2024MNRAS.527.6675B


Query : 2024MNRAS.527.6675B

2024MNRAS.527.6675B - Mon. Not. R. Astron. Soc., 527, 6675-6690 (2024/January-3)

ExoMol line lists - LVI. The SO line list, MARVEL analysis of experimental transition data and refinement of the spectroscopic model.

BRADY R.P., YURCHENKO S.N., TENNYSON J. and KIM G.-S.

Abstract (from CDS):

A semi-empirical IR/Vis line list, SOLIS, for the sulphur monoxide molecule 32S16O is presented. SOLIS includes accurate empirical rovibrational energy levels, uncertainties, lifetimes, quantum number assignments, and transition probabilities in the form of Einstein A coefficients covering the $X\, {}^{3}\Sigma ^{-}$$, a\, {}^{1}\Delta , b\, {}^{1}\Sigma ^{+}, A\, {}^{3}\Pi , B\, {}^{3}\Sigma ^{-}, A^{\prime \prime }\, {}^{3}\Sigma ^{+}, A^{\prime }\, {}^{3}\Delta$, and $e\, {}^{1}\Pi$ systems and wavenumber range up to 43 303.5 cm–1 (≥230.93 nm) with J ≤ 69. SOLIS has been computed by solving the rovibronic Schrödinger equation for diatomics using the general purpose variational code DUO and starting from a published ab initio spectroscopic model of SO (including potential energy curves, coupling curves, (transition) dipole moment curves) which is refined to experimental data. To this end, a database of 50 106 experimental transitions, 48 972 being non-redundant, has been compiled through the analysis of 29 experimental sources, and a self-consistent network of 8558 rovibronic energy levels for the X, a, b, A, B, and C electronic states has been generated with the MARVEL algorithm covering rotational and vibrational quantum numbers J ≤ 69 and v ≤ 30 and energies up to 52 350.40 cm–1. No observed transitions connect to the $B\, {}^{3}\Sigma ^{-}$(v = 0) state which is required to model perturbations correctly, so we leave fitting the $B\, {}^3\Sigma ^-$ and $C\, {}^3\Pi$ state UV model to a future project. The SO line list is available at ExoMol from www.exomol.com.

Abstract Copyright: © 2023 The Author(s) The Author(s) 2022. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): molecular data - planets and satellites: atmospheres - stars: atmospheres - exoplanets

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 WASP-39b Pl 14 29 18.4151689656 -03 26 40.204480380           ~ 345 1

Query : 2024MNRAS.527.6675B

Basic data :
WASP-39b -- Extra-solar Planet
Other object types:
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Pl (), Pl? (WASP)
ICRS coord. (ep=J2000) :
14 29 18.4151689656 -03 26 40.204480380 (Optical) [ 0.0134 0.0112 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
14 26 42.3678042295 -03 13 19.810112735 [ 0.0134 0.0112 90 ]
Gal coord. (ep=J2000) :
344.4035836639826 +51.3711104248527 [ 0.0134 0.0112 90 ]
Proper motions mas/yr :
-19.041 0.437 [0.017 0.014 90] A 2020yCat.1350....0G
Parallaxes (mas):
4.6435 [0.0144] A 2020yCat.1350....0G
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NAME-IAU Bocaprins WASP-39b

References (345 between 1850 and 2026) (Total 345)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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