Download utils/create_splits.py from AnonAstroData/SBI-16-3D: direct link, hf CLI and curl.
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https://huggingface.co/datasets/AnonAstroData/SBI-16-3D/resolve/main/utils/create_splits.py
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curl -L -o create_splits.py https://huggingface.co/datasets/AnonAstroData/SBI-16-3D/resolve/main/utils/create_splits.py
3.66 kB
| import os | |
| import random | |
| from glob import glob | |
| import json | |
| from huggingface_hub import hf_hub_download | |
| from tqdm import tqdm | |
| import numpy as np | |
| from astropy.io import fits | |
| from astropy.wcs import WCS | |
| import datasets | |
| from datasets import DownloadManager | |
| from fsspec.core import url_to_fs | |
| def get_fits_footprint(fits_path): | |
| """ | |
| Process a FITS file to extract WCS information and calculate the footprint. | |
| Parameters: | |
| fits_path (str): Path to the FITS file. | |
| Returns: | |
| tuple: A tuple containing the WCS footprint coordinates. | |
| """ | |
| with fits.open(fits_path) as hdul: | |
| hdul[1].data = hdul[1].data[0, 0] | |
| wcs = WCS(hdul[1].header) | |
| shape = sorted(tuple(wcs.pixel_shape))[:2] | |
| footprint = wcs.calc_footprint(axes=shape) | |
| coords = list(footprint.flatten()) | |
| return coords | |
| def calculate_pixel_scale(header): | |
| """ | |
| Calculate the pixel scale in arcseconds per pixel from a FITS header. | |
| Parameters: | |
| header (astropy.io.fits.header.Header): The FITS header containing WCS information. | |
| Returns: | |
| Mean of the pixel scales in x and y. | |
| """ | |
| # Calculate the pixel scales in arcseconds per pixel | |
| pixscale_x = header.get('CDELT1', np.nan) | |
| pixscale_y = header.get('CDELT2', np.nan) | |
| return np.mean([pixscale_x, pixscale_y]) | |
| def make_split_jsonl_files(config_type="tiny", data_dir="./data", | |
| outdir="./splits", seed=42): | |
| """ | |
| Create jsonl files for the SBI-16-3D dataset. | |
| config_type: str, default="tiny" | |
| The type of split to create. Options are "tiny" and "full". | |
| data_dir: str, default="./data" | |
| The directory where the FITS files are located. | |
| outdir: str, default="./splits" | |
| The directory where the jsonl files will be created. | |
| seed: int, default=42 | |
| The seed for the random split. | |
| """ | |
| random.seed(seed) | |
| os.makedirs(outdir, exist_ok=True) | |
| fits_files = glob(os.path.join(data_dir, "*.fits")) | |
| random.shuffle(fits_files) | |
| if config_type == "tiny": | |
| train_files = fits_files[:2] | |
| test_files = fits_files[2:3] | |
| elif config_type == "full": | |
| split_idx = int(0.8 * len(fits_files)) | |
| train_files = fits_files[:split_idx] | |
| test_files = fits_files[split_idx:] | |
| else: | |
| raise ValueError("Unsupported config_type. Use 'tiny' or 'full'.") | |
| def create_jsonl(files, split_name): | |
| output_file = os.path.join(outdir, f"{config_type}_{split_name}.jsonl") | |
| with open(output_file, "w") as out_f: | |
| for file in tqdm(files): | |
| #print(file, flush=True, end="...") | |
| with fits.open(file, memmap=False) as hdul: | |
| image_id = os.path.basename(file).split(".fits")[0] | |
| ra = hdul["SCI"].header.get('CRVAL1', 0) | |
| dec = hdul["SCI"].header.get('CRVAL2', 0) | |
| pixscale = calculate_pixel_scale(hdul["SCI"].header) | |
| footprint = get_fits_footprint(file) | |
| read_pattern = hdul[0].header.get('READPATT', 0) | |
| # get the number of groups per int | |
| ntimes = hdul["SCI"].data.shape[1] | |
| item = {"image_id": image_id, "image": file, "ra": ra, "dec": dec, | |
| "pixscale": pixscale, "ntimes": ntimes, "read_pattern": read_pattern, "footprint": footprint} | |
| out_f.write(json.dumps(item) + "\n") | |
| create_jsonl(train_files, "train") | |
| create_jsonl(test_files, "test") | |
| if __name__ == "__main__": | |
| make_split_jsonl_files("tiny") | |
| make_split_jsonl_files("full") |