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 images and spectra, obtained with different instrumental configurations (filters, slits, gratings), for each of which is derived a set of higher level data.
Reference : Title : APIS/HST data collection (2021) Abstract : The APIS/HST data collection is composed of 3 (…)
The APIS service provides access to UV spectro-imaging auroral observations of solar system planets and moons.
Most recent articles
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APIS/HST data collection
2 June 2019, by Laurent LAMY -
APIS/Cassini/UVIS data collection
2 June 2019, by Laurent LAMYAPIS/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 between 2004 and 2017.
Reference : Title : APIS/Cassini/UVIS data collection (2021) Abstract : The APIS/Cassini/UVIS data collection has been built from original Cassini/UVIS spectro-imaging auroral observations of Saturn in the Extreme- and Far-Ultraviolet (…) -
Hisaki database
2 June 2019, by Laurent LAMYHisaki 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 daily observations obtained with different instrumental configurations (slits, gratings) by Hisaki during its nominal mission which extended from 2013 to 2023. The provided level 1 data consist of 2D spectra acquired during one day of observation with 1-min resolution. For graphic (…) -
VO tools
3 July 2018, by Florence HENRYCassis
Aladin
The interactive use of VO tools ’Aladin’ or ’Cassis’ (enabled by clicking on the links below each quicklook) requires the user to have launched the relevant software before. The data are then transmitted automatically to the chosen tool through the SAMP protocol. -
Cassis is not launched
3 July 2018, by Florence HENRYYou have to launch Cassis. See the help section for more details.
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Team
30 June 2015, by Laurent LAMYTeam
The APIS service is developed at LESIA, Observatoire de Paris, CNRS. The database is archived and maintained at Paris Astronomical Data Centre. NameStatusInstituteRole L. Lamy Assistant astronomer LESIA-Observatoire de Paris Scientific responsible R. Prangé Research Director LESIA-Observatoire de Paris Scientific expertise F. Henry Research engineer LESIA-Observatoire de Paris Project manager R. Romagnan Research engineer LESIA-Observatoire de Paris Query of external VO (…) -
Graphics
16 July 2013, by Laurent LAMYGraphics :
Animated version :
https://cdn.esahubble.org/archives/... -
Help for VO tools
4 July 2013, by Florence HENRYImages can be interactively read with Aladin. First option : you can directly use Aladin online with your web browser (applet mode). In this case, simply click on the link "view with Aladin" below the image of interest. The relevant applet will be launched automatically. Second option : you possess the latest version of Aladin on your computer (if not, you can download it). In this case, launch the application first, and then click on the link "view with Aladin" below the image of interest. (…)
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Specview is not launched
4 July 2013, by Florence HENRYYou have to launch Specview. See the help section for more details.
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Aladin is not launched
4 July 2013, by Florence HENRYYou have to launch Aladin. See the help section for more details.