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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
2,528,750,302,881,171,500
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
23.362926
6.398422
1.484013
0.006127
0.0508
0.017728
-0.007665
-7567302259786487267
53.168982
-27.863668
2,528,750,303,162,352,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
23.27519
7.935032
1.634318
0.008015
0.025793
0.025566
0.02033
-7567302259786486458
53.170533
-27.862157
2,528,750,304,000,038,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0,0.0,0.0,0.0,0.0,0.0,(...TRUNCATED)
25.069054
9.265326
0.305892
0.006942
0.024848
0.065756
-0.019941
-7567302259786485636
53.171762
-27.860523
2,528,750,308,651,039,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.0013175341300666332,0(...TRUNCATED)
25.416208
3.371781
0.210904
0.001569
0.101927
0.088415
0.003152
-7567302259786487000
53.168353
-27.863019
2,528,750,308,674,055,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.012485136277973652,0.(...TRUNCATED)
27.149031
2.218172
0.041365
0.001208
0.249478
0.277418
0.004609
-7567302259786486999
53.167919
-27.862961
2,528,750,308,755,582,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.008271699771285057,-0.(...TRUNCATED)
26.514816
2.482898
0.074185
0.001219
0.146716
0.219323
-0.006259
-7567302259786486514
53.168992
-27.862096
2,528,750,308,845,406,700
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.015459511429071426,0.0(...TRUNCATED)
20.850353
4.765753
14.696917
0.002328
0.030057
0.018907
0.009943
-7567302259786486178
53.168419
-27.861856
2,528,750,308,981,540,000
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.028007248416543007,0.0(...TRUNCATED)
27.288443
3.158828
0.03638
0.001337
0.238352
0.294734
-0.072931
-7567302259786486005
53.170247
-27.861321
2,528,750,308,983,089,700
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[0.0014625698095187545,-0(...TRUNCATED)
25.786896
3.176177
0.147597
0.001409
0.120125
0.131587
0.024242
-7567302259786486004
53.170247
-27.861201
2,528,750,309,014,724,600
{"band":["f090w","f115w","f150w","f200w","f277w","f356w","f444w"],"flux":[[[-0.009114574640989304,0.(...TRUNCATED)
25.359226
4.112514
0.222977
0.001638
0.134256
0.061251
0.049515
-7567302259786485688
53.170197
-27.860743
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mmu_jwst_gds HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_jwst_gds.

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_gds")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_jwst_gds",
    search_filter=lsdb.ConeSearch(ra=53.0, dec=-28.0, 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_gds — 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_gds_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
17,494 11 8 6.3 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 17,494 122,458 N/A N/A N/A 122,458 122,458 17,494 17,494 17,494 17,494 17,494 17,494 17,494 17,494 17,494 17,494
Example row 2528743702220181960 [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)] [0.02, 0.02, 0.02, 0.02, 0.04, 0.04, … (7 total)] 25.85 4.665 0.1431 0.0007781 0.05192 0.07733 -0.03422 -7567302259786491648 53.17 -27.87
Minimum value 2528743693306351542 f090w N/A N/A N/A 0.032999999821186066 0.019999999552965164 17.325851440429688 0.6315596699714661 0.02997756563127041 0.00019976860494352877 7.402321352856234e-05 2.9240540243336e-05 -1.2243539094924927 -7567302259786424111 53.051927973650635 -27.87760950265767
Maximum value 2528752620411181000 f444w N/A N/A N/A 0.14499999582767487 0.03999999910593033 27.499950408935547 276.15155029296875 415.23297119140625 0.3415043354034424 2.141709089279175 1.9386420249938965 1.0062775611877441 -7567302259786494449 53.22671287579358 -27.723125018856216

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

crossmatched = mmu_jwst_gds.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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