FXT Data Center

FXT DAS

The Follow-up X-ray Telescope Data Analysis Software (FXTDAS) is to achieve the EP-FXT data analysis processing and extract scientific products, e.g. energy spectra, images, light curves, ancillary response files (ARF), redistribution matrix files (RMF) and background files.

FXT has three scientific observation modes: the full frame mode (FF), the partial window mode (PW) and the timing mode (TM), and FXTDAS is designed to allow the general users to analyse FXT data observed in these modes.

The software is written in ftools style and are fully compatible with the HEASoft software.

FXT DAS - Latest Version

Version 1.20 Updates:

Data Analysis Software:

1. Added an instrumental background estimation module (fxtbkggen) for extended source analysis.

The estimation is based on the spectrum of cleaned events in frame-store area (FSA).

2. Added PSF image and EEF estimation modules (fxtpsfgen and fxteefgen) for any detector

position (rawX and rawY) and any energy (eV).

3. Optimazed the exposure map calculation method in fxtexpogen. Added the parameter

'edgecovermask' to mark the 20 rows near the readout side as 0 in the exposure map.

Added the parameter 'area_scale' for scaling the effective area.

4. Added support of the analysis of fsaevt data in the pipeline tool (fxtchain).

The spectrum of the cleaned events in FSA can be obtained by running fxtchain with

the parameter set to ‘datatype=fsaevt’.

Calibration Database:

1. Updated the E-C relationship based on Cas A observations.

2. Updated the energy resolution based on Fe55 onboard FXT.

3. Updated the Ancillary Response Files (ARFs), suitable for the energy band of 0.5-10 keV.

The validity period of the contamination effect on ARF has been updated to April 2025.

Bug Fixes:

1. Adjusted the energy precision of ARF file to match that of RMF file.

2. Added key words 'TLMIN4=0' and 'TLMAX4=1023' to RMF file.

All updates in this version have been integrated into fxtchain. We recommend users to use fxtchain (refer to Chapter 6 of the USER GUIDE 1.20) to complete FXT data (both evt and fsaevt) analysis.

You can download the source code of FXTDAS. In addition, the docker image is also provided. If you encounter any installation problem, it is recommended to use the docker version, or please report them on the helpdesk.

*Source code for linux:

EP-FXT software v1.20 source code for linux or IHEPDocs: EP-FXT software v1.20 source code for linux

*Docker image:

When loading a Docker image, use docker load < x.tar.gz for compressed files ending in .tar.gz, and use docker load -i x.tar for uncompressed files ending in .tar.

EP-FXT software v1.20 docker image or IHEPDocs: EP-FXT software v1.20 docker image

FXT DAS - Historical Version

EP-FXT software v1.10

2025/05/29

EP-FXT software v1.05

2024/09/27

FXT CALDB

The Einstein Probe Follow-up X-ray Telescope (EP-FXT) Calibration Database (CALDB) is an essential resource for researchers working with EP-FXT data. The CALDB contains a comprehensive collection of calibration files necessary for accurate data reduction and analysis. These files provide detailed information about the properties and performance of the EP-FXT detectors, mirrors, and other instrument components. The CALDB is organized into a well-defined directory structure, making it easy for users to locate and access the calibration files required for their specific analysis tasks.

Some of the key calibration files included in the EP-FXT CALDB are:

1）Ancillary Response Files (ARF): These files contain information about the effective area of the detectors and mirrors as a function of energy.

2）Response Matrix Files (RMF): These files characterize the energy response of the EP-FXT detectors, accounting for energy dispersion and detector resolution.

3）Point Spread Function (PSF) files: These files describe the spatial distribution of X-ray photons as they are focused by the EP-FXT mirrors.

4）Energy Encircled Fraction (EEF) files: These files provide information on the fraction of energy contained within a given radius for a point source.

5）Telescope Definition (TELDEF) files: These files describe the geometry and alignment of the EP-FXT detectors and mirrors.

6）Vignetting files: These files contain information on the reduction of the telescope's effective area due to off-axis angles.

7）Filter Transmission (FTRANS) files: These files describe the transmission properties of the filters used in EP-FXT.

8）Quantum Efficiency (QE) files: These files provide information on the detectors' sensitivity to incoming photons as a function of energy.

9）Gain and Charge Transfer Inefficiency (GAIN) files: These files contain information about the gain calibration and charge transfer inefficiency of the EP-FXT detectors.

10）Mirror effective area (EFF) files: These files provide data on the reflectivity and efficiency of the EP-FXT mirrors as a function of energy.

11）Background files: These files contain information on the instrumental and astrophysical background components relevant to the EP-FXT observations.

The EP-FXT CALDB plays a crucial role in ensuring that researchers can obtain the most accurate and reliable results from their analysis of EP-FXT data. By providing up-to-date calibration information, the CALDB enables scientists to fully exploit the exceptional capabilities of the Einstein Probe Follow-up X-ray Telescope and contribute to the advancement of our knowledge of the high-energy universe.