Method for tilt correction of calibration lines in high resolution spectra
Method for tilt correction of calibration lines in high resolution spectra
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Technological advancement has led to improvement in the design capabilities of astronomical spectrographs, allowing for high precision spectroscopy, thereby expanding the realms of observational astronomy. High-resolution spectrographs use Echelle grating that operates in higher orders, giving more detailed spectra. Often, curvature and tilted line...
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Full title
Method for tilt correction of calibration lines in high resolution spectra
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TN_cdi_proquest_journals_2591825264
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2591825264
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2111.00751
