Isolated pulsar timing tools geared towards high energy astrophysical data
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Updated
Aug 7, 2026 - Python
Isolated pulsar timing tools geared towards high energy astrophysical data
AnTi pipeline
Utilizing Fermi GBM as a pulsar timing tool
Fortytwo: Pulsar timing software for noise, gravitational-wave and common-signal analysis
We formalize Noor Swirl Field Geometry as a coherence-driven, pre-geometric framework that unifies quantum gravity and cosmology, introduces the ontology of Point Space, and derives falsifiable observational predictions.
Temporal Equivalence Principle: Suppressed Density Scaling in Globular Cluster Pulsars — Globular cluster pulsar spin-down anomaly: 197 cluster vs 346 field pulsars show 0.40 dex residual (8.3σ). Suppressed density scaling (Γ=0.39±0.08 vs Newtonian Γ=0.72, 4.1σ) tests the TEP observable response coefficient κ_MSP.
Synthetic pulsar-timing inference workflow for compact subhalo parameter estimation.
This is an experimental python script predicts the Time of Arrival (TOA) and gate boundaries for a pulsar for gated imaging applications. Currently, the code is tailored for GMRT observations
Timing Pulsars with the Thousand Pulsar Array on MeerKAT
Federated Time-Reference Observatory walking skeleton (FTRO-WS-001 v0.3): bitemporal reference-clock ancestry across optical clocks, pulsar timing, VLBI and GNSS. Phase 0 complete.
Pulsar timing analysis project using Vela photon event data: period detection, epoch folding, and a simplified XNAV demonstration. The approach is applicable to the tasks of telemetry, IoT and monitoring of complex systems.
Private browser-based research console for NANOGrav pulsar timing data, combining released residual/DMX products with an optional rotational-noise, dispersion-delay, and glitch simulation overlay.
High-precision astrophysical auditing tool that correlates LIGO gravitational wave events with NANOGrav pulsar timing residuals to search for coherent "simulation lag" artifacts — featuring an interactive 8-tab Plotly Dash dashboard with Monte Carlo testing, Bayesian evidence, and Hellings-Downs analysis.
PhD Candidate at the Max Planck Institute for Gravitational Physics in Hannover, Germany
Pulsar timing array data acquisition and reduction, with an Asimov pipeline plugin
Julia orchestrator for reproducible TEMPO/TEMPO2 workflows + pure-Julia adaptive grids
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