astroeasy 1.2.0

Astrometry.net made easy - plate solving and index management

astroeasy

Astrometry.net made easy - a standalone Python package for plate-solving with containerized execution, clean API, and indices management.

Installation

pip install astroeasy

Optional extras (only if you need them — the core install is unchanged):

pip install "astroeasy[catalog]"   # online Gaia queries (astroquery)
pip install "astroeasy[cascade]"   # catalog-native fast solving (see below)

Quick Start

from astroeasy import (
    AstrometryConfig,
    Detection,
    ImageMetadata,
    solve_field,
)

# Configure astrometry.net
config = AstrometryConfig(
    indices_path="/data/indices/5200-LITE",
    docker_image="astrometry-cli",  # Or None for local installation
)

# Your detected sources (x, y pixel coordinates with optional flux)
detections = [
    Detection(x=100, y=200, flux=1000),
    Detection(x=500, y=300, flux=800),
    # ... more detections
]

# Image metadata
metadata = ImageMetadata(width=4096, height=4096)

# Solve!
result = solve_field(detections, metadata, config)

if result.success:
    print(f"Solved! Center: {result.wcs.center_ra:.4f}, {result.wcs.center_dec:.4f}")
    print(f"Pixel scale: {result.wcs.pixel_scale:.3f} arcsec/pix")
    print(f"Matched {len(result.matched_stars)} catalog stars")

Setup

Option 1: Docker (Recommended)

Build the astrometry.net container:

cd astroeasy/dotnet
docker build -t astrometry-cli .

Verify installation:

astroeasy test-install --docker astrometry-cli

Option 2: Local Installation

If you have astrometry.net installed locally:

astroeasy test-install --local

Index Files

Astrometry.net requires index files for plate solving. We recommend the 5200_LITE series (~15 GB) for most use cases.

Download Indices

astroeasy indices download --series 5200_LITE --output /data/indices/5200-LITE

Verify Indices

astroeasy indices examine --series 5200_LITE --path /data/indices/5200-LITE

FOV-Filtered Downloads

Download only the index files needed for your camera's field of view (saves significant disk space).

--fov is the field of view on a side, in degrees — so --fov 2.0 means a 2°×2° field (4 square degrees) on a square detector. Filtered downloads land in an automatic subdirectory of --output named <series>_<fov>deg (e.g. 4200_2p0deg) so they can't be mixed up with a full series download:

# 1-degree (1°x1°) FOV camera (~4.9 GB instead of ~35 GB for 5200_LITE_4100)
# -> downloads to /data/indices/5200_LITE_4100_1p0deg
astroeasy indices download --series 5200_LITE_4100 --output /data/indices --fov 1.0

# 2-degree (2°x2°) FOV camera (~1.3 GB instead of ~32 GB for 4200)
# -> downloads to /data/indices/4200_2p0deg
astroeasy indices download --series 4200 --output /data/indices --fov 2.0

Validate a filtered set by passing the same --fov to examine:

astroeasy indices examine --series 4200 --path /data/indices/4200_2p0deg --fov 2.0

Supported Index Series

Series	Size	Description
5200_LITE	~36 GB	Recommended - good balance of coverage and size
5200	~80 GB	Full 5200 series with photometry
4100	~0.4 GB	Smaller, for wider fields
4200	~32 GB	Alternative to 4100
5200_LITE_4100	~35 GB	Combined 5200_LITE + 4100

CLI Reference

Plate Solving

# Solve with configuration file
astroeasy solve --config astrometry.yaml --image image.fits

# Solve with explicit parameters
astroeasy solve --xylist sources.csv --width 4096 --height 4096 \
    --indices-path /data/indices/5200-LITE \
    --docker-image astrometry-cli

Index Management

# Download indices
astroeasy indices download --series 5200_LITE --output /data/indices

# Check index completeness
astroeasy indices examine --series 5200_LITE --path /data/indices

# List supported series
astroeasy indices --help

Installation Verification

# Test Docker installation
astroeasy test-install --docker astrometry-cli

# Test local installation
astroeasy test-install --local

Fast Solving (cascade)

Optional and fully additive. Everything above is unchanged. If you use astroeasy for astrometry.net plate solving, you can ignore this section — the cascade lives behind pip install "astroeasy[cascade]" and the astroeasy.cascade namespace, and solve_field behaves exactly as before whether or not the extra is installed.

For a fixed camera that solves many frames, the cascade trades a one-time setup for sub-second, network-free solves. It escalates cheapest-first and only ever returns a solution that clears a likelihood-based acceptance gate (so a confident-but-wrong match is rejected, not returned):

• T0 — refine from a prior/propagated WCS or a boresight hint (fastest).
• T1 — tetra3 lost-in-space pattern match against a local pattern DB (vendored; see astroeasy/_vendor/README.md).
• T3/T4 — the standard solve_field astrometry.net backstop (hinted, then blind). The cascade never fails a frame astrometry.net would have solved.

