<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Vogt FPA</dc:creator>
  <dc:creator>Kerber F</dc:creator>
  <dc:creator>Mehner A</dc:creator>
  <dc:creator>Yu S</dc:creator>
  <dc:creator>Pfrommer T</dc:creator>
  <dc:creator>Lo Curto G</dc:creator>
  <dc:creator>Figueira P</dc:creator>
  <dc:creator>Parraguez D</dc:creator>
  <dc:creator>Pepe FA</dc:creator>
  <dc:creator>Mégevand D</dc:creator>
  <dc:creator>Riva M</dc:creator>
  <dc:creator>Di Marcantonio P</dc:creator>
  <dc:creator>Lovis C</dc:creator>
  <dc:creator>Amate M</dc:creator>
  <dc:creator>Molaro P</dc:creator>
  <dc:creator>Cabral A</dc:creator>
  <dc:creator>Osorio MRZ</dc:creator>
  <dc:date>2019</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">Raman scattering enables unforeseen uses for the laser guide-star system of the Very Large Telescope. Here, we present the observation of one up-link sodium laser beam acquired with the ESPRESSO spectrograph at a resolution λ/Δλ∼140 000. In 900 s on source, we detect the pure rotational Raman lines of ^{16}O_{2}, ^{14}N_{2}, and ^{14}N^{15}N (tentatively) up to rotational quantum numbers J of 27, 24, and 9, respectively. We detect the ^{16}O_{2} fine-structure lines induced by the interaction of the electronic spin S and end-over-end rotational angular momentum N in the electronic ground state of this molecule up to N=9. The same spectrum also reveals the ν_{1←0} rotational-vibrational Q-branch for ^{16}O_{2} and ^{14}N_{2}. These observations demonstrate the potential of using laser guide-star systems as accurate calibration sources for characterizing new astronomical spectrographs.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://sonar.ch/global/documents/46774</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevLett.123.061101</dc:relation>
  <dc:relation>info:eu-repo/semantics/altIdentifier/pmid/31491188</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:source>Physical review letters. - 2019</dc:source>
  <dc:subject xmlns:ns1="xml" ns1:lang="en">General Physics and Astronomy</dc:subject>
  <dc:title xmlns:ns2="xml" ns2:lang="en">Rotational and Rotational-Vibrational Raman Spectroscopy of Air to Characterize Astronomical Spectrographs.</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>
