Investigation of unidentified lines in optical cometary spectra
Blond Hanten, Elsa
Promotor(s) : Jehin, Emmanuel
Date of defense : 5-Sep-2024/6-Sep-2024 • Permalink : http://hdl.handle.net/2268.2/21661
Details
Title : | Investigation of unidentified lines in optical cometary spectra |
Translated title : | [fr] Etude des raies non identifiées dans les spectres optiques de comètes |
Author : | Blond Hanten, Elsa |
Date of defense : | 5-Sep-2024/6-Sep-2024 |
Advisor(s) : | Jehin, Emmanuel |
Committee's member(s) : | Hutsemekers, Damien
Grodent, Denis de Keyser, Johan |
Language : | English |
Number of pages : | 103 |
Keywords : | [en] comet [en] cometary atlas [en] spectrum [en] fluorescence [en] UVES |
Discipline(s) : | Physical, chemical, mathematical & earth Sciences > Space science, astronomy & astrophysics |
Target public : | Researchers Professionals of domain Student |
Institution(s) : | Université de Liège, Liège, Belgique |
Degree: | Master en sciences spatiales, à finalité approfondie |
Faculty: | Master thesis of the Faculté des Sciences |
Abstract
[en] The first objective of this thesis focuses on enhancing the Atlas of cometary lines developed
by Hardy and the ULiège COMETA team in 2022. This Atlas is based on the spectra of
comets C/2002 T7 (LINEAR), C/2016 R2 (PANSTARRS), C/2002 X5 (Kudo-Fujikawa), and
8P/Tuttle obtained by the ULiège team using the high-resolution Ultraviolet and Visual Echelle
Spectrograph (UVES). The use of spectra that are centred and offset in the tail direction allows
the identification of new lines, especially ionic ones. A total of 579 new lines have been identified
in the spectra, among which 57 were previously unidentified lines in the Atlas. The remaining 522
lines are new lines that had not previously been detected in the version of the Atlas developed by
Hardy. The second objective of the thesis focuses on developing a fluorescence model of imidogen (NH). We describe how the model was set up, and then present the results obtained from the model. The thesis ends with numerous perspectives on continuing the identification of new lines using different comparison techniques.
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