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Python package for INTEGRAL IBIS/ISGRI lightcurve analysis

Project description

ISGRI

Python toolkit for INTEGRAL/ISGRI data analysis.

Features

Command Line Interface

Query catalogs directly from the terminal:

  • Filter by time, position, quality, revolution
  • Export results to FITS/CSV
  • List SWIDs for batch processing

SCW Catalog Query

Query INTEGRAL Science Window catalogs with a fluent Python API:

  • Filter by time, position, quality, revolution
  • Calculate detector offsets
  • Export results to FITS/CSV

Light Curve Analysis

Extract and analyze ISGRI light curves:

  • Event loading with PIF weighting
  • Custom time binning
  • Module-by-module analysis
  • Quality metrics (chi-squared tests)
  • Time conversions (IJD to/from UTC)

Installation

pip install isgri

Quick Start

CLI Usage

# Configure default paths (once)
isgri config-set --catalog ~/data/scw_catalog.fits

# Query by time range
isgri query --tstart 2010-01-01 --tstop 2010-12-31

# Query Crab with quality cut
isgri query --ra 83.63 --dec 22.01 --max-chi 2.0 --fov full

# Get list of SWIDs for processing
isgri query --tstart 3000 --tstop 3100 --list-swids > swids.txt

# Export results
isgri query --tstart 3000 --tstop 3100 --output results.fits

Query SCW Catalog

from isgri.catalog import ScwQuery

# Load catalog
cat = ScwQuery("path_to_catalog.fits")

# Find Crab observations in 2010 with good quality
results = (cat
    .time(tstart="2010-01-01", tstop="2010-12-31")
    .quality(max_chi=2.0)
    .position(ra=83.63, dec=22.01, fov_mode="full")
    .get()
)

print(f"Found {len(results)} observations")

Analyze Light Curves

from isgri.utils import LightCurve, QualityMetrics

# Load events with PIF weighting
lc = LightCurve.load_data(
    events_path="isgri_events.fits",
    pif_path="source_model.fits",
    pif_threshold=0.5
)

# Create 1-second binned light curve
time, counts = lc.rebin(binsize=1.0, emin=20, emax=100)

# Compute quality metrics
qm = QualityMetrics(lc, binsize=1.0, emin=20, emax=100)
chi = qm.raw_chi_squared()
print(f"Chisq/dof = {chi:.2f}")

Configuration

ISGRI stores configuration in default config folder for each system (see: platformdirs package)

# View current config
isgri config

# Set paths
isgri config-set --archive /path/to/archive --catalog /path/to/catalog.fits

Config can also be used in Python:

from isgri.config import get_config

cfg = get_config()
print(cfg.archive_path)
print(cfg.catalog_path)

Local config file isgri_config.toml in current directory overrides global config.

Documentation

Project Structure

isgri/
├── catalog/          # SCW catalog query tools
│   ├── scwquery.py   # Main query interface
│   └── wcs.py        # Coordinate transformations
├── utils/            # Light curve analysis utilities
│   ├── lightcurve.py # Light curve class
│   ├── quality.py    # Quality metrics
│   ├── pif.py        # PIF tools
│   ├── file_loaders.py
│   └── time_conversion.py
├── config.py         # Configuration management
└── cli.py            # Command line interface

Requirements

  • Python ≥ 3.10
  • astropy
  • numpy

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