Mr-Moose: An advanced SED-fitting tool for heterogeneous multi-wavelength datasets
arXiv:1804.01748 · doi:10.1093/mnras/sty831
Abstract
We present the public release of MrMoose, a fitting procedure that is able to perform multi-wavelength and multi-object spectral energy distribution (SED) fitting in a Bayesian framework. This procedure is able to handle a large variety of cases, from an isolated source to blended multi-component sources from an heterogeneous dataset (i.e. a range of observation sensitivities and spectral/spatial resolutions). Furthermore, MrMoose handles upper-limits during the fitting process in a continuous way allowing models to be gradually less probable as upper limits are approached. The aim is to propose a simple-to-use, yet highly-versatile fitting tool fro handling increasing source complexity when combining multi-wavelength datasets with fully customisable filter/model databases. The complete control of the user is one advantage, which avoids the traditional problems related to the "black box" effect, where parameter or model tunings are impossible and can lead to overfitting and/or over-interpretation of the results. Also, while a basic knowledge of Python and statistics is required, the code aims to be sufficiently user-friendly for non-experts. We demonstrate the procedure on three cases: two artificially-generated datasets and a previous result from the literature. In particular, the most complex case (inspired by a real source, combining Herschel, ALMA and VLA data) in the context of extragalactic SED fitting, makes MrMoose a particularly-attractive SED fitting tool when dealing with partially blended sources, without the need for data deconvolution.
References in corpus (23)
- Astropy: A Community Python Package for Astronomy
- emcee: The MCMC Hammer
- Stellar population synthesis at the resolution of 2003
- Starburst99: Synthesis Models for Galaxies with Active Star Formation
- Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
- The Spitzer Space Telescope Mission
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- Analysis of galaxy SEDs from far-UV to far-IR with CIGALE: Studying a SINGS test sample
- Modeling the Panchromatic Spectral Energy Distributions of Galaxies
- AGN Dusty Tori: I. Handling of Clumpy Media
- Revisiting the Infrared Spectra of Active Galactic Nuclei with a New Torus Emission Model
- Three-dimensional radiative transfer modeling of AGN dusty tori as a clumpy two-phase medium
- Dusty, Radiation Pressure Dominated Photoionization. I. Model Description, Structure And Grids
- The Large APEX Bolometer Camera LABOCA
- Radiative Transfer Modeling of Three-Dimensional Clumpy AGN Tori and its Application to NGC 1068
- Spectral ageing in the lobes of FR-II radio galaxies: New methods of analysis for broadband radio data
- SEDfit: Software for Spectral Energy Distribution Fitting of Photometric Data
- AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
- ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z=4.75
- BayesCLUMPY: Bayesian Inference with Clumpy Dusty Torus Models
- Self-consistent 2-phase AGN torus models: SED library for observers
- The Mysterious Morphology of MRC0943-242 as Revealed by ALMA and MUSE
- SEDeblend: A new method for deblending spectral energy distributions in confused imaging
Cited by in corpus (11)
- The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
- Massive galaxies on the road to quenching: ALMA observations of powerful high redshift radio galaxies
- New Radio-Loud QSOs at the end of the Re-ionisation Epoch
- SMM J04135+10277: A distant QSO-starburst system caught by ALMA
- Constraining the Radio Properties of the =6.44 QSO VIK J23183113
- Hubble Space Telescope observations of the old pulsar PSR J0108-1431
- Multi-wavelength properties of three new radio-powerful quasi-stellar objects discovered from RACS
- Comprehensive view on a radio-loud QSO: from the radio to the optical/NIR to the X-ray band
- The Dragonfly Galaxy. III. Jet-brightening of a High-redshift Radio Source Caught in a Violent Merger of Disk Galaxies
- High- radio Quasars in RACS I: Selection, identification, and multi-wavelength properties
- HST WFC3/Grism Observations of the Candidate Ultra-High-Redshift Radio Galaxy GLEAM J0917-0012