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dc.contributor.authorFerber, R.
dc.contributor.authorEr, Alev
dc.contributor.authorGuzelcimen, Feyza
dc.contributor.authorOzturk, İpek
dc.contributor.authorBasar, Gönül
dc.contributor.authorTamanis, M.
dc.contributor.authorKroeger, S.
dc.date.accessioned2021-03-03T11:49:31Z
dc.date.available2021-03-03T11:49:31Z
dc.date.issued2015
dc.identifier.citationEr A., Guzelcimen F., Basar G., Ozturk İ., Tamanis M., Ferber R., Kroeger S., "HIGH-RESOLUTION FOURIER TRANSFORM SPECTROSCOPY OF Nb I IN THE NEAR-INFRARED", ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, cilt.221, sa.1, 2015
dc.identifier.issn0067-0049
dc.identifier.othervv_1032021
dc.identifier.otherav_2a331c24-6e66-426e-b461-360bcceda880
dc.identifier.urihttp://hdl.handle.net/20.500.12627/33161
dc.identifier.urihttps://doi.org/10.1088/0067-0049/221/1/14
dc.description.abstractIn this study, a Fourier Transform spectrum of Niobium (Nb) is investigated in the near-infrared spectral range from 6000 to 12,000 cm(-1) (830-1660 nm). The Nb spectrum is produced using a hollow cathode discharge lamp in an argon atmosphere. Both Nb and Ar spectral lines are visible in the spectrum. A total of 110 spectral lines are assigned to the element Nb. Of these lines, 90 could be classified as transitions between known levels of atomic Nb. From these classified Nb I transitions, 27 have not been listed in literature previously. Additionally, 8 lines are classified for the first time.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleHIGH-RESOLUTION FOURIER TRANSFORM SPECTROSCOPY OF Nb I IN THE NEAR-INFRARED
dc.typeMakale
dc.relation.journalASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
dc.contributor.departmentUniversity of Latvia , ,
dc.identifier.volume221
dc.identifier.issue1
dc.contributor.firstauthorID226009


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