Spectroscopic Analysis Tool for intEgraL fieLd unIt daTacubEs (satellite): Case studies of NGC 7009 and NGC 6778 with MUSE
arXiv:2203.06175 · doi:10.1093/mnras/stac632
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.
arXiv comment20 pages, 20 figures, 7 tables, Accepted for publication in MNRAS
References in corpus (45)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Astropy: A Community Python Package for Astronomy
- The NumPy array: a structure for efficient numerical computation
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- The MUSE second-generation VLT instrument
- PyNeb: a new tool for analyzing emission lines. I. Code description and validation of results
- Mocassin: A fully three-dimensional Monte Carlo photoionization code
- Planetary Nebulae: Observational Properties, Mimics, and Diagnostics
- The dusty MOCASSIN: fully self-consistent 3D photoionisation and dust radiative transfer models
- Ionization Correction Factors for Planetary Nebulae: I- Using optical spectra
- Effects of Pre-ionisation in Radiative Shocks I: Self-Consistent Models
- New Galactic supernova remnants discovered with IPHAS
- NGC 6778: Strengthening the link between extreme abundance discrepancy factors and central star binarity in planetary nebulae
- Extensive Online Shock Model Database
- Integral field spectroscopy of planetary nebulae: mapping the line diagnostics and hydrogen-poor zones with VLT FLAMES
- Very deep spectroscopy of the bright Saturn Nebula NGC 7009 -- I. Observations and plasma diagnostics
- Discovery of close binary central stars in the planetary nebulae NGC 6326 and NGC 6778
- Diffuse X-ray emission from the planetary nebula NGC 7009
- Low-ionization structures in planetary nebulae - I: physical, kinematic and excitation properties
- Atomic Data Assessment with PyNeb
- Imaging the elusive H-poor gas in the high ADF planetary nebula NGC 6778
- Temperature Variations from HST Imagery and Spectroscopy of NGC 7009
- The physical parameters, excitation and chemistry of the rim, jets and knots of the planetary nebula NGC 7009
- On the nitrogen abundance of FLIERs: the outer knots of the planetary nebula NGC 7009
- The 3-D ionization structure and evolution of NGC 7009 (Saturn Nebula)
- MUSE spectroscopy of planetary nebulae with high abundance discrepancies
- IFU spectroscopy of southern PNe: III
- Synthetic observations of simulated pillars of creation
- The extinction and dust-to-gas structure of the planetary nebula NGC 7009 observed with MUSE
- NGC 6778: a disrupted planetary nebula around a binary central star
- Very deep spectroscopy of the bright Saturn Nebula NGC 7009 - II. Analysis of the rich optical recombination spectrum
- Low-ionization pairs of knots in planetary nebulae: physical properties and excitation
- 3-D Photoionization Structure and Distances of Planetary Nebulae I. NGC6369
- The MUSE view of the planetary nebula NGC 3132
- Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS I. Description of the Observations, Global Emission-line Measurements, and CNO Abundances
- Exploring the differences of integrated and spatially resolved analysis using integral field unit data: The case of Abell 14
- An Imaging Spectroscopic Survey of the Planetary Nebula NGC 7009 with MUSE
- Mapping and Spectroscopy of the Planetary Nebula NGC 7009 in the Visual and Infrared
- Spatially resolved physical and chemical properties of the planetary nebula NGC 3242
- H emission in the low-ionisation structures of the Planetary Nebulae NGC 7009 and NGC 6543
- IFU spectroscopy of Southern PNe: VII Photo-ionization modelling of intermediate excitation class objects
- 3-D Photoionization Structure and Distances of Planetary Nebulae II. Menzel 1
- Physico-chemical spectroscopic mapping of the planetary nebula NGC 40 and the 2D_NEB, a new 2D algorithm to study ionised nebulae
- The impact of strong recombination on temperature determination in planetary nebulae
- The Voronoi tessellation method in astronomy
Cited by in corpus (7)
- Low-ionization structures in planetary nebulae -- III. The statistical analysis of physico-chemical parameters and excitation mechanisms
- Low-ionization structures in planetary nebulae -- II. Densities, temperatures, abundances and excitation of 6 PNe
- Detection of the [C I] 8727 emission line. Low-ionization structures in NGC 7009
- The [S II] Spectral Images of the Planetary Nebula NGC 7009: II. Major Axis
- Low-ionization structures in planetary nebulae -- IV. The molecular hydrogen counterpart
- Dissecting NGC 3132: Tracing the mass-loss history of the southern ring planetary nebula
- [Fe II] 1.644m imaging survey of planetary nebulae with low-ionisation structures