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_healpix_29
int64
image
dict
mag_auto
float32
flux_radius
float32
flux_auto
float32
fluxerr_auto
float32
cxx_image
float32
cyy_image
float32
cxy_image
float32
object_id
string
ra
float64
dec
float64
804,018,977,499,831,600
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.0270996056497097,-0.0(...TRUNCATED)
26.396162
3.79354
0.084921
0.001467
0.179037
0.082052
0.028201
1757963689505804547
215.048338
52.996059
804,018,977,507,967,400
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.043169647455215454,-0.(...TRUNCATED)
25.190783
6.253964
0.26862
0.002271
0.069881
0.036206
0.016975
1757963689505804513
215.048932
52.99619
804,018,977,557,908,200
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.031696759164333344,0.(...TRUNCATED)
21.814142
6.515933
6.237586
0.003118
0.014127
0.018947
-0.004031
1757963689505804514
215.049304
52.996547
804,018,977,642,280,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0008344646776095033,0.(...TRUNCATED)
26.751333
4.50507
0.060949
0.001736
0.127673
0.097406
-0.09131
1757963689505803767
215.051337
52.996968
804,018,977,681,408,500
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,-0.0196848325431(...TRUNCATED)
22.639841
9.512934
2.874316
0.010836
0.054295
0.02597
-0.004323
1757963689505803667
215.052865
52.997684
804,018,977,841,872,800
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.003209212329238653,-0.(...TRUNCATED)
26.057745
3.293733
0.115512
0.001704
0.107947
0.168231
-0.044204
1757963689505804953
215.050418
52.998655
804,018,977,905,195,500
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.03919825330376625,-0.(...TRUNCATED)
25.981054
3.180061
0.121288
0.001165
0.116337
0.122431
-0.017337
1757963689505805264
215.047235
52.996957
804,018,977,948,666,600
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.02888817898929119,-0.(...TRUNCATED)
25.370157
4.262614
0.221568
0.001693
0.12398
0.050373
-0.010004
1757963689505805001
215.049273
52.997569
804,018,977,956,702,700
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.1343301385641098,-0.0(...TRUNCATED)
26.774261
3.483444
0.059409
0.001309
0.171224
0.128301
0.019655
1757963689505805002
215.048949
52.997681
804,018,978,014,015,600
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.015589146874845028,-0(...TRUNCATED)
24.454128
6.965165
0.542881
0.002726
0.044586
0.019894
-0.027448
1757963689505806609
215.047255
52.997482
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mmu_jwst_ceers HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_jwst_ceers.

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_ceers")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_jwst_ceers",
    search_filter=lsdb.ConeSearch(ra=215.0, dec=53.0, 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_ceers — 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_ceers_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
24,518 11 9 8.2 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 24,518 171,626 N/A N/A N/A 171,626 171,626 24,518 24,518 24,518 24,518 24,518 24,518 24,518 24,518 24,518 24,518
Example row 804002297459820835 [f090w, f115w, f150w, f200w, f277w, … (7 total)] [[[0.01465, 0.03999, 0.0095, … (96 total)], … (96 total)], … (7 total… [[[1606, 1537, 1521, 1697, 1743, 1692, … (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)] 21.62 2.014 6.875 0.0014 0.0496 0.06944 -0.001268 1757963689505803332 214.7 52.75
Minimum value 804001887516808636 f090w N/A N/A N/A 0.032999999821186066 0.03999999910593033 17.203704833984375 1.6584279537200928 0.047454044222831726 0.0005687509546987712 1.5739618902443908e-05 3.137264502584003e-05 -2.257167339324951 1757963689505748225 214.69148780378492 52.72084420518769
Maximum value 804019014425927361 f444w N/A N/A N/A 0.14499999582767487 0.03999999910593033 26.99991798400879 336.2449645996094 476.9996032714844 18.44452667236328 1.9025871753692627 1.8590304851531982 0.965598464012146 1757963689505829844 215.17615155042228 53.02129352482981

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

crossmatched = mmu_jwst_ceers.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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