J/A+A/629/A112      Complex refractive index of CO ice         (Giuliano+, 2019)

Broadband spectroscopy of astrophysical ice analogues. I. Direct measurement of complex refractive index of CO ice using terahertz time-domain spectroscopy. Giuliano B.M., Gavdush A.A., Mueller B., Zaytsev K.I., Grassi T., Ivlev A.V., Palumbo M.E., Baratta G.A., Scire C., Komandin G.A., Yurchenko S.O., Caselli P. <Astron. Astrophys. 629, A112 (2019)> =2019A&A...629A.112G 2019A&A...629A.112G (SIMBAD/NED BibCode)
ADC_Keywords: Interstellar medium ; Carbon monoxide ; Spectroscopy Keywords: astrochemistry - methods: laboratory: solid state - ISM: molecules - infrared: ISM Abstract: Reliable, directly measured optical properties of astrophysical ice analogs in the infrared (IR) and terahertz (THz) range are missing. These parameters are of great importance to model the dust continuum radiative transfer in dense and cold regions, where thick ice mantles are present, and are necessary for the interpretation of future observations planned in the far-IR region. Coherent THz radiation allows direct measurement of the complex dielectric function (refractive index) of astrophysically relevant ice species in the THz range. The time-domain waveforms and the frequency-domain spectra of reference samples of CO ice, deposited at a temperature of 28.5K and annealed to 33K at different thicknesses, have been recorded. A new algorithm is developed to reconstruct the real and imaginary parts of the refractive index from the time-domain THz data. The complex refractive index in the wavelength range of 1mm-150um (0.3-2.0THz) has been determined for the studied ice samples, and compared with available data found in the literature. The developed algorithm of reconstructing the real and imaginary parts of the refractive index from the time-domain THz data enables, for the first time, the determination of optical properties of astrophysical ice analogs without using the Kramers-Kronig relations. The obtained data provide a benchmark to interpret the observational data from current ground based facilities as well as future space telescope missions, and have been used to estimate the opacities of the dust grains in presence of CO ice mantles. Description: Optical properties of CO ice. (a) Real part of the refractive index, (b) amplitude absorption coefficient, (c) real and (d) imaginary parts of the dielectric permittivity (see Eqs. 1 and 2). For all deposition intervals, the dielectric curves demonstrate the existence of a Lorenz-like absorption peak, centered near 1.5THz and featuring similar bandwidth. Distortions of the results seen at frequencies below 0.3THz (such as an oscillatory character of n and varepsilon as well as an increase of varepsilon with decreasing frequency) are due to diffraction effects (see Sec.2.2). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig6_4m.dat 75 135 Complex refractive index and dielectric properties for 4 min steps deposition fig6_5m.dat 75 135 Complex refractive index and dielectric properties for 5 min steps deposition fig6_6m.dat 75 135 Complex refractive index and dielectric properties for 6 min steps deposition -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): fig6_4m.dat fig6_5m.dat fig6_6m.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.9 THz Freq Frequency 17- 27 F11.9 --- nre Real refractive index 32- 43 F12.9 --- alpha Amplitude absorption coefficient 49- 59 F11.9 --- eps-real Real dielectric permittivity 65- 75 F11.9 --- eps-imag Imaginary dielectric permittivity -------------------------------------------------------------------------------- Acknowledgements: Barbara Michela Giuliano, giuliano(at)mpe.mpg.de
(End) Patricia Vannier [CDS] 26-Jul-2019
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line