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Using radio astronomical receivers for molecular spectroscopic characterization in astrochemical laboratory simulations: A proof of concept

AutorTanarro, Isabel ; Alemán, B.; Pardo Carrión, Juan Ramón ; Santoro, G.; Lauwaet, Koen; Moreno, E.; Agúndez, Marcelino; Goicoechea, Javier R. ; Sobrado, Jesús Manuel ; Martínez, Lidia; Doménech, José Luis ; Herrero, Víctor J. ; Peláez, Ramón J. ; Castellanos, M.; Martín-Gago, José A. ; Cernicharo, José
Palabras claveMethods: laboratory: molecular
Instrumentation: spectrographs
Astrochemistry
Molecular data
Fecha de publicación22-dic-2017
EditorEDP Sciences
CitaciónAstronomy & Astrophysics 609: A15 (2018)
ResumenWe present a proof of concept on the coupling of radio astronomical receivers and spectrometers with chemical reactors and the performances of the resulting setup for spectroscopy and chemical simulations in laboratory astrophysics. Several experiments including cold plasma generation and UV photochemistry were performed in a 40 cm long gas cell placed in the beam path of the Aries 40 m radio telescope receivers operating in the 41–49 GHz frequency range interfaced with fast Fourier transform spectrometers providing 2 GHz bandwidth and 38 kHz resolution. The impedance matching of the cell windows has been studied using di erent materials. The choice of the material and its thickness was critical to obtain a sensitivity identical to that of standard radio astronomical observations. Spectroscopic signals arising from very low partial pressures of CH3OH, CH3CH2OH, HCOOH, OCS, CS, SO2 (<103 mbar) were detected in a few seconds. Fast data acquisition was achieved allowing for kinetic measurements in fragmentation experiments using electron impact or UV irradiation. Time evolution of chemical reactions involving OCS, O2 and CS2 was also observed demonstrating that reactive species, such as CS, can be maintained with high abundance in the gas phase during these experiments
DescripciónI. Tanarro et al. -- 16 pags., 18 figs., app.
Versión del editorhttp://doi.org/10.1051/0004-6361/201730969
URIhttp://hdl.handle.net/10261/160485
DOI10.1051/0004-6361/201730969
ISSN0004-6361
E-ISSN1432-0746
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