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Fermipy: An open-source Python package for analysis of Fermi-LAT Data
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Fermipy is an open-source python framework that facilitates analysis of data collected by the Fermi Large Area Telescope (LAT). Fermipy is built on the Fermi Science Tools, the publicly available software suite provided by NASA for the LAT mission. Fermipy provides a high-level interface for analyzing LAT data in a simple and reproducible way. The current feature set includes methods for extracting spectral energy distributions and lightcurves, generating test statistic maps, finding new source candidates, and fitting source position and extension. Fermipy leverages functionality from other scientific python packages including NumPy, SciPy, Matplotlib, and Astropy and is organized as a community-developed package following an open-source development model. We review the current functionality of Fermipy and plans for future development.
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Cited by 8 Pith papers
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Searching for $\gamma$-ray emission from a bona fide Compact Symmetric Object sample: a $\gamma$-ray signal near GB6 J0906+4124
No bona fide CSO in a 73-source sample is firmly detected in 16 years of Fermi-LAT data; a ~4σ signal near GB6 J0906+4124 is a plausible but unconfirmed counterpart.
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Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars
Systematic Fermi-LAT search detects VHE emission from 14 Compton-dominated blazars (4 new at >5σ) and constrains the emitting region to >1.1–1.4 BLR radii.
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An 18-year Fermi-LAT stacking limit on GeV $\gamma$-ray emission from particle-accelerating colliding-wind binaries
Clean stack of six high-latitude PACWBs is null (p=0.83), yielding F(>1 GeV)≲1.1e-11 ph cm^{-2} s^{-1} and η≲4e-6 (d/kpc)^2, two orders below η Car.
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Searching for Internal Absorption Signatures in High-Redshift Blazars
Fermi-LAT data for nine z≥3 FSRQs show no significant internal BLR absorption except a 1.7σ hint in 4FGL J0733.8+0455, whose gamma-ray emission region is constrained to d/R_BLR≥0.93.
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Modeling the Multiwavelength Emission of 3C 279 during the 14 years of Fermi-LAT Era
A 14-year, 168-epoch SED study of 3C 279 finds that a one-zone leptonic model with varying Doppler factor and electron population can explain the flares, with the emission region outside the BLR in most states.
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Multi-wavelength analysis of FSRQ B2 1348+30B: Constraints on the jet power
A 14.5-year multiwavelength analysis of the blazar B2 1348+30B yields jet power limits of about 2.6e46 to 4.2e48 erg/s, with the heavy-jet estimate far exceeding Eddington luminosity.
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BL Lacertae under the Flare of 2024: Probing Temporal and Spectral Dynamics
The October 2024 flare of BL Lacertae varied on a ~1 hour timescale, and its broadband spectrum is claimed to require a proton-based component at the highest energies.
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Detection of Quasiperiodic Oscillations in the Blazar PKS 0735+178 with TESS
A transient ~11.2-hour optical QPO is detected in blazar PKS 0735+178 at 3-4 sigma significance using TESS sectors 71-72.
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