Marvel analysis of the measured high-resolution rovibrational spectra of H2S. (arXiv:1812.10503v1 [astro-ph.EP])
<a href="http://arxiv.org/find/astro-ph/1/au:+Chubb_K/0/1/0/all/0/1">Katy L. Chubb</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Naumenko_O/0/1/0/all/0/1">Olga Naumenko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Keely_S/0/1/0/all/0/1">Stefan Keely</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bartolotto_S/0/1/0/all/0/1">Sebestiano Bartolotto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Macdonald_S/0/1/0/all/0/1">Skye Macdonald</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mukhtar_M/0/1/0/all/0/1">Mahmoud Mukhtar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Grachov_A/0/1/0/all/0/1">Andrey Grachov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+White_J/0/1/0/all/0/1">Joe White</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coleman_E/0/1/0/all/0/1">Eden Coleman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_A/0/1/0/all/0/1">Anwen Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fazliev_A/0/1/0/all/0/1">Alexander Z. Fazliev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Polovtseva_E/0/1/0/all/0/1">Elena R. Polovtseva</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Horneman_V/0/1/0/all/0/1">Veli-Matti Horneman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Campargue_A/0/1/0/all/0/1">Alain Campargue</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Furtenbacher_T/0/1/0/all/0/1">Tibor Furtenbacher</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Csaszar_A/0/1/0/all/0/1">Attila G. Cs&#xe1;sz&#xe1;r</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yurchenko_S/0/1/0/all/0/1">Sergei N. Yurchenko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tennyson_J/0/1/0/all/0/1">Jonathan Tennyson</a>

44325 measured and assigned transitions of H$_2^{32}$S, the parent
isotopologue of the hydrogen sulfide molecule, are collated from 33
publications into a single database and reviewed critically. Based on this
information, rotation-vibration energy levels are determined for the ground
electronic state using the Measured Active Rotational-Vibrational Energy Levels
(MARVEL) technique. The ortho and para principal components of the measured
spectroscopic network of H$_2^{32}$S are considered separately. The verified
set of 25293 ortho- and 18778 para- H$_2^{32}$S transitions determine 3969
ortho and 3467 para energy levels. The Marvel results are compared with
alternative data compilations, including a theoretical variational linelist.

44325 measured and assigned transitions of H$_2^{32}$S, the parent
isotopologue of the hydrogen sulfide molecule, are collated from 33
publications into a single database and reviewed critically. Based on this
information, rotation-vibration energy levels are determined for the ground
electronic state using the Measured Active Rotational-Vibrational Energy Levels
(MARVEL) technique. The ortho and para principal components of the measured
spectroscopic network of H$_2^{32}$S are considered separately. The verified
set of 25293 ortho- and 18778 para- H$_2^{32}$S transitions determine 3969
ortho and 3467 para energy levels. The Marvel results are compared with
alternative data compilations, including a theoretical variational linelist.

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