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@PHDTHESIS{Batra:607161,
      author       = {Batra, Gayatri},
      othercontributors = {Schnell, Melanie and Friedrichs, Gernot},
      title        = {{I}nvestigating molecules of astrochemical interest using
                      rotational and infrared spectroscopy},
      school       = {Christian-Albrechts-Universität zu Kiel},
      type         = {Dissertation},
      reportid     = {PUBDB-2024-01804},
      pages        = {200},
      year         = {2024},
      note         = {Dissertation, Christian-Albrechts-Universität zu Kiel,
                      2024},
      abstract     = {The 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.},
      cin          = {FS-SMP},
      cid          = {I:(DE-H253)FS-SMP-20171124},
      pnm          = {631 - Matter – Dynamics, Mechanisms and Control
                      (POF4-631) / PHGS, VH-GS-500 - PIER Helmholtz Graduate
                      School $(2015_IFV-VH-GS-500)$},
      pid          = {G:(DE-HGF)POF4-631 / $G:(DE-HGF)2015_IFV-VH-GS-500$},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)11},
      urn          = {urn:nbn:de:gbv:8:3-2024-00362-8},
      doi          = {10.3204/PUBDB-2024-01804},
      url          = {https://bib-pubdb1.desy.de/record/607161},
}