LZIFU: an emission-line fitting toolkit for integral field spectroscopy data
arXiv:1607.06561 · doi:10.1007/s10509-016-2865-2
Abstract
We present LZIFU (LaZy-IFU), an IDL toolkit for fitting multiple emission lines simultaneously in integral field spectroscopy (IFS) data. LZIFU is useful for the investigation of the dynamical, physical and chemical properties of gas in galaxies. LZIFU has already been applied to many world-class IFS instruments and large IFS surveys, including the Wide Field Spectrograph, the new Multi Unit Spectroscopic Explorer (MUSE), the Calar Alto Legacy Integral Field Area (CALIFA) survey, the Sydney-Australian-astronomical-observatory Multi-object Integral-field spectrograph (SAMI) Galaxy Survey. Here we describe in detail the structure of the toolkit, and how the line fluxes and flux uncertainties are determined, including the possibility of having multiple distinct kinematic components. We quantify the performance of LZIFU, demonstrating its accuracy and robustness. We also show examples of applying LZIFU to CALIFA and SAMI data to construct emission line and kinematic maps, and investigate complex, skewed line profiles presented in IFS data. The code is made available to the astronomy community through github. LZIFU will be further developed over time to other IFS instruments, and to provide even more accurate line and uncertainty estimates.
19 pages, 14 figure, accepted to Astrophysics and Space Science. Code available at https://github.com/hoiting/LZIFU/releases
References in corpus (21)
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- The MUSE second-generation VLT instrument
- The SAMI Galaxy Survey: instrument specification and target selection
- Recovering galaxy star formation and metallicity histories from spectra using VESPA
- CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release
- The Wide Field Spectrograph (WiFeS): Performance and Data Reduction
- Metallicity gradients in local field star-forming galaxies: Insights on inflows, outflows, and the coevolution of gas, stars and metals
- Contour binning: a new technique for spatially-resolved X-ray spectroscopy applied to Cassiopeia A
- The SAMI Galaxy Survey: Shocks and Outflows in a normal star-forming galaxy
- Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting
- The SAMI Galaxy Survey: Early Data Release
- Stellar Population and Kinematic Profiles in Spiral Bulges & Disks: Population Synthesis of Integrated Spectra
- IFU observations of luminous type II AGN - I. Evidence for ubiquitous winds
- Starburst-AGN mixing: II. Optically-selected active galaxies
- Probing the Physics of Narrow Line Regions in Active Galaxies II: The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)
- Probing the Physics of Narrow Line Regions in Active Galaxies III: Accretion and Cocoon Shocks in the LINER NGC1052
- Shocked Gas in IRAS F17207-0014: ISM Collisions and Outflows
- Morphologies and stellar populations of galaxies in the core of Abell 2218
- Galaxy Interactions in Compact Groups II: abundance and kinematic anomalies in HCG 91c
- The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3
- The Hector Survey: integral field spectroscopy of 100,000 galaxies
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- The SAMI Galaxy Survey: the third and final data release
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- The Effects of Diffuse Ionized Gas and Spatial Resolution on Metallicity Gradients: TYPHOON Two-Dimensional Spectrophotometry of M83
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- Dissecting Galaxies: Separating Star Formation, Shock Excitation and AGN Activity in the Central Region of NGC 613
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- Probing the Physics of Narrow Line Regions in Active Galaxies IV: Full data release of The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)
- The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies
- Metallicity, ionization parameter, and pressure variations of HII regions in the TYPHOON spiral galaxies
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- BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE
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- The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge
- The SAMI Galaxy Survey: Physical drivers of stellar-gas kinematic misalignments in the nearby Universe
- SDSS-IV MaNGA: The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies
- Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
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- A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
- The SAMI Galaxy Survey: the difference between ionised gas and stellar velocity dispersions
- An increase in black hole activity in galaxies with kinematically misaligned gas
- Mapping electron temperature variations across a spiral arm in NGC 1672
- A Multiwavelength view of IC 860: What Is in Action inside Quenching Galaxies
- The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure
- The SAMI Galaxy Survey: Bayesian Inference for Gas Disk Kinematics using a Hierarchical Gaussian Mixture Model
- The complex multi-component outflow of the Seyfert galaxy NGC 7130
- Constraints on the densities and temperature of Seyfert 2 NLR
- The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
- The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
- An interacting galaxy pair at the origin of a light echo
- The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies
- Shocked POststarburst Galaxy Survey. IV. Outflows in Shocked Post-Starburst Galaxies Are Not Responsible For Quenching
- The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations