Extended analysis of the high resolution FTIR spectrum of 32S16O2 in the region of the ν2 band: Line positions, strengths, and pressure broadening widths

2018 ◽  
Vol 210 ◽  
pp. 141-155 ◽  
Author(s):  
O.N. Ulenikov ◽  
E.S. Bekhtereva ◽  
O.V. Gromova ◽  
M. Quack ◽  
G.Ch. Mellau ◽  
...  
Keyword(s):  
High Resolution ◽  
Ftir Spectrum ◽  
Pressure Broadening ◽  
Extended Analysis ◽  
Line Positions

Re-analysis of the high resolution FTIR spectrum of C2H2D2-cis in the region of 1280–1400cm−1

2016 ◽  
Vol 170 ◽  
pp. 69-82 ◽  
Author(s):  
O.N. Ulenikov ◽  
O.V. Gromova ◽  
E.S. Bekhtereva ◽  
I.A. Konov ◽  
Yu.V. Chertavskikh ◽  
...  
Keyword(s):  
High Resolution ◽  
Ftir Spectrum

Extended analysis of the ν3 band of HD32S: Line positions, energies, and line strengths

2019 ◽  
Vol 230 ◽  
pp. 131-141 ◽  
Author(s):  
O.N. Ulenikov ◽  
E.S. Bekhtereva ◽  
O.V. Gromova ◽  
N.I. Raspopova ◽  
C. Sydow ◽  
...  
Keyword(s):  
Extended Analysis ◽  
Line Positions ◽  
Line Strengths

scholarly journals Molecular cross-sections for high-resolution spectroscopy of super-Earths, warm Neptunes, and hot Jupiters

2020 ◽  
Vol 495 (1) ◽  
pp. 224-237 ◽  
Author(s):  
Siddharth Gandhi ◽  
Matteo Brogi ◽  
Sergei N Yurchenko ◽  
Jonathan Tennyson ◽  
Phillip A Coles ◽  
...  
Keyword(s):  
High Resolution ◽  
Cross Sections ◽  
Cross Correlation ◽  
High Resolution Spectroscopy ◽  
High Signal ◽  
Pressure Broadening ◽  
Spectral Signatures ◽  
Hot Jupiters ◽  
Wide Range ◽  
Infrared Spectral

ABSTRACT High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of hot Jupiters. Key to such detections is accurately and precisely modelled spectra for cross-correlation against the R ≳ 20 000 observations. There is a need for the latest generation of opacities which form the basis for high signal-to-noise detections using such spectra. In this study we present and make publicly available cross-sections for six molecular species, H2O, CO, HCN, CH4, NH3, and CO2 using the latest line lists most suitable for low- and high-resolution spectroscopy. We focus on the infrared (0.95–5 μm) and between 500 and 1500 K where these species have strong spectral signatures. We generate these cross-sections on a grid of pressures and temperatures typical for the photospheres of super-Earth, warm Neptunes, and hot Jupiters using the latest H2 and He pressure broadening. We highlight the most prominent infrared spectral features by modelling three representative exoplanets, GJ 1214 b, GJ 3470 b, and HD 189733 b, which encompass a wide range in temperature, mass, and radii. In addition, we verify the line lists for H2O, CO, and HCN with previous high-resolution observations of hot Jupiters. However, we are unable to detect CH4 with our new cross-sections from HRS observations of HD 102195 b. These high-accuracy opacities are critical for atmospheric detections with HRS and will be continually updated as new data become available.

The high-resolution FTIR spectrum of the ν6 band of C2H3D

2010 ◽  
Vol 263 (2) ◽  
pp. 160-165 ◽  
Author(s):  
T.L. Tan ◽  
G.B. Lebron
Keyword(s):  
High Resolution ◽  
Ftir Spectrum

High-Resolution FTIR Spectrum of HSSH in the SH-Stretching Region: The ν5 Band

1994 ◽  
Vol 164 (2) ◽  
pp. 390-394 ◽  
Author(s):  
P. Mittler ◽  
K.M.T. Yamada ◽  
G. Winnewisser ◽  
M. Birk
Keyword(s):  
High Resolution ◽  
Ftir Spectrum

High-Resolution FTIR Spectrum of Vinyl Fluoride: Rovibrational Analysis of the Torsion Mode at 712 cm−1

1995 ◽  
Vol 171 (2) ◽  
pp. 504-512 ◽  
Author(s):  
A. Gambi ◽  
A. Delorenzi ◽  
S. Giorgianni ◽  
P. Stoppa
Keyword(s):  
High Resolution ◽  
Ftir Spectrum ◽  
Vinyl Fluoride ◽  
Torsion Mode

High-Resolution FTIR Spectrum of CF2CH2 near 3060 cm−1: Rovibrational Analysis of the Methylene Symmetrical Stretching

1993 ◽  
Vol 160 (2) ◽  
pp. 446-455 ◽  
Author(s):  
A. Delorenzi ◽  
S. Giorgianni ◽  
A. Gambi ◽  
R. Visinoni ◽  
S. Ghersetti
Keyword(s):  
High Resolution ◽  
Ftir Spectrum
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