1FGL J1018.65856
- Metals in the Intracluster Medium of MS 1512.4+3647 Observed with Suzaku: Implications for the Metal Enrichment History
- The NuSTAR, XMM-Newton, and Suzaku view of A3395 at the intercluster filament interface
- Suzaku Observations of Fe K-shell Lines in the Supernova Remnant W51C and Hard X-ray Sources in the Proximity
- Search for the time evolution of the synchrotron X-ray spectrum of the youngest Galactic supernova remnant G1.9+0.3 using Suzaku
- XMM-Newton and Suzaku Spectroscopic Studies of Unidentified X-ray Sources towards the Galactic Bulge: 1RXS J180556.1343818 and 1RXS J173905.2392615
- Long Term X-Ray Spectral Variation of the Wolf-Rayet Binary WR 102-1 in the Galactic bulge: evidence for wind distortion in the binary