000607161 001__ 607161
000607161 005__ 20250404221613.0
000607161 0247_ $$2URN$$aurn:nbn:de:gbv:8:3-2024-00362-8
000607161 0247_ $$2datacite_doi$$a10.3204/PUBDB-2024-01804
000607161 037__ $$aPUBDB-2024-01804
000607161 041__ $$aEnglish
000607161 1001_ $$0P:(DE-H253)PIP1089725$$aBatra, Gayatri$$b0$$eCorresponding author$$gfemale
000607161 245__ $$aInvestigating molecules of astrochemical interest using rotational and infrared spectroscopy$$f2019-08-15 - 2024-01-25
000607161 260__ $$c2024
000607161 300__ $$a200
000607161 3367_ $$2DataCite$$aOutput Types/Dissertation
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000607161 3367_ $$02$$2EndNote$$aThesis
000607161 3367_ $$0PUB:(DE-HGF)11$$2PUB:(DE-HGF)$$aDissertation / PhD Thesis$$bphd$$mphd$$s1743761649_121578
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000607161 502__ $$aDissertation, Christian-Albrechts-Universität zu Kiel, 2024$$bDissertation$$cChristian-Albrechts-Universität zu Kiel$$d2024$$o2024-01-25
000607161 520__ $$aThe objective of this thesis is to investigate molecules of astronomical interest with a multi-spectroscopic approach to allow the chemical inventory of interstellar molecules to be better determined. This will also contribute towards a more comprehensive understanding of their formation mechanisms in the Interstellar medium. The major part of this thesis was done utilizing rotational spectroscopy. Analysis of rotational spectra delivers line lists and rotational constants for the molecules studied. Application of these to the observational data sets allows astronomers to search for the molecules in interstellar space. It is a very structure-sensitive technique that is not only conformer-specific but also isotopologue-specific. The different frequency ranges covered by the rotational spectrometers overlap with various radio telescopes. For example, the low-frequency data overlaps with facilities such as the Jansky Very Large Array and the Effelsberg 100m Radio Telescope. The W-band spectrometer overlaps with the Band 3 operating regime (86-114 GHz) of the Atacama Large Millimeter/submillimeter Array. This makes the laboratory data directly applicable to radio astronomy. In addition to rotational spectroscopy, we also utilized IR spectroscopic techniques like Infrared reflection absorption spectroscopy and IR-UV ion dip spectroscopy. With the commencement of the James Webb Space Telescope, the vibrational spectroscopy data can be used to search the vibrational features of the molecules of interest in the Interstellar medium.
000607161 536__ $$0G:(DE-HGF)POF4-631$$a631 - Matter – Dynamics, Mechanisms and Control (POF4-631)$$cPOF4-631$$fPOF IV$$x0
000607161 536__ $$0G:(DE-HGF)2015_IFV-VH-GS-500$$aPHGS, VH-GS-500 - PIER Helmholtz Graduate School (2015_IFV-VH-GS-500)$$c2015_IFV-VH-GS-500$$x1
000607161 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000607161 7001_ $$0P:(DE-H253)PIP1013514$$aSchnell, Melanie$$b1$$eThesis advisor$$udesy
000607161 7001_ $$0P:(DE-HGF)0$$aFriedrichs, Gernot$$b2$$eThesis advisor
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000607161 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1013514$$aDeutsches Elektronen-Synchrotron$$b1$$kDESY
000607161 9101_ $$0I:(DE-H253)_CFEL-20120731$$6P:(DE-H253)PIP1013514$$aCentre for Free-Electron Laser Science$$b1$$kCFEL
000607161 9131_ $$0G:(DE-HGF)POF4-631$$1G:(DE-HGF)POF4-630$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lVon Materie zu Materialien und Leben$$vMatter – Dynamics, Mechanisms and Control$$x0
000607161 9141_ $$y2024
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000607161 9201_ $$0I:(DE-H253)FS-SMP-20171124$$kFS-SMP$$lSpectroscopy of molecular processes$$x0
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