ORCID Profile
0000-0002-6138-1869
Does something not look right? The information on this page has been harvested from data sources that may not be up to date. We continue to work with information providers to improve coverage and quality. To report an issue, use the Feedback Form.
Publisher: Springer Netherlands
Date: 2008
Publisher: Oxford University Press (OUP)
Date: 14-07-2014
Publisher: American Astronomical Society
Date: 10-02-2007
DOI: 10.1086/510112
Publisher: EDP Sciences
Date: 06-05-2011
Publisher: Springer Science and Business Media LLC
Date: 03-01-2023
Publisher: EDP Sciences
Date: 24-03-2006
Publisher: Springer Science and Business Media LLC
Date: 08-12-2022
Publisher: Oxford University Press (OUP)
Date: 10-03-2022
Abstract: Integral field spectroscopy (IFS) provides a unique capability to spectroscopically study extended sources over a 2D field of view, but it also requires new techniques and tools. In this paper, we present an automatic code, Spectroscopic Analysis Tool for intEgraL fieLd unIt daTacubEs, satellite, designed to fully explore such capability in the characterization of extended objects, such as planetary nebulae, H ii regions, galaxies, etc. satellite carries out 1D and 2D spectroscopic analysis through a number of pseudo-slits that simulate slit spectrometry, as well as emission line imaging. The 1D analysis permits direct comparison of the integral field unit (IFU) data with previous studies based on long-slit spectroscopy, while the 2D analysis allows the exploration of physical properties in both spatial directions. Interstellar extinction, electron temperatures and densities, ionic abundances from collisionally excited lines, total elemental abundances, and ionization correction factors are computed employing the pyneb package. A Monte Carlo approach is implemented in the code to compute the uncertainties for all the physical parameters. satellite provides a powerful tool to extract physical information from IFS observations in an automatic and user configurable way. The capabilities and performance of satellite are demonstrated by means of a comparison between the results obtained from the Multi Unit Spectroscopic Explorer (MUSE) data of the planetary nebula NGC 7009 with the results obtained from long-slit and IFU data available in the literature. The satellite characterization of NGC 6778 based on MUSE data is also presented.
Publisher: IOP Publishing
Date: 08-2004
DOI: 10.1086/422894
Location: Mexico
No related grants have been discovered for Jorge García-Rojas.