unibion.blogg.se - Generation zero map coordinates

XIS data begin as part of the RPT telemetry downloaded from Suzaku, andĪre converted into a collection of FITS files by the mk1stfits routine at ISAS. Pile-up, timing mode, and others) in chapter 5. Scale of non-SCI data, energy scale of SCI data, contamination, XIS and XIS analysis (the loss of XIS2, the XIS0 anomaly, SCI, energy Users should familiarize themselves with the current issues with the Quite similar to that of ASCA SIS and Chandra ACIS.

Significant improvements since the ASCA SIS, the data reduction is The BIĬhip has an increased quantum efficiency at low ( keV) energies withĪ small decrease at higher energies. ``front-illuminated'' (FI) and one ``back-illuminated'' (BI). The XIS consists of four CCD detectors, three of which are

6.6.4.4 Reducing Run Time for xissimargfgen.

6.6.4.3 Generating ARFs in Sky Coordinates: Caveats.

6.6.4.2 Example: ARF of a Uniformly Extended Source.

6.6.4 Generating ARF Files using Xissimarfgen (or Xisarfgen).

6.6.3 Generating RMF Files using Xisrmfgen.

6.6.2 Combining Spectra and Responses using addascaspec.

6.6.1.2 Building Response Files: The Simple Way (2).

6.6.1.1 Building Response Files: The simple Way (1).

6.6.1 Rebinning XIS Spectra Generating Responses using Xisresp.

6.5.1 Combining 3x3 and 5x5 Editing Mode Data.

6.4 Full XIS Reprocessing and Screening using Aepipeline.

6.3 Energy Scale Reprocessing ( Xispi) and Screening using Xisrepro.

HXD Data Analysis Up: Suzaku ABC Guide Previous: 5.