DATABASE and NKABS code
We present here a Database about the spectroscopy of Astrophysical ices in the infrared including refractive index from the LASA laboratory and associated laboratories (LNLS, GANIL, PUC-RIO). This Database is presented in two groups: 1- Unirradiated ices and 2- processed ices by coscmic-ray analogs. Future databases will also cover X-ray and electron bombardment data.
Additonaly, we also present a code for the determination of optical constants (complex refractive index) of thin films directly from the absorbance data in the infrared, called NKABS. The code is written in the Python language, being more accurated and faster than previous methods in the literature. For solving the Kramers-Kronig relationship, we used the Maclaurin's methodoly. Unlike other codes, which found convergence in 30 to 40 iterations, the NKABS reach the convergence in just 4 or 5 iterations. Additionally, to evaluate the error, this code calculates the MAPE (Mean Absolute Percentage Error) and the chi-square χ2. The typical MAPE error obtained using NKABS is less than 1 x 10-3%. The code is available on-line as well as the data base obtained here. The NKABS can be also employed for the calculation refractive index of processed samples (by heating or radiation). Such data, as well as the the refractive index of virgin samples, are needed as input in several astrophysical models that calculates the radiative transfer in dusty astrophysical environments such as protoplanetary disks and circunstellar environments as well dense molecular clouds.The first version of the code was developed during the PhD thesis of Will Robson in 2013.
The original paper can be obtained here:
DATABASE 1: UNIRRADIATED FTIR spectra (absorbance) and optical constants (m=n+ik) of astrophysical ices and thin films.
Data Label | Temp (K) |
Sample (IR Absorbance and optical constants) |
Reference/notes |
G1 | 10 | CO | Rocha & Pilling (2014), Ehrenfreund et al. 1999 |
G2 | 13 | CO2 | Rocha & Pilling (2014), Pilling et al. 2010b |
G3 | 14 | NH3 | Rocha & Pilling (2014), Pilling et al. 2012 |
G4 | 12 | SO2 | Rocha & Pilling (2014) |
S1 | 300 | alpha-glycine | Rocha & Pilling (2014), Pilling et al. 2011 |
S2 | 14 | alpha-gycine | Rocha & Pilling (2014), Portugal et al. 2013 |
S3 | 300 | beta-glycine | Rocha & Pilling (2014), Pilling et al. 2013 |
S4 | 300 | DL-proline | Rocha & Pilling (2014), Pilling et al. 2011 |
S5 | 300 | DL-valine | Rocha & Pilling (2014), Pilling et al. 2011 |
S6 | 300 | adenine | Rocha & Pilling (2014), Pilling et al. 2011 |
S7 | 300 | uracil | Rocha & Pilling (2014), Pilling et al. 2011 |
L1 | 12 | H2O (amorphous) | Rocha & Pilling (2014) |
L2 | 165 | H2O (crystalline) | Rocha & Pilling (2014) |
L3 | 12 | acetone | Rocha & Pilling (2014) |
L4 | 12 | acetonirtile | Rocha & Pilling (2014) |
L5 | 12 | acetic acid | Rocha & Pilling (2014) |
L6 | 12 | formic acid | Rocha & Pilling (2014) |
L7 | 12 | ethanol | Rocha & Pilling (2014) |
L8 | 12 | methanol | Rocha & Pilling (2014) |
L9 | 13 | cycle-hexane | Rocha & Pilling (2014), Pilling et al. 2012 |
M1 | 12 | Titan aerosol - N2CH4 (19:1) | Rocha & Pilling (2014) |
M2 | 13 | H2O:CO2 (9:1) | Rocha & Pilling (2014), Pilling et al. 2010b |
M3 | 13 | H2O:CO2 (1:1) | Rocha & Pilling (2014), Pilling et al. 2010b |
M4 | 13 | H2O:HCOOH (1:1) | Rocha & Pilling (2014), Bergantini et al 2013 |
M5 | 13 | H2O:NH3:CO (1:0.5:0.4) | Rocha & Pilling (2014), Pilling et al. 2010a |
M6 | 14 | H2O:NH3:c-C6H12 (1:0.3:0.7) | Rocha & Pilling (2014), Pilling et al. 2012 |
M7 | 80 | Enceladus - H2O:CO2:NH3:CH4 (9:1:1:1) | Rocha & Pilling (2014) |
M8 | 90 | Europa -H2O:CO2:NH3:SO2 (10:1:1:1) | Rocha & Pilling (2014) |
OBS: G# films from condensed gaseous samples, S# films from solid samples,L# films frozen thin films from evaporated liquid samples in vaccum, M# films from mixed samples.
