Validation of open-source science tools and background model construction in -ray astronomy
arXiv:1910.08088 · doi:10.1051/0004-6361/201936452
Abstract
In classical analyses of -ray data from IACTs, such as H.E.S.S., aperture photometry, or photon counting, is applied in a (typically circular) region of interest (RoI) encompassing the source. A key element in the analysis is to estimate the amount of background in the RoI due to residual cosmic ray-induced air showers in the data. Various standard background estimation techniques have been developed in the last decades, most of them rely on a measurement of the background from source-free regions within the observed field of view. However, in particular in the Galactic plane, source analysis and background estimation are hampered by the large number of, sometimes overlapping, -ray sources and large-scale diffuse -ray emission. For complicated fields of view, a three-dimensional (3D) likelihood analysis shows the potential to be superior to classical analysis. In this analysis technique, a spectromorphological model, consisting of one or multiple source components and a background component, is fitted to the data, resulting in a complete spectral and spatial description of the field of view. For the application to IACT data, the major challenge of such an approach is the construction of a robust background model. In this work, we apply the 3D likelihood analysis to various test data recently made public by H.E.S.S., using the open analysis frameworks ctools and Gammapy. First, we show that, when using these tools in a classical analysis approach and comparing to the proprietary H.E.S.S. analysis framework, virtually identical high-level analysis results are obtained. We then describe the construction of a generic background model from data of H.E.S.S. observations, and demonstrate that a 3D likelihood analysis using this background model yields high-level analysis results that are highly compatible with those obtained from the classical analyses. (abridged)
16(+6) pages, 23(+10) figures
References in corpus (22)
- Astropy: A Community Python Package for Astronomy
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Observations of the Crab Nebula with H.E.S.S
- An Exceptional VHE Gamma-Ray Flare of PKS 2155-304
- High-energy particle acceleration in the shell of a supernova remnant
- The H.E.S.S. Galactic plane survey
- The Fermi Galactic Center GeV Excess and Implications for Dark Matter
- Background Modelling in Very-High-Energy gamma-ray Astronomy
- A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with H.E.S.S
- Gamma-Hadron Separation in Very-High-Energy gamma-ray astronomy using a multivariate analysis method
- H.E.S.S. Observations of PKS 2155-304
- Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with H.E.S.S
- Simultaneous multiwavelength observations of the second exceptional gamma-ray flare of PKS 2155-304 in July 2006
- VHE gamma-ray emission of PKS 2155-304: spectral and temporal variability
- H.E.S.S. observations of RX J1713.7-3946 with improved angular and spectral resolution; evidence for gamma-ray emission extending beyond the X-ray emitting shell
- Probing the extent of the non-thermal emission from the Vela X region at TeV energies with H.E.S.S
- GammaLib and ctools: A software framework for the analysis of astronomical gamma-ray data
- Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S
- Impact of aerosols and adverse atmospheric conditions on the data quality for spectral analysis of the H.E.S.S. telescopes
- Characterizing the gamma-ray long-term variability of PKS 2155-304 with H.E.S.S. and Fermi-LAT
- A new template background estimate for source searching in TeV gamma-ray astronomy
- A new method of reconstructing very-high-energy gamma-ray spectra: the Template Background Spectrum
Cited by in corpus (26)
- Revealing x-ray and gamma ray temporal and spectral similarities in the GRB 190829A afterglow
- Gammapy: A Python package for gamma-ray astronomy
- Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi
- Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433
- A deep spectromorphological study of the -ray emission surrounding the young massive stellar cluster Westerlund 1
- Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
- TeV emission of Galactic plane sources with HAWC and H.E.S.S
- Evidence of 100 TeV -ray emission from HESS J1702-420: A new PeVatron candidate
- HESS J1809193: a halo of escaped electrons around a pulsar wind nebula?
- Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis
- Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
- Toward the ultimate reach of current imaging atmospheric Cherenkov telescopes and their sensitivity to TeV dark matter
- Probing the galactic cosmic-ray density with current and future -ray instruments
- Detection prospects of very and ultra high-energy gamma rays from extended sources with ASTRI, CTA, and LHAASO
- Very-high-energy -ray emission from young massive star clusters in the Large Magellanic Cloud
- The Making of Catalogues of Very-High-Energy γ-ray Sources
- Exploring the high energy frontiers of the Milky Way with ground-based gamma-ray astronomy: PeVatrons and the quest for the origin of Galactic cosmic-rays
- Prospects for combined analyses of hadronic emission from -ray sources in the Milky Way with CTA and KM3NeT
- Testing source confusion and identification capability in Cherenkov Telescope Array data
- Background rejection using image residuals from large telescopes in imaging atmospheric Cherenkov telescope arrays
- Analysis Methods for Gamma-ray Astronomy
- Validation of standardized data formats and tools for ground-level particle-based gamma-ray observatories
- Event types in H.E.S.S.: a combined analysis for different telescope types and energy ranges
- Search for long-term variability of HESS J1745-290
- Standardised formats and open-source analysis tools for the MAGIC telescopes data
- Unveiling extended gamma-ray emission around HESS J1813-178