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J/A+A/540/A2        Refractive index of hydrocarbon solids    (Jones, 2012)

Variations on a theme - the evolution of hydrocarbon solids. II. Optical property modelling - the optEC(s) model. Jones A. <Astron. Astrophys. 540, A2 (2012)> =2012A&A...540A...2J
ADC_Keywords: Interstellar medium ; Models Keywords: dust, extinction - ISM: general Abstract: The properties of hydrogenated amorphous carbon (a-C:H) dust are known to evolve in response to the local conditions. We present an adaptable model for the determination of the optical properties of low-temperature, interstellar a-C:H grains that is based on the fundamental physics of their composition. Description: The imaginary part of the complex refractive index m(n,k), k, for a-C:H materials, from 50eV to cm wavelengths, is derived and the real part, n, of the complex refractive index m(n,k) is then calculated using the Kramers-Kronig relations. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file optecsn.dat 159 1000 *Real part of the refractive index data optecsk.dat 159 1000 *Imaginary part of the refractive index data
Note on *.dat: for a suite of a-C:H materials predicted by the optEC(s) model as a function of wavelength [micron], energy E [eV] and band gap Eg [eV].
See also: J/A+A/542/A98 : Hydrocarbon solids. optEC(s) model. II. (Jones, 2012) Byte-by-byte Description of file: optecsn.dat
Bytes Format Units Label Explanations
1- 9 E9.4 um lambda Wavelength 11- 19 E9.4 eV E Energy equivalent to wavelength 21- 29 E9.4 --- n0 Real part of m(n,k) Eg = -0.1 eV (Eg-) 31- 39 E9.4 --- n1 Real part of m(n,k) Eg = 0.0 eV 41- 49 E9.4 --- n2 Real part of m(n,k) Eg = 0.1 eV 51- 59 E9.4 --- n3 Real part of m(n,k) Eg = 0.25 eV 61- 69 E9.4 --- n4 Real part of m(n,k) Eg = 0.5 eV 71- 79 E9.4 --- n5 Real part of m(n,k) Eg = 0.75 eV 81- 89 E9.4 --- n6 Real part of m(n,k) Eg = 1.0 eV 91- 99 E9.4 --- n7 Real part of m(n,k) Eg = 1.5 eV 101-109 E9.4 --- n8 Real part of m(n,k) Eg = 1.15 eV 111-119 E9.4 --- n9 Real part of m(n,k) Eg = 1.75 eV 121-129 E9.4 --- n10 Real part of m(n,k) Eg = 2.0 eV 131-139 E9.4 --- n11 Real part of m(n,k) Eg = 2.25 eV 141-149 E9.4 --- n12 Real part of m(n,k) Eg = 2.5 eV 151-159 E9.4 --- n13 Real part of m(n,k) Eg = 2.67 eV (Eg+)
Byte-by-byte Description of file: optecsk.dat
Bytes Format Units Label Explanations
1- 9 E9.4 um lambda Wavelength 11- 19 E9.4 eV E Energy equivalent to wavelength 21- 29 E9.4 --- k0 Imaginary part of m(n,k) Eg = -0.1 eV (Eg-) 31- 39 E9.4 --- k1 Imaginary part of m(n,k) Eg = 0.0 eV 41- 49 E9.4 --- k2 Imaginary part of m(n,k) Eg = 0.1 eV 51- 59 E9.4 --- k3 Imaginary part of m(n,k) Eg = 0.25 eV 61- 69 E9.4 --- k4 Imaginary part of m(n,k) Eg = 0.5 eV 71- 79 E9.4 --- k5 Imaginary part of m(n,k) Eg = 0.75 eV 81- 89 E9.4 --- k6 Imaginary part of m(n,k) Eg = 1.0 eV 91- 99 E9.4 --- k7 Imaginary part of m(n,k) Eg = 1.5 eV 101-109 E9.4 --- k8 Imaginary part of m(n,k) Eg = 1.15 eV 111-119 E9.4 --- k9 Imaginary part of m(n,k) Eg = 1.75 eV 121-129 E9.4 --- k10 Imaginary part of m(n,k) Eg = 2.0 eV 131-139 E9.4 --- k11 Imaginary part of m(n,k) Eg = 2.25 eV 141-149 E9.4 --- k12 Imaginary part of m(n,k) Eg = 2.5 eV 151-159 E9.4 --- k13 Imaginary part of m(n,k) Eg = 2.67 eV (Eg+)
History: * 13-Mar-2012: First version * 15-Aug-2012: Corrected version, from author Acknowledgements: Anthony Jones, Anthony.Jones(at)ias.u-psud.fr References: Jones, Paper I, 2012A&A...540A...1J Jones, Paper III, 2012A&A...542A..98J, Cat. J/A+A/542/A98
(End) Anthony Jones [IAS], Patricia Vannier [CDS] 16-Feb-2012
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

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