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_healpix_29
int64
image
dict
a_g
float32
a_r
float32
a_i
float32
a_z
float32
a_y
float32
g_extendedness_value
float32
r_extendedness_value
float32
i_extendedness_value
float32
z_extendedness_value
float32
y_extendedness_value
float32
g_cmodel_mag
float32
g_cmodel_magerr
float32
r_cmodel_mag
float32
r_cmodel_magerr
float32
i_cmodel_mag
float32
i_cmodel_magerr
float32
z_cmodel_mag
float32
z_cmodel_magerr
float32
y_cmodel_mag
float32
y_cmodel_magerr
float32
g_sdssshape_psf_shape11
float32
g_sdssshape_psf_shape22
float32
g_sdssshape_psf_shape12
float32
r_sdssshape_psf_shape11
float32
r_sdssshape_psf_shape22
float32
r_sdssshape_psf_shape12
float32
i_sdssshape_psf_shape11
float32
i_sdssshape_psf_shape22
float32
i_sdssshape_psf_shape12
float32
z_sdssshape_psf_shape11
float32
z_sdssshape_psf_shape22
float32
z_sdssshape_psf_shape12
float32
y_sdssshape_psf_shape11
float32
y_sdssshape_psf_shape22
float32
y_sdssshape_psf_shape12
float32
g_sdssshape_shape11
float32
g_sdssshape_shape22
float32
g_sdssshape_shape12
float32
r_sdssshape_shape11
float32
r_sdssshape_shape22
float32
r_sdssshape_shape12
float32
i_sdssshape_shape11
float32
i_sdssshape_shape22
float32
i_sdssshape_shape12
float32
z_sdssshape_shape11
float32
z_sdssshape_shape22
float32
z_sdssshape_shape12
float32
y_sdssshape_shape11
float32
y_sdssshape_shape22
float32
y_sdssshape_shape12
float32
ra
float64
dec
float64
object_id
string
713,959,823,852,017,300
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0.036729
0.025801
0.018512
0.014318
0.012186
1
1
1
1
1
23.57872
0.029127
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0.02545
22.470736
0.022609
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0.041115
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0.00936
0.096748
0.104854
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0.001566
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-0.001253
0.122316
0.100335
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0.127188
0.148077
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0.009033
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0.290117
0.299273
0.040846
244.007026
53.391454
74701399811696099
713,959,824,164,611,500
{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[-0.03560321778059006,0.01697284355759620(...TRUNCATED)
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{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[0.012548841536045074,-0.0677550733089447(...TRUNCATED)
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1
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-0.025472
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-0.027316
244.002942
53.405185
74701399811696385
713,959,881,442,108,900
{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[-0.037616658955812454,-0.060279320925474(...TRUNCATED)
0.037473
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0.018887
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1
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1
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1
23.571358
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21.087294
0.023667
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0.05727
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244.005094
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{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[0.017568612471222878,0.0550166554749012,(...TRUNCATED)
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23.801575
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22.513254
0.011517
20.822948
0.002839
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0.006174
0.046765
0.058526
0.002564
0.0948
0.103236
-0.004794
0.060145
0.052492
0.002258
0.064217
0.062635
-0.003996
0.128769
0.099021
0.001719
0.049327
0.059932
0.005765
0.098566
0.103193
-0.002674
0.059261
0.052631
0.001742
0.062945
0.063225
-0.004068
0.127916
0.100915
0.003603
244.020035
53.410421
74701399811696631
713,959,884,588,131,700
{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[0.06552830338478088,0.15365546941757202,(...TRUNCATED)
0.037987
0.026685
0.019146
0.014808
0.012604
1
1
1
1
1
22.687286
0.010265
21.990005
0.01008
21.675776
0.009391
21.392231
0.022175
21.677366
0.039741
0.046744
0.058472
0.002557
0.094834
0.103241
-0.004783
0.060179
0.052505
0.00227
0.064239
0.062676
-0.003988
0.128829
0.099079
0.001776
0.187987
0.209654
-0.012622
0.234209
0.242516
-0.017455
0.181689
0.157642
-0.005399
0.188006
0.174376
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244.020593
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1,246,371,216,093,014,800
{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[-0.006217591464519501,0.0150287337601184(...TRUNCATED)
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1
1
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1
1
23.387188
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-0.000289
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0.097221
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0.103667
-0.00039
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-0.000354
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0.06152
0.578342
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0.556629
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33.763531
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1,246,371,217,746,173,700
{"band":["hsc-g","hsc-r","hsc-i","hsc-z","hsc-y"],"flux":[[[-0.015146964229643345,0.0028905812650918(...TRUNCATED)
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23.797316
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mmu_hsc_pdr3_dud_22.5 HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_hsc_pdr3_dud_22.5.

