Fitting infrared ice spectra with genetic modelling algorithms Presenting the ENIIGMA fitting tool

Autor: W. R. M. Rocha, Lars E. Kristensen, G. Perotti, Jes K. Jørgensen
Jazyk: angličtina
Rok vydání: 2021
Předmět:
010504 meteorology & atmospheric sciences
Infrared
Evolutionary algorithm
MU-M
FOS: Physical sciences
Context (language use)
LOW-MASS STARS
01 natural sciences
Spectral line
Matrix decomposition
symbols.namesake
0103 physical sciences
Range (statistics)
OPTICAL-CONSTANTS
Instrumentation and Methods for Astrophysics (astro-ph.IM)
010303 astronomy & astrophysics
SPITZER SPECTROSCOPIC SURVEY
Solar and Stellar Astrophysics (astro-ph.SR)
molecules [ISM]
protostars [stars]
ASTROPHYSICAL ICES
0105 earth and related environmental sciences
Physics
ABSORPTION FEATURES
astrochemistry
INTERSTELLAR ICE
ISM [infrared]
Astronomy and Astrophysics
LINE-OF-SIGHT
YOUNG STELLAR OBJECTS
Astrophysics - Astrophysics of Galaxies
Astrophysics - Solar and Stellar Astrophysics
13. Climate action
Space and Planetary Science
Gaussian noise
Astrophysics of Galaxies (astro-ph.GA)
symbols
Astrophysics::Earth and Planetary Astrophysics
ORGANIC-MOLECULES
Astrophysics - Instrumentation and Methods for Astrophysics
Degeneracy (mathematics)
Algorithm
volatile [solid state]
Zdroj: Rocha, W R M, Perotti, G, Kristensen, L E & Jorgensen, J K 2021, ' Fitting infrared ice spectra with genetic modelling algorithms Presenting the ENIIGMA fitting tool ', Astronomy & Astrophysics, vol. 654, A158 . https://doi.org/10.1051/0004-6361/202039360
DOI: 10.1051/0004-6361/202039360
Popis: Context. A variety of laboratory ice spectra simulating different chemical environments, ice morphology as well as thermal and energetic processing are demanded to provide an accurate interpretation of the infrared spectra of protostars. To answer which combination of laboratory data best fit the observations, an automated statistically-based computational approach becomes necessary. Aims. To introduce a new approach, based on evolutionary algorithms, to search for molecules in ice mantles via spectral decomposition of infrared observational data with laboratory ice spectra. Methods. A publicly available and open-source fitting tool, called ENIIGMA (dEcompositioN of Infrared Ice features using Genetic Modelling Algorithms), is introduced. The tool has dedicated Python functions to carry out continuum determination of the protostellar spectra, silicate extraction, spectral decomposition and statistical analysis to calculate confidence intervals and quantify degeneracy. As an assessment of the code, several tests were conducted with known ice samples and constructed mixtures. A complete analysis of the Elias 29 spectrum was performed as well. Results. The ENIIGMA fitting tool can identify the correct ice samples and their fractions in all checks with known samples tested in this paper. Concerning the Elias 29 spectrum, the broad spectral range between 2.5-20 $\mu$m was successfully decomposed after continuum determination and silicate extraction. This analysis allowed the identification of different molecules in the ice mantle, including a tentative detection of CH$_3$CH$_2$OH. Conclusions. The ENIIGMA is a toolbox for spectroscopy analysis of infrared spectra that is well-timed with the launch of the James Webb Space Telescope. Additionally, it allows for exploring the different chemical environments and irradiation fields in order to correctly interpret astronomical observations.
Comment: 23 pages, 19 figures, 3 tables. Accepted for publication in A&A
Databáze: OpenAIRE