J/A+A/632/A128      New fitting concep                            (Breda+, 2019)

A new fitting concept for the robust determination of Sersic model parameters. Breda I., Papaderos P., Gomes J.-M., Amarantidis S. <Astron. Astrophys. 632, A128 (2019)> =2019A&A...632A.128B 2019A&A...632A.128B (SIMBAD/NED BibCode)
ADC_Keywords: Models ; Galaxies, photometry Keywords: galaxies: photometry - galaxies: structure - galaxies: fundamental parameters - techniques: photometric - galaxies: starburst - galaxies: elliptical and lenticular, cD Abstract: We present a new fitting concept (iFIT) that permits a robust determination of the equivalent SL model for the general case of galaxies with imperfect SL profiles. iFIT has been extensively tested on synthetic data with a Sersic index 0.3<η<4.2 and an effective radius 1≤Reff(")≤20. Applied to non PSF-convolved data, iFIT can infer the Sersic exponent η with an absolute error of ≤0.2 even for shallow SBPs. As for PSF-degraded data, iFIT can recover the input SL model parameters with a satisfactorily accuracy almost over the entire considered parameter space as long as FWHM(PSF)≤Reff. This study also includes examples of applications of iFIT to ETGs and local low-mass starburst galaxies. These tests confirm that iFIT shows little sensitivity on PSF corrections and SBP limiting surface brightness, and that subtraction of the best-fitting SL model in two different bands generally yields a good match to the observed radial color profile. Description: iFIT is a 1D surface photometry tool for the robust determination of Sersic model parameters, optimally suited for the automated, non-supervised structural characterization of galaxies. It allows for correction of PSF convolution effects, offering the user the option of choosing between a Moffat, Gaussian, or user-supplied PSF. iFIT, which is a standalone FORTRAN code, can be applied to any SBP that is provided in ASCII format and it has the capability of convenient graphical storage of its output. The iFIT distribution package is supplemented with an auxiliary SBP derivation tool in python. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file ifit_fv.f 512 343 iFit source code (written in FORTRAN) ifit_fv 512 532 iFit executable ex_sbp.py 84 111 Algorithm to extract the SBP from an image cfit.py 111 243 Algorithm to fit isophotes to an image -------------------------------------------------------------------------------- Acknowledgements: Iris Breda, iris.breda(at)astro.up.pt History: 16-Dec-2019: on-line version 18-Feb-2020: file cfit.py added
(End) Patricia Vannier [CDS] 18-Oct-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