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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
1,918,128,957,852,083,500
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
26.911093
3.589572
0.0515
0.005171
0.513252
0.624147
0.222822
-1793941820439718330
150.14008
2.143476
1,918,128,958,002,657,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
20.694067
40.107693
18.694893
0.0372
0.006949
0.008871
0.014979
-1793941820439717389
150.1384
2.143163
1,918,128,958,076,590,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
25.461721
5.547605
0.198952
0.005556
0.153027
0.144123
0.006753
-1793941820439718351
150.136882
2.143268
1,918,128,958,078,720,800
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
25.895924
3.792562
0.131434
0.005058
0.157264
0.224739
0.084428
-1793941820439718350
150.136846
2.143332
1,918,128,958,123,012,400
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
23.120605
7.196118
1.820781
0.010974
0.045734
0.036392
0.046453
-1793941820439718291
150.137615
2.143606
1,918,128,958,134,758,700
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
24.861403
5.764541
0.347105
0.005878
0.176126
0.179402
0.222842
-1793941820439718292
150.137783
2.143661
1,918,128,958,180,921,300
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
26.628628
3.450473
0.066802
0.005407
0.531239
0.344739
0.323295
-1793941820439718300
150.139493
2.143667
1,918,128,958,184,875,300
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
23.316284
11.519317
1.562246
0.013762
0.014161
0.062471
0.019098
-1793941820439717387
150.1395
2.143894
1,918,128,958,204,591,400
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
19.94677
186.182648
38.132221
0.085478
0.013817
0.016024
0.029738
-1793941820439717388
150.139065
2.143784
1,918,128,958,247,224,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
25.10858
4.070457
0.278513
0.017701
0.11747
0.11303
-0.000666
-1793941820439718230
150.14007
2.144281
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mmu_jwst_primer_cosmos HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_jwst_primer_cosmos.

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_cosmos")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_jwst_primer_cosmos",
    search_filter=lsdb.ConeSearch(ra=150.0, dec=2.0, 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 β€” textual metadata file describing the HATS collection of catalogs
  • mmu_jwst_primer_cosmos β€” main HATS catalog directory
    • dataset/ β€” Apache Parquet dataset directory for the main catalog
      • ... parquet metadata and data files in sub directories ...
    • hats.properties β€” textual metadata file describing the main HATS catalog
    • partition_info.csv β€” CSV file with a list of catalog HEALPix tiles (catalog partitions)
    • skymap.fits β€” HEALPix skymap FITS file with row-counts per HEALPix tile of fixed order 10
  • mmu_jwst_primer_cosmos_10arcs/ β€” 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
51,058 11 15 15.1 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? β€” image image image image image image β€” β€” β€” β€” β€” β€” β€” β€” β€” β€”
Value count 51,058 357,406 N/A N/A N/A 357,406 357,406 51,058 51,058 51,058 51,058 51,058 51,058 51,058 51,058 51,058 51,058
Example row 1918117816734487009 [f090w, f115w, f150w, f200w, f277w, … (7 total)] [[[0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, … (96 total)], … (96 total)], … [[[0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, … (96 total)], … (96 total)], … [[[False, False, False, False, False, … (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)] 26.48 2.555 0.07643 0.003804 0.2659 0.3691 0.1555 4779921206430939062 150 2.158
Minimum value 1918035224610977248 f090w N/A N/A N/A 0.032999999821186066 0.03999999910593033 15.154260635375977 1.093169927597046 0.04745382070541382 0.0009272033930756152 5.68464383832179e-06 1.775023883965332e-05 -1.4645973443984985 -1793941820439658733 150.0225356463053 2.142978850173105
Maximum value 1918143149034739361 f444w N/A N/A N/A 0.14499999582767487 0.03999999910593033 26.99997901916504 558.0476684570312 3149.892578125 46.66569519042969 2.4375405311584473 1.9571294784545898 1.3657711744308472 4779921206430994078 150.22745237191987 2.506566292130767

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

crossmatched = mmu_jwst_primer_cosmos.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 (96Γ—96 pixels) centered on sources from photometric catalogs. The images are multi-band, with 6 or 7 filters covering wavelengths from approximately 0.9ΞΌm to 4.4ΞΌm.

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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