DATABASE 2 : FTIR spectra (absorbance) and optical constants (m=n+ik) of bombarded astrophysical ices and thin films by heavy ions. NEW!!!!
Data Label |
Temp (K) |
Sample (IR absorbance and optical constants) |
Projectile |
Flucence (x1010 ions cm-2) |
References / Notes |
D1a |
13 |
52 MeV 58Ni13+ |
0 |
Rocha et al. (2016); Pilling et al. (2010b) |
|
D1b |
13 |
52 MeV 58Ni13+ |
100 |
Rocha et al. (2016); Pilling et al. (2010b) |
|
D1c |
13 |
52 MeV 58Ni13+ |
1000 |
Rocha et al. (2016); Pilling et al. (2010b) |
|
D2a |
13 |
52 MeV 58Ni13+ |
0 |
Rocha et al. (2016); Pilling et al. (2010b) |
|
D2b |
13 |
52 MeV 58Ni13+ |
100 |
Rocha et al. (2015); Pilling et al. (2010b) |
|
D2c |
13 |
52 MeV 58Ni13+ |
500 |
Rocha et al. (2016); Pilling et al. (2010b) |
|
D3a |
16 |
40 MeV 58Ni11+ |
0 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D3b |
16 |
40 MeV 58Ni11+ |
100 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D3c |
16 |
40 MeV 58Ni11+ |
1000 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D4a |
16 |
40 MeV 58Ni11+ |
0 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D4b |
16 |
40 MeV 58Ni11+ |
100 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D4c |
16 |
40 MeV 58Ni11+ |
1000 |
Rocha et al. (2016); de Barros et al. (in prep) |
|
D5a |
13 |
46 MeV 58Ni13+ |
0 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D5b |
13 |
46 MeV 58Ni13+ |
100 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D5c |
13 |
46 MeV 58Ni13+ |
1600 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D6a |
15 |
46 MeV 58Ni11+ |
0 |
Rocha et al. (2016); Bergantini et al. (2014) |
|
D6b |
15 |
46 MeV 58Ni11+ |
100 |
Rocha et al. (2016); Bergantini et al. (2014) |
|
D6c |
15 |
46 MeV 58Ni11+ |
1000 |
Rocha et al. (2016); Bergantini et al. (2014) |
|
D7a |
15 |
40 MeV 58Ni11+ |
0 |
Rocha et al. (2016); de Barros et al. (2014b) |
|
D7b |
15 |
40 MeV 58Ni11+ |
100 |
Rocha et al. (2016); de Barros et al. (2014b) |
|
D7c |
15 |
40 MeV 58Ni11+ |
1000 |
Rocha et al. (2016); de Barros et al. (2014b) |
|
D8a |
13 |
46 MeV 58Ni13+ |
0 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D8b |
13 |
46 MeV 58Ni13+ |
100 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D8c |
13 |
46 MeV 58Ni13+ |
2000 |
Rocha et al. (2016); Pilling et al. (2010a) |
|
D9a |
13 |
632 MeV 58Ni24+ |
0 |
Rocha et al. (2016); Pilling et al. (2012) |
|
D9b |
13 |
632 MeV 58Ni24+ |
200 |
Rocha et al. (2016); Pilling et al. (2012) |
|
D9c |
13 |
632 MeV 58Ni24+ |
3000 |
Rocha et al. (2016); Pilling et al. (2012) |
|
D10a |
72 |
15.7 MeV 16O5+ |
0 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D10b |
72 |
15.7 MeV 16O5+ |
10 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D10c |
72 |
15.7 MeV 16O5+ |
100 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D11a |
15 |
220 MeV 16O7+ |
0 |
Rocha et al. (2016); de Barros et al. (2014a) |
|
D11b |
15 |
220 MeV 16O7+ |
1700 |
Rocha et al. (2016); de Barros et al. (2014a) |
|
D11c |
15 |
220 MeV 16O7+ |
9600 |
Rocha et al. (2016); de Barros et al. (2014a) |
|
D12a |
35 |
15.7 MeV 16O5+ |
0 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D12b |
35 |
15.7 MeV 16O5+ |
10 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D12c |
35 |
15.7 MeV 16O5+ |
100 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D13a |
72 |
15.7 MeV 16O5+ |
0 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D13b |
72 |
15.7 MeV 16O5+ |
10 |
Rocha et al. (2016); Pilling et al. (in prep.) |
|
D13c |
72 |
15.7 MeV 16O5+ |
100 |
Rocha et al. (2016); Pilling et al. (in prep.) |
Grupo de Pesquisa em AstroquĂmica e Astrobiologia - GAA
Last update 30/09/2016