11 releases

0.2.8 May 22, 2023
0.2.7 May 22, 2023
0.2.6 Apr 26, 2023
0.2.4 Mar 23, 2023
0.1.1 Jan 26, 2023

#388 in Algorithms

22 downloads per month

Apache-2.0 OR MIT

55KB
988 lines

WCS parsing library written in pure Rust

API Documentation on docs.rs

This crate must be used conjointly with fitsrs It takes a FITS header and parse it to define a WCS. A WCS object allow two operations:

  • The projection of a (lon, lat) tuple given in degrees into the image space XY (in pixels)
  • The unprojection of a vertex in the image space into a tuple (lon, lat) on the sphere This crate heavily relies on the work done by F.-X. Pineau (@fxpineau) for the mapproj crate

The reference for the FITS WCS standard for undistorted celestial coordinate systems is Representations of celestial coordinates in FITS Calabretta, M. R., and Greisen, E. W., Astronomy & Astrophysics, 395, 1077-1122, 2002

To Do list

  • Add conic projections (COD, COE, COO, COP)
  • Add cylindrical projections (CAR, CEA, CYP, MER)
  • Add hybrid projection (HPX)
  • Add pseudo cylindrical projections (AIT, MOL, PAR, SFL)
  • Add zenithal projections (AIR, ARC, AZP, SIN, STG, SZP, TAN, ZEA, ZPN)
  • Zenithal projections not supported (FEYE, NCP)
  • Add polyconic and pseudoconic projections (BON, PCO)?
  • Add quad cube projections (TSC, CSC, QSC)?
  • Check and possibly document constants to be added to match WCS projection bounds
  • Support CRPIX + CD convention
  • Support CRPIX + PC + CDELT convention
  • Support CRPIX + CROTA + CDELT convention
  • Add support for LONPOLE?
  • SIP convention support
  • SIP not tested
  • TPV World Coordinate System non-standard convention
  • Add generation of projection files and plots (partially done)

Example

use std::fs::File;
use std::io::BufReader;

use fitsrs::Fits;
use wcsrs::{
    WCS,
    ImgXY, LonLat
};

fn main() {
    // 1. Parse a fits file using fitsrs
    let mut f = File::open("<your fits file path>").unwrap();
    let mut reader = BufReader::new(f);
    let Fits { hdu } = Fits::from_reader(&mut reader).unwrap();

    let header = hdu.get_header();
    // Get the crval and crpix values along each axes
    let crval1 = header
        .get_parsed::<f64>(b"CRVAL1  ")
        .unwrap_or(Ok(0.0))
        .unwrap();
    let crval2 = header
        .get_parsed::<f64>(b"CRVAL2  ")
        .unwrap_or(Ok(0.0))
        .unwrap();
    let crpix1 = header
        .get_parsed::<f64>(b"CRPIX1  ")
        .unwrap_or(Ok(0.0))
        .unwrap();
    let crpix2 = header
        .get_parsed::<f64>(b"CRPIX2  ")
        .unwrap_or(Ok(0.0))
        .unwrap();

    // 2. Create a WCS from a specific header unit
    let wcs = WCS::new(&header).unwrap();

    // 3. Once the WCS object is created, performs:
    // * The projection of the center (lon, lat) = (crval1, crval2)
    let lonlat = LonLat::new(crval1.to_radians(), crval2.to_radians());
    let xy = wcs
        .proj_lonlat(&lonlat)
        .unwrap();
    assert_delta!(xy.x(), crpix1 - 1.0, 1e-6);
    assert_delta!(xy.y(), crpix2 - 1.0, 1e-6);

    // * The unprojection of (X, Y) = (crpix1, crpix2)
    let xy = ImgXY::new(crpix1 - 1.0, crpix2 - 1.0);
    let lonlat = wcs
        .unproj_lonlat(&xy)
        .unwrap();
    assert_delta!(lonlat.lon(), crval1.to_radians(), 1e-6);
    assert_delta!(lonlat.lat(), crval2.to_radians(), 1e-6);
}

Dependencies

~2.6–4MB
~75K SLoC