Dataset
An exhaustive description of the APIS service can be found in this article, Arxiv pre-print. A brief description of the available observations is reminded below.
APIS/HST data collection
The APIS primary database consists of an internal base of HST FUV planetary auroral observations acquired by the STIS, ACS/SBC (and WFPC2) instruments since 1997. These include >12500 individual (...)
Read more »APIS/Cassini/UVIS data collection
The APIS service queries an internal internal base of Cassini/UVIS FUV auroral observations of Saturn, made of 8000 individual slewing of both the northern and southern auroral regions obtained (...)
Read more »Hisaki database
Since 2017, the APIS search interface also queries external Hisaki EUV spectro-imaging observations of solar system planets acquired with the EXCEED instrument. These now include >1600 individual (...)
Read more »Acknowledgements
Acknowledgements
The path from the original idea to observe a target to the value-added data delivered by APIS is long and complex, and involves a significant work from many persons and services (...)