About the atomic and molecular databases in the planetary community — A contribution in the Laboratory Astrophysics Data WG IAU 2022 GA session. (arXiv:2302.05452v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Rengel_M/0/1/0/all/0/1">M. Rengel</a>

This paper corresponds to an invited oral contribution to the session 5A
organised by the IAU inter-commission B2-B5 working group (WG) “Laboratory
Astrophysics Data Compilation, Validation and Standardization: from the
Laboratory to FAIR usage in the Astronomical Community” at the IAU 2022 General
Assembly (GA). This WG provides a platform where to discuss the Findability,
Accessibility,Interoperability, Reuse (FAIR) usage of laboratory Atomic and
Molecular (A&M) data in astronomy and astrophysics.

A&M data play a key role in the understanding of the physics and chemistry of
processes in several research topics, including planetary science and
interdisciplinary research in particular the atmospheres of planets and
planetary explorations, etc. Databases, compilation of spectroscopic
parameters, and facility tools are used by computer codes to interpret
spectroscopic observations and simulate them. In this talk I presented existing
A&M databases of interest to the planetary community focusing on access,
organisation, infrastructures, limitations and issues, etc.

This paper corresponds to an invited oral contribution to the session 5A
organised by the IAU inter-commission B2-B5 working group (WG) “Laboratory
Astrophysics Data Compilation, Validation and Standardization: from the
Laboratory to FAIR usage in the Astronomical Community” at the IAU 2022 General
Assembly (GA). This WG provides a platform where to discuss the Findability,
Accessibility,Interoperability, Reuse (FAIR) usage of laboratory Atomic and
Molecular (A&M) data in astronomy and astrophysics.

A&M data play a key role in the understanding of the physics and chemistry of
processes in several research topics, including planetary science and
interdisciplinary research in particular the atmospheres of planets and
planetary explorations, etc. Databases, compilation of spectroscopic
parameters, and facility tools are used by computer codes to interpret
spectroscopic observations and simulate them. In this talk I presented existing
A&M databases of interest to the planetary community focusing on access,
organisation, infrastructures, limitations and issues, etc.

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