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Journal ArticleDOI

HITEMP, the high-temperature molecular spectroscopic database

TLDR
In this paper, a new molecular spectroscopic database for high-temperature modeling of the spectra of molecules in the gas phase is described, called HITEMP, which is analogous to the HITRAN database but encompasses many more bands and transitions than HitRAN for the absorbers H2O, CO2, CO, NO and OH.
Abstract
A new molecular spectroscopic database for high-temperature modeling of the spectra of molecules in the gas phase is described. This database, called HITEMP, is analogous to the HITRAN database but encompasses many more bands and transitions than HITRAN for the absorbers H2O, CO2, CO, NO, and OH. HITEMP provides users with a powerful tool for a great many applications: astrophysics, planetary and stellar atmospheres, industrial processes, surveillance, non-local thermodynamic equilibrium problems, and investigating molecular interactions, to name a few. The sources and implementation of the spectroscopic parameters incorporated into HITEMP are discussed.

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Citations
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Journal ArticleDOI

Impact of Clouds and Hazes on the Simulated JWST Transmission Spectra of Habitable Zone Planets in the TRAPPIST-1 System

TL;DR: In this paper, a 3D General Circulation Model (GCM) simulation with the LMD Generic model supplemented by 1-D photochemistry simulations at the terminator with the Atmos model was performed to simulate several possible atmospheres for TRAPPIST-1e, 1f and 1g: modern Earth, Archean Earth, and CO2-rich atmospheres.
Journal ArticleDOI

Retrieval of exoplanet emission spectra with HyDRA

TL;DR: HyDRA as discussed by the authors uses the standard architecture of a parametric atmospheric model coupled with Bayesian statistical inference using the Nested Sampling algorithm to detect H2O and a combined CO/CO2 at 8-sigma significance.
Journal ArticleDOI

Aeronomical constraints to the minimum mass and maximum radius of hot low-mass planets

TL;DR: In this paper, the authors generalize the Jeans escape parameter taking hydrodynamic and Roche lobe effects into account, and find that the escape rate of hot (i.e. T eq ⪆ 1000 K) low-mass (M pl ⪅ 5 M ⊕ ) planets with high-mass high-energy stellar radiation, when they orbit M-dwarfs, lies in the boiling-off regime.
Journal ArticleDOI

A New Approach to Analyzing Hst Spatial Scans: the Transmission Spectrum of HD 209458 b

TL;DR: In this paper, the authors present a new pipeline for analyzing the data obtained with the spatial scanning technique, starting from the raw data provided by the instrument, taking into account the geometric distortions of the instrument and the impact of which may become important when they are combined with the scanning process.
Journal ArticleDOI

Exoplanet atmospheres with GIANO. I. Water in the transmission spectrum of HD 189733b

TL;DR: In this article, a series of spectra of the exoplanet HD 189733 b taken at the Telescopio Nazionale Galileo with the near-infrared spectrograph GIANO during two transits of the planet was used to demonstrate the concept of using high-resolution spectroscopy to investigate the composition, structure, and circulation patterns of ex-oplanet atmospheres.
References
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Journal ArticleDOI

The HITRAN 2008 molecular spectroscopic database

TL;DR: The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, added line-shape formalisms, and validity, and molecules, isotopologues, and perturbing gases have been added that address the issues of atmospheres beyond the Earth.
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The hitran molecular database: editions of 1991 and 1992

TL;DR: The HITRAN molecular absorption database as mentioned in this paper contains line parameters for 31 species and their isotopomers that are significant for terrestrial atmospheric studies, including chlorofluorocarbons and other molecular species that are not amenable to line-by-line representation.
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The determination of an accurate isotope dependent potential energy surface for water from extensive ab initio calculations and experimental data

TL;DR: In this article, a high quality ab initio potential energy surface (PES) and dipole moment function (DPM) for water has been determined and an adjusted PES is empirically adjusted to improve the agreement between the computed line positions and those from the HITRAN 92 data base with J⩽5 for H216O.
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The HITRAN database: 1986 edition.

TL;DR: A description and summary of the latest edition of the AFGL HITRAN molecular absorption parameters database are presented and a FORTRAN program is now furnished to allow rapid access to the molecular transitions and for the creation of customized output.
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A high-accuracy computed water line list

TL;DR: The most complete water line list in existence, comprising over 500 million transitions (65 per cent more than any other list) and also the most accurate (over 90 per cent of all known experimental energy levels are within 0.3 cm −1 of the BT2 values) is presented in this article.
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