pyaraucaria is a Python library providing a collection of common routines and command-line tools used in the Araucaria Project and OCA (Observatorio Cerro Armazones) observatory software. It aims to be a lightweight, dependency-focused toolkit for astronomical data processing and observatory operations.
The library requires Python 3.10+.
pip install git+https://github.com/araucaria-project/pyaraucaria.gitgit clone https://github.com/araucaria-project/pyaraucaria.git
cd pyaraucaria
uv sync --all-extrasAdd to your pyproject.toml dependencies:
pyaraucaria = { git = "https://github.com/araucaria-project/pyaraucaria.git"}Warning If your project uses poetry the installed versions of poetry have to be >=2.0.0 for git depenndency to pyaraucaria.
Or directly form PyPi, after checking versions (PyPi releases may lag behind GitHub):
dependencies = [
"pyaraucaria>=2.11.0",
]pyaraucaria.coordinates contains dependency-free, fast routines to parse and format sexagesimal coordinates (RA/Dec).
from pyaraucaria.coordinates import ra_to_decimal, dec_to_sexagesimal
ra = ra_to_decimal('12:30:00') # Returns 187.5
dec = dec_to_sexagesimal(-15.5) # Returns '-15:30:00.000'Lookup for objects/targets parameters using one of its aliases.
Uses Objects.database and TAB.ALL files.
from pyaraucaria.lookup_objects import ObjectsDatabase
od = ObjectsDatabase()
od.lookup_object('lmc105_8_11987')pyaraucaria.date handles conversion between Julian dates, datetime objects, and heliocentric corrections.
pyaraucaria.fits provides utilities for reading and writing FITS files, including header management and array saving.
pyaraucaria.ffs provides optimized routines for star detection in images and basic image statistics (mean, median, noise estimation).
pyaraucaria.focus implements various telescope focusing algorithms (RMS, FWHM, Lorentzian, Laplacian).
pyaraucaria.ephemeris offers calculations for moon illumination, object visibility, and other ephemeris-related data using astropy.
pyaraucaria.ephemeris exposes a clean, object-oriented API for use in your own Python projects.
from astropy.coordinates import EarthLocation
from astropy.time import Time
import astropy.units as u
from ocacal import Sun, Moon, Stars
# Define Observer Location
loc = EarthLocation(lat=-24.6*u.deg, lon=-70.2*u.deg, height=2400*u.m)
# Or use a named site
# loc = EarthLocation.of_site('paranal')Find precise times when the Sun reaches specific altitudes.
sun = Sun(loc)
# Check for horizon (0), -6, and -12 degrees
# Returns a list of event dictionaries sorted by time
events = sun.get_events_by_altitude([0, -6, -12], start_time=Time.now())
for e in events:
print(f"Altitude {e['target_alt']}° at {e['time_utc']} (Az: {e['az']:.1f}°)")Efficiently calculate data for multiple stars using vectorization.
# Define your catalog
catalog = [
{'id': 'Vega', 'ra': 279.23, 'dec': 38.78},
{'id': 'Deneb', 'ra': 310.35, 'dec': 45.28}
]
stars = Stars(loc, catalog)
# Get positions for the next 5 hours in 1-hour steps
times = Time.now() + [0, 1, 2, 3, 4, 5] * u.hour
ephemeris = stars.get_ephemeris(times)
# Result is a dictionary keyed by Star ID
for star_id, data in ephemeris.items():
print(f"--- {star_id} ---")
for point in data:
print(f"Time: {point['time_utc']} | Alt: {point['alt']:.2f}°")pyaraucaria.airmass calculates airmass based on elevation using Kasten and Young's model.
pyaraucaria.reddening provides lookup for interstellar reddening based on coordinate databases (e.g., LMC).
pyaraucaria.dome_eq calculates the required dome azimuth for telescopes on equatorial mounts.
pyaraucaria.obs_plan contains a parser for custom observation plan formats using the lark grammar library.
Query the object database from the command line.
lookup_objects -j hd167003Perform star detection and calculate statistics on a FITS file.
find_stars path/to/image.fits gain=1.2 rn_noise=5.0To run tests:
python -m unittest discover testsThis project is licensed under the LGPL-3.0-or-later License.