Difference between revisions of "Publication Plan"
(→Detector related) |
|||
| (4 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
| − | + | == Instrumentation papers == | |
| − | ==Calibration == | + | === Calibration === |
* 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 === |
| − | == Imaging == | + | === Imaging === |
| + | * Coarse flare locator? | ||
| − | == Software and data analysis == | + | === Software and data analysis === |
* 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.
