Highlights

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EP-FXT 数据分析软件发布v1.20版本

 

2025年5月30日,EP-FXT团队发布FXT数据分析软件和标定数据库v1.20版本。此版本在v1.10版本基础上,根据FXT在轨标定观测优化了数据分析软件,更新了标定数据库。下载链接:http://epfxt.ihep.ac.cn/analysis。EP-FXT团队将根据FXT标定进展持续更新数据分析软件和标定数据库。

 

版本1.20更新内容:

数据分析软件:

1. 增加了仪器本底估计模块 (fxtbkggen);

2. 增加了PSF图像提取模块 (fxtpsfgen);

3. 更新了曝光图生成模块 (fxtexpogen),提升了运行速度,增加了边缘效应修正功能;

4. 更新了pipeline模块 (fxtchain),增加了fsa数据处理功能.

 

标定数据库:

1. 更新E-C关系;

2. 更新能量分辨率;

3. 更新辅助响应文件ARF,本版本适用能量范围(0.5-10 keV)

 

Bug修复:

1. 调整ARF文件中能量的精度与RMF文件一致;

2. 补充RMF文件关键字TLMIN4=0和TLMAX4=1023.

 

 

EP-FXT Data Analysis Software Releases New Version 1.20

 

On May 30, 2025, the EP-FXT team released version 1.20 for the data analysis software (FXTDAS) and the associated calibration database (CalDB). This release includes significant improvements to FXTDAS and updates to the CalDB, based on the latest in-orbit calibration of FXT. Compared to v1.10, version 1.20 delivers improvements in data processing performance, offers additional modules and functionalities, and incorporates more accurate calibration. The software package and calibration files are available for download at: http://epfxt.ihep.ac.cn/analysis.  

 

Version 1.20 Updates:

Data Analysis Software:

1. Added an instrumental background estimate module (fxtbkggen);

2. Added PSF image and EEF estimate modules (fxtpsfgen and fxteefgen);

3. Updated the exposure map module (fxtexpogen): improved computation speed and added an edge mask function;

4. Update the pipeline module (fxtchain) to support both ‘evt’ data and ‘fsaevt’ data.

 

Calibration Database:

1. Updated the E-C relationship;

2. Updated the energy resolution;

3. Updated the Ancillary Response File (ARF), suitable for the energy band of 0.5-10 keV in this version.

 

Bug Fixes:

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

2. Added keywords TLMIN4=0 and TLMAX4=1023 to RMF file.

 

EP Observation

        Source Name:2RXS J111140.2-224929

 

        RA :167.918

 

        DEC:-22.8248

 

        FXT a/b Mode:ff/ff

 

        FXT a/b Filter: THIN/THIN

 

FXT Notice(“风行天”记)

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Notice_#16_EFT241123-0ABA_20241123:Discovery of a New X-ray Source by EP-FXT

2024-11-25

Notice_#15_EFT241122-0AB1_20241122:Discovery of a New X-ray Source by EP-FXT

2024-11-25

Notice_#14_EFT241115A-0A10_20241117:Discovery of a New X-ray Source by EP-FXT

2024-11-18

News

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04-08

2025

在致密星并合产生的伽马射线暴中发现磁星存在的直接证据

02-26

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“天关”卫星捕捉到罕见的X射线双星系统

EP Mission

The Einstein Probe (EP) is a mission of the Chinese Academy of Sciences (CAS) dedicated to time-domain high-energy astrophysics. Its primary goals are to discover high-energy transients and monitor variable objects. To achieve this, EP employs a very large instantaneous field-of-view (3600 square degrees), along with moderate spatial resolution (FWHM ~5 arcmin) and energy resolution.  Its wide-field imaging capability is achieved by using established technology of novel lobster-eye optics, thereby offering unprecedentedly high sensitivity and large Grasp, which would supersede previous and existing X-ray all-sky monitors. To complement this powerful capability to discover and monitor sources over a wide area, EP also carries a conventional X-ray focusing telescope with a larger effective area to perform follow-up characterization and precise localization of newly-discovered transients. Public transient alerts will be issued rapidly to trigger multi-wavelength follow-up observations from the world-wide community. The satellite has a weight of ~1450 kg and average power of ~1212 W in total. In the normal survey mode, during one orbit of 97 minutes three fields will be observed on the night-side of the sky with a ~20 min pointing each. Over three orbits almost the entire night sky will be sampled, with cadences ranging from several to a few ten revisits per day depending on the sky location. The mission is aimed for launch by the end of 2023 with a nominal lifetime of 3 years (5 years as a goal).

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