The native tiers read stars from a local Gaia mirror (HEALPix-tiled binary, queried offline) rather than the network. Build the mirror with your own Gaia export; the readers live in astroeasy.catalog.mirror.

One-time setup per sensor

# Characterize a sensor from a few blind-solved sidereal frames: measures
# scale / FoV / rotation / depth, writes a SensorProfile, and builds the
# tetra3 pattern DB. (Needs stock indices for the blind pass + a Gaia mirror.)
astroeasy characterize frame1.fits frame2.fits frame3.fits \
    --sensor-id dao01 --out profiles/ \
    --indices-path /data/indices/4200 --mirror /data/gaia-mirror

# Or build artifacts directly:
astroeasy build-tetra3-db --mirror /data/gaia-mirror --out dao01.npz --fov 2.0
astroeasy build-index     --mirror /data/gaia-mirror --out dao01_index/ --fov 2.0 --depth 16

Solving

from astroeasy.cascade import solve
from astroeasy.cascade.profile import SensorProfile

profile = SensorProfile.from_yaml("profiles/dao01.yaml")
result = solve(
    detections, metadata,
    profile=profile,
    mirror_dir="/data/gaia-mirror",      # enables the native tiers + gate
    dotnet_config=config,                # the astrometry.net backstop (optional)
    prior_wcs=previous_solution,         # enables the fast T0 path (optional)
)

if result.solve.success:
    print(f"solved via {result.tier}: {result.solve.wcs.center_ra:.4f}, "
          f"{result.solve.wcs.center_dec:.4f}")
# result.attempts holds per-tier telemetry (gate scores, timings)

solve() returns a CascadeResult wrapping a standard SolveResult (.solve) plus the winning .tier and per-tier .attempts. With no mirror, no profile artifacts, and only a dotnet_config, it degrades to a plain astrometry.net solve. See docs/catalog-native-solving-roadmap.md for the design.

Configuration

YAML Configuration File

# astrometry.yaml
indices_path: /data/indices/5200-LITE
indices_series: 5200_LITE
docker_image: astrometry-cli  # null for local execution
cpulimit_seconds: 30
min_width_degrees: 0.1
max_width_degrees: 10.0
tweak_order: 2
max_sources: 100
min_sources_for_attempt: 4

Python Configuration

from astroeasy import AstrometryConfig

config = AstrometryConfig(
    indices_path="/data/indices/5200-LITE",
    docker_image="astrometry-cli",
    cpulimit_seconds=60,
    min_width_degrees=0.5,
    max_width_degrees=5.0,
)

# Load from YAML
config = AstrometryConfig.from_yaml("astrometry.yaml")

# Save to YAML
config.to_yaml("astrometry.yaml")

API Reference

Models

from astroeasy import Detection, ImageMetadata, WCSResult, SolveResult

# Detection - a source in pixel coordinates
detection = Detection(x=100.5, y=200.3, flux=1000.0)

# ImageMetadata - image dimensions and optional hints
metadata = ImageMetadata(
    width=4096,
    height=4096,
    boresight_ra=180.0,   # Optional RA hint (degrees)
    boresight_dec=45.0,   # Optional Dec hint (degrees)
)

# SolveResult - the result of plate solving
result = solve_field(detections, metadata, config)
result.success       # bool
result.status        # WCSStatus enum
result.wcs           # WCSResult or None
result.matched_stars # list[MatchedStar]

# WCSResult - WCS solution
result.wcs.center_ra   # RA at reference pixel (degrees)
result.wcs.center_dec  # Dec at reference pixel (degrees)
result.wcs.pixel_scale # Approximate pixel scale (arcsec/pix)
result.wcs.to_astropy_wcs()  # Convert to astropy WCS

Functions

from astroeasy import solve_field, test_install, examine_indices, download_indices

# Plate solve
result = solve_field(detections, metadata, config)

# Test installation
is_working = test_install(docker_image="astrometry-cli")
is_working = test_install()  # Local

# Index management
is_complete = examine_indices("/data/indices", series="5200_LITE")
download_indices("/data/indices", series="5200_LITE")

Legacy Python Module Usage

The package can also be invoked as Python modules:

# Test local installation
python -m astroeasy.dotnet.local

# Test Docker installation
python -m astroeasy.dotnet.docker

# Index management
python -m astroeasy.indices examine --series 5200_LITE --index_path /data/indices
python -m astroeasy.indices download --series 5200_LITE --index_path /data/indices

License

MIT