Difference between revisions of "Publication Plan"
(→Detector related) |
|||
(3 intermediate revisions by the same user not shown) | |||
Line 1: | Line 1: | ||
− | == Instrumentation | + | == Instrumentation papers == |
=== Calibration === | === Calibration === | ||
Line 5: | Line 5: | ||
* Hualin Xiao, STIX timing calibration using GRBs and localization of GRBs using STIX data | * Hualin Xiao, STIX timing calibration using GRBs and localization of GRBs using STIX data | ||
+ | * STIX energy calibration, who takes the lead? | ||
=== Crab === | === Crab === | ||
Line 10: | Line 11: | ||
=== Imaging === | === Imaging === | ||
+ | * Coarse flare locator? | ||
=== Software and data analysis === | === Software and data analysis === | ||
Line 15: | Line 17: | ||
* Hualin Xiao, STIX data processing pipeline and STIX data center | * Hualin Xiao, STIX data processing pipeline and STIX data center | ||
− | === | + | === Others === |
− | * Hualin Xiao, STIX | + | * Hualin Xiao, Responses of STIX to solar energetic charge particles. It will discuss what energies and what incoming angles of SEPs can be detected by STIX. |
Latest revision as of 08:12, 20 July 2021
Contents
1 Instrumentation papers
1.1 Calibration
- Hualin Xiao, STIX timing calibration using GRBs and localization of GRBs using STIX data
- STIX energy calibration, who takes the lead?
1.2 Crab
1.3 Imaging
- Coarse flare locator?
1.4 Software and data analysis
- Hualin Xiao, STIX data processing pipeline and STIX data center
1.5 Others
- Hualin Xiao, Responses of STIX to solar energetic charge particles. It will discuss what energies and what incoming angles of SEPs can be detected by STIX.