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_hsc_pdr3_dud_22.5")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_hsc_pdr3_dud_22.5",
    search_filter=lsdb.ConeSearch(ra=242.0, dec=55.0, 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_hsc_pdr3_dud_22.5 � 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_hsc_pdr3_dud_22.5_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
474,954 54 156 335.6 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 a_g a_r a_i a_z a_y g_extendedness_value r_extendedness_value i_extendedness_value z_extendedness_value y_extendedness_value g_cmodel_mag g_cmodel_magerr r_cmodel_mag r_cmodel_magerr i_cmodel_mag i_cmodel_magerr z_cmodel_mag z_cmodel_magerr y_cmodel_mag y_cmodel_magerr g_sdssshape_psf_shape11 g_sdssshape_psf_shape22 g_sdssshape_psf_shape12 r_sdssshape_psf_shape11 r_sdssshape_psf_shape22 r_sdssshape_psf_shape12 i_sdssshape_psf_shape11 i_sdssshape_psf_shape22 i_sdssshape_psf_shape12 z_sdssshape_psf_shape11 z_sdssshape_psf_shape22 z_sdssshape_psf_shape12 y_sdssshape_psf_shape11 y_sdssshape_psf_shape22 y_sdssshape_psf_shape12 g_sdssshape_shape11 g_sdssshape_shape22 g_sdssshape_shape12 r_sdssshape_shape11 r_sdssshape_shape22 r_sdssshape_shape12 i_sdssshape_shape11 i_sdssshape_shape22 i_sdssshape_shape12 z_sdssshape_shape11 z_sdssshape_shape22 z_sdssshape_shape12 y_sdssshape_shape11 y_sdssshape_shape22 y_sdssshape_shape12 ra dec object_id
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 float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float float double double string
Nested? image image image image image image
Value count 474,954 2,374,770 N/A N/A N/A 2,374,770 2,374,770 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954 474,954
Example row 714608920907664824 [hsc-g, hsc-r, hsc-i, hsc-z, hsc-y] [[[0.01553, 0.01353, 0.04066, � (160 total)], � (160 total)], � (5 to� [[[6186, 6202, 6196, 6281, 6295, � (160 total)], � (160 total)], � (5� [[[True, True, True, True, True, � (160 total)], � (160 total)], � (5� [0.6551, 0.7859, 0.584, 0.6869, � (5 total)] [0.168, 0.168, 0.168, 0.168, 0.168] 0.02099 0.01475 0.01058 0.008184 0.006966 1 1 1 1 1 22.12 0.002044 21.82 0.002492 21.62 0.002321 21.52 0.004113 21.45 0.009543 0.07804 0.07675 -0.001801 0.1104 0.1124 -0.0007987 0.06518 0.05811 0.002674 0.08575 0.08443 -0.001878 0.09401 0.09101 0.004777 0.1922 0.204 0.05422 0.2435 0.2615 0.05549 0.1893 0.196 0.0582 0.2264 0.2352 0.05529 0.2284 0.2484 0.05748 242.2 54.85 75339253994786944
Minimum value 713959823852017263 hsc-g N/A N/A N/A -0.0 0.1679999977350235 0.014865555800497532 0.010442594066262245 0.007492423988878727 0.005794813856482506 0.004932244773954153 -0.0 -0.0 -0.0 -0.0 -0.0 13.40178108215332 5.988774501020089e-05 15.156841278076172 4.929747592541389e-05 12.742855072021484 3.227664274163544e-05 14.046401977539062 3.8605219742748886e-05 11.048727035522461 5.5523487390019e-05 0.002351417439058423 0.0023516854271292686 -1.1424497365951538 0.03563915193080902 0.007416512351483107 -0.3677349090576172 0.026111777871847153 0.031780991703271866 -0.4359694719314575 0.020980196073651314 0.03532128408551216 -0.4710213541984558 0.03327632322907448 0.03366565331816673 -0.02028796635568142 0.0015113428235054016 0.000953439564909786 -27798.8203125 0.0003241318336222321 0.0019716571550816298 -6958.20068359375 -0.3635726273059845 0.002350886119529605 -10027.140625 -8.943077087402344 0.00019998368225060403 -4239.42626953125 -0.002925257198512554 0.0018239404307678342 -13199.34375 33.606262488492874 -6.082362086730274 36429191050166698
Maximum value 1924448822636503838 hsc-z N/A N/A N/A 4.95881462097168 0.1679999977350235 0.20999060571193695 0.14751191437244415 0.1058378592133522 0.08185745030641556 0.06967281550168991 1.0 1.0 1.0 1.0 1.0 inf inf inf inf 22.499998092651367 inf inf inf inf inf 1.708125114440918 1.8359121084213257 0.08827947825193405 1.164284586906433 0.4658052623271942 0.7985565066337585 4.0367865562438965 4.870001316070557 0.03867558762431145 1.1716283559799194 1.332167387008667 0.059275317937135696 0.29171323776245117 0.32067495584487915 0.13825233280658722 28392.671875 37255.6015625 2947.21435546875 12577.33984375 16102.716796875 2831.651123046875 21279.3046875 15267.2314453125 3927.672607421875 1384974.125 243522.625 917168.0 16140.8369140625 13590.5048828125 6681.443359375 353.9145417236136 56.82558416535321 76557903720361081

