CSST On-Orbit Calibration Strategy and Data System

PO
Not scheduled
15m
Wichernhaus

Wichernhaus

Board: A207
poster presentation Automation of data pipeline and workflows Poster

Speaker

Juanjuan Ren (National Astronomical Observatories, Chinese Academy of Sciences)

Description

The China Space Station Survey Telescope (CSST) is a next-generation Stage-IV sky survey telescope, which is scheduled to be launched in 2027. It is equipped with five scientific instruments, i.e. Multi-band Imaging and Slitless Spectroscopy Survey Camera (SC), Multi-Channel Imager (MCI), Integral Field Spectrograph (IFS), Cool Planet Imaging Coronagraph (CPI-C), and THz Spectrometer (TS). Due to the large field of view, simultaneous multi-band photometric imaging and slitless spectroscopic surveys, various scientific objectives, and multiple scientific instruments, the on-orbit calibration strategy of CSST is complicated and challenging. The CSST On-Orbit Calibration Team mainly focused on the research of on-orbit calibration observation strategy, the reduction of observational calibration data (i.e. the development of toolkits to produce the calibration reference files), and the management of the various calibration data products, with the aim to support the automation of scientific data processing pipeline. Here we mainly introduce the on-orbit calibration strategy that are currently devised for CSST and the corresponding calibration data system.

Affiliation of the submitter National Astronomical Observatories, Chinese Academy of Sciences
Attendance in-person

Primary author

Juanjuan Ren (National Astronomical Observatories, Chinese Academy of Sciences)

Co-authors

Bingli Niu (Nanjing Institute of Astronomical Optics & Technology ,National Astronomical Observatories ,CAS) Bowei Zhao (National Astronomical Observatories, Chinese Academy of Sciences) Chenxiaoji Ling (National Astronomical Observatories, Chinese Academy of Sciences) Chun Xu (Shanghai Astronomical Observatory, Chinese Academy of Sciences) Jundan Nie (National Astronomical Observatories, Chinese Academy of Sciences) Li Shao (National Astronomical Observatories, Chinese Academy of Sciences) Peng Wei (National Astronomical Observatories, Chinese Academy of Sciences) Rui Wang (National Astronomical Observatories, Chinese Academy of Sciences) Shoulin Wei (Kunming University of Science and Technology) Siyuan Tan (Purple Mountain Observatory, CAS) Su Yao (National Astronomical Observatories, Chinese Academy of Sciences) Xiyan Peng (Shanghai Astronomical Observatory, Chinese Academy of Sciences) Zhimin Zhou (National Astronomical Observatories, Chinese Academy of Sciences)

Presentation materials