Zn I spectra in the 1300–6500cm−1 range

Civiš, Svatopluk; Ferus, Martin; Chernov, V. E.; Zanozina, E. M.; Juha, L.

doi:10.1016/j.jqsrt.2013.10.017

Cited by 11 publications

(3 citation statements)

References 31 publications

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“…The error estimation of the results of the present work was described recently. 37,38 As mentioned above, no values for the In I ng and nh energy levels are available in the literature. To identify the lines corresponding to these levels, we rst calculated the approximate energies of these states using the Rydberg formula.…”

Section: Resultsmentioning

confidence: 99%

“…This study continues the series of Fourier transform infrared (FTIR) spectroscopic studies of metal atom IR spectra. [30][31][32][33][34][35][36][37][38] Timeresolved FTIR spectroscopy is an experimental technique that was originally developed and used for studying the kinetics of various physical and/or chemical 39 processes occurring in dynamic systems.…”

Section: Time-resolved Ftir Spectrometrymentioning

confidence: 99%

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Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range

Civiš

Kubelík

Ferus

et al. 2014

J. Anal. At. Spectrom.

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Section: Resultsmentioning

confidence: 99%

Section: Time-resolved Ftir Spectrometrymentioning

confidence: 99%

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range

Civiš

Kubelík

Ferus

et al. 2014

J. Anal. At. Spectrom.

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“…These original ideas have re-emerged in the light of new experiments carried out very recently in several studies showing, for example, that the atmosphere of Titan, the largest moon of Saturn, can produce nucleobases in rich HCN-based discharge chemistry . [142,143]. Energetic processes such as lightning also act as a strong abiotic fixation process for the removal of atmospheric N2.…”

Section: Atmospheric Electricitymentioning

confidence: 99%

Ariel – a window to the origin of life on early earth?

et al. 2020

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Is there life beyond Earth? An ideal research program would first ascertain how life on Earth began and then use this as a blueprint for its existence elsewhere. But the origin of life on Earth is still not understood, what then could be the way forward? Upcoming observations of terrestrial exoplanets provide a unique opportunity for answering this fundamental question through the study of other planetary systems. If we are able to see how physical and chemical environments similar to the early Earth evolve we open a window into our own Hadean eon, despite all information from this time being long lost from our planet's geological record. A careful investigation of the chemistry expected on young exoplanets is therefore necessary, and the preparation of reference materials for spectroscopic observations is of paramount importance. In particular, the deduction of chemical markers identifying specific processes and features in exoplanetary environments, ideally "uniquely". For instance, prebiotic feedstock molecules, in the form of aerosols and vapours, could be observed in transmission spectra in the near future whilst their surface deposits could be observed from reflectance spectra. The same detection methods also promise to identify particular intermediates of chemical and physical processes known to be prebiotically plausible. Is Ariel truly able to open a window to the past and answer questions concerning the origin of life on our planet and the universe? In this paper, we discuss aspects of prebiotic chemistry that will help in formulating future observational and data interpretation strategies for the Ariel mission. This paper is intended to open a discussion and motivate future detailed laboratory studies of prebiotic processes on young exoplanets and their chemical signatures.

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Kr I spectra in the 5–14 µm range

Civiš

Kubelík

Pastorek

et al. 2020

Journal of Quantitative Spectroscopy and Radiative Transfer

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Zn I spectra in the 1300–6500cm−1 range

Cited by 11 publications

References 31 publications

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range

Ariel – a window to the origin of life on early earth?

Kr I spectra in the 5–14 µm range

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Zn I spectra in the 1300–6500cm−1 range

Cited by 11 publications

References 31 publications

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm−1 range

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm−1 range

Ariel – a window to the origin of life on early earth?

Kr I spectra in the 5–14 µm range

Contact Info

Product

Resources

About

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range

Laser ablation of an indium target: time-resolved Fourier-transform infrared spectra of In I in the 700–7700 cm⁻¹ range