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mmu_jwst_primer_uds HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_jwst_primer_uds.

This dataset is part of the Multimodal Universe, a large-scale collection of multimodal astronomical data. For full details, see the paper: The Multimodal Universe: Enabling Large-Scale Machine Learning with 100TBs of Astronomical Scientific Data.

Access the catalog

We recommend the use of the LSDB Python framework to access HATS catalogs. LSDB can be installed via pip install lsdb or conda install conda-forge::lsdb, see more details in the docs. The following code provides a minimal example of opening this catalog:

import lsdb

# Full sky coverage.
catalog = lsdb.open_catalog("https://huggingface.co/datasets/UniverseTBD/mmu_jwst_primer_uds")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_jwst_primer_uds",
    search_filter=lsdb.ConeSearch(ra=34.0, dec=-5.0, radius_arcsec=3600.0),
)

Each catalog in this collection is represented as a separate Apache Parquet dataset and can be accessed with a variety of tools, including pandas, pyarrow, dask, Spark, DuckDB.

File structure

This catalog is represented by the following files and directories:

  • collection.properties — textual metadata file describing the HATS collection of catalogs
  • mmu_jwst_primer_uds — main HATS catalog directory
    • dataset/ — Apache Parquet dataset directory for the main catalog
      • ... parquet metadata and data files in sub directories ...
    • hats.properties — textual metadata file describing the main HATS catalog
    • partition_info.csv — CSV file with a list of catalog HEALPix tiles (catalog partitions)
    • skymap.fits — HEALPix skymap FITS file with row-counts per HEALPix tile of fixed order 10
  • mmu_jwst_primer_uds_10arcs/ — default margin catalog to ensure data completeness in cross-matching, the margin threshold is 10.0 arcseconds
    • ... margin catalog files and directories ...

Catalog metadata

Metadata of the main HATS catalog, excluding margins and indexes:

Number of rows Number of columns Number of partitions Size on disk HATS Builder
66,660 11 22 22.7 GiB hats-import v0.7.3, hats v0.7.3

Catalog columns

The main HATS catalog contains the following columns:

Name _healpix_29 image.band image.flux image.ivar image.mask image.psf_fwhm image.scale mag_auto flux_radius flux_auto fluxerr_auto cxx_image cyy_image cxy_image object_id ra dec
Data Type int64 list[string] list[list<element: list<element: float>>] list[list<element: list<element: float>>] list[list<element: list<element: bool>>] list[float] list[float] float float float float float float float string double double
Nested? — image image image image image image — — — — — — — — — —
Value count 66,660 466,620 N/A N/A N/A 466,620 466,620 66,660 66,660 66,660 66,660 66,660 66,660 66,660 66,660 66,660 66,660
Example row 1244081442258414734 [f090w, f115w, f150w, f200w, f277w, … (7 total)] [[[0.1339, 0.1695, 0.01594, -0.01652, … (96 total)], … (96 total)], …… [[[104.3, 99.23, 130.4, 121.7, 108.9, … (96 total)], … (96 total)], …… [[[True, True, True, True, True, True, … (96 total)], … (96 total)], … [0.033, 0.04, 0.05, 0.066, 0.092, … (7 total)] [0.04, 0.04, 0.04, 0.04, 0.04, 0.04, … (7 total)] 24.76 4.374 0.3911 0.004391 0.04621 0.1452 0.009686 5481758738572589643 34.22 -5.207
Minimum value 1244073128803644245 f090w N/A N/A N/A 0.032999999821186066 0.03999999910593033 15.883356094360352 0.5410636067390442 0.04745132848620415 0.000631449802313 1.4279617062129546e-05 2.961887548735831e-05 -1.0529983043670654 -1502803815681653184 34.19782039975754 -5.3373375913611865
Maximum value 1244836278796287736 f444w N/A N/A N/A 0.14499999582767487 0.03999999910593033 26.999980926513672 775.8671875 1609.376708984375 237.3377227783203 3.3322954177856445 1.9879162311553955 2.0581705570220947 5481758738572675269 34.53875468066159 -5.06434849884021

"Nested" indicates whether the column is stored as a nested field inside another "struct" column.

"Value count" may be different from the total number of rows for nested columns: each nested element is counted as a single value.

Crossmatch with another catalog

HATS catalogs can be efficiently crossmatched using LSDB, which leverages the HEALPix partitioning to avoid loading the full datasets into memory:

import lsdb

mmu_jwst_primer_uds = lsdb.open_catalog("https://huggingface.co/datasets/UniverseTBD/mmu_jwst_primer_uds")
other = lsdb.open_catalog("https://huggingface.co/datasets/<org>/<other_catalog>")

crossmatched = mmu_jwst_primer_uds.crossmatch(other, radius_arcsec=1.0)
print(crossmatched)

See the LSDB documentation for more details on crossmatching and other operations.

Dataset-specific context

Original survey
This dataset is based on the James Webb Space Telescope (JWST) NIRCam observations from early deep field surveys.

Data modality
The dataset consists of fixed-size image cutouts (96×96 pixels) centered on sources from photometric catalogs. The images are multi-band, with 6 or 7 filters covering wavelengths from approximately 0.9μm to 4.4μm.

Typical use cases
Images from these JWST deep field surveys have been used in a large number of scientific publications, including machine learning applications.

Caveats
Different surveys have different wavelength coverage, and missing bands are represented as arrays of zeros to simplify data loading.

Citation
The data are in the public domain. The dataset uses data products retrieved from the Dawn JWST Archive (DJA), an initiative of the Cosmic Dawn Center (DAWN).

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