"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_hsc_pdr3_dud_22.5 = lsdb.open_catalog("https://huggingface.co/datasets/UniverseTBD/mmu_hsc_pdr3_dud_22.5")
other = lsdb.open_catalog("https://huggingface.co/datasets/<org>/<other_catalog>")

crossmatched = mmu_hsc_pdr3_dud_22.5.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 Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP), a wide-field imaging survey conducted with the Hyper Suprime-Cam on the Subaru Telescope. It uses data from the Deep and UltraDeep fields of the third Public Data Release (PDR3), which cover a smaller area of the sky but provide deeper (lower-noise) observations.

Data modality
The dataset consists of multi-band image cutouts (160 × 160 pixels) in five optical bands (g, r, i, z, y), extracted from larger survey images. Each cutout is centered on an object and is associated with measurements from the survey’s analysis pipeline. The dataset contains approximately 400,000 objects.

Typical use cases
This dataset can be used for machine learning applications on astronomical images, such as detecting rare objects, classifying sources, or characterizing galaxy properties.

Caveats
The dataset is restricted to the Deep/UltraDeep fields, which cover a relatively small area of the sky compared to the full survey, although with deeper (lower-noise) observations. In addition, the sample is constructed using selection criteria such as magnitude limits, requiring multiple observations across all bands, and removing objects affected by artifacts or unreliable measurements. As a result, the dataset may not fully represent the broader survey.

Citation
Data from the HSC-SSP can be used under the conditions specified by the survey. Users should include the credit “NAOJ / HSC Collaboration” and follow the usage terms.

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