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_healpix_29
int64
lightcurve
dict
ra
float64
dec
float64
obj_type
string
object_id
string
27,677,490,352,178,670
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", ...
50.415459
16.86739
SN Ib/c
SN2006aj
2,829,561,277,534,609,400
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", ...
148.625885
-25.708139
SN IIb
SN2006T
2,835,488,839,065,606,700
{ "band": [ "B", "B", "B", "B", "H", "H", "H", "H", "I", "I", "I", "I", "J", "J", "J", "J", "Ks", "Ks", "Ks", "Ks", "R", "R", "R", "R", "U", "U", "U", "U", "V", "V", "V", "V", "i'", ...
149.350677
-19.356421
SN Ic
SN2007aw
2,870,298,439,381,265,400
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "J", "J", "J", "J", "J", "J", "J", "J", "Ks", "Ks"...
145.805832
-9.61472
SN IIb
SN2006ba
314,745,796,130,558,400
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "I", "I", "I", "J", ...
150.399963
21.61167
SN Ib
SN2007ag
356,194,615,710,917,900
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", ...
137.397293
33.119141
SN Ib
SN2007uy
356,194,751,035,896,960
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", ...
137.377716
33.138969
SN Ib
SN2008D
379,977,268,336,903,360
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", ...
173.013748
36.701
SN Ib/c
SN2006lv
396,044,076,338,267,260
{ "band": [ "B", "B", "B", "H", "H", "H", "I", "I", "I", "J", "J", "J", "Ks", "Ks", "Ks", "R", "R", "R", "U", "U", "U", "V", "V", "V", "i'", "i'", "i'", "r'", "r'", "r'", "u'", "u'", "u'...
177.359085
51.82272
SN Ic
SN2007bg
407,975,593,271,372,540
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", ...
139.336578
41.909081
SN Ibn
SN2006jc
43,256,176,323,661,384
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "I", "I", "J", "J", "J", "J", ...
37.047379
19.60375
SN Ib
SN2006F
437,471,792,971,433,860
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "I", "I", "I", "J", ...
116.860458
26.925671
SN Ic
SN2005kf
446,670,850,767,360,800
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "J", "J", "J", "J", "J", "J", "J", "J", "Ks", "Ks"...
110.93013
33.44389
SN Ib
SN2001ej
504,770,873,312,005,300
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", ...
137.176376
44.814281
SN Ic
SN2005mf
539,018,042,342,926,100
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", ...
154.194824
73.440666
SN Ib
SN2006gi
553,502,723,412,288,600
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", ...
93.384712
69.730331
SN Ic
SN2007iq
610,586,881,407,441,400
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", ...
234.874329
24.434811
SN Ib
SN2009er
678,505,876,556,635,300
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "I", "I", "I", "J", "J", "J", "J", "J", "J", "J", ...
248.159454
41.459221
SN IIb
SN2008cw
69,513,900,429,126,850
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "H", "I", "I", ...
46.453999
36.769611
SN Ic
SN2005ek
708,628,372,409,470,000
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", ...
267.088287
54.15144
SN Ic
SN2007cl
717,993,244,981,365,600
{ "band": [ "B", "B", "B", "H", "H", "H", "I", "I", "I", "J", "J", "J", "Ks", "Ks", "Ks", "R", "R", "R", "U", "U", "U", "V", "V", "V", "i'", "i'", "i'", "r'", "r'", "r'", "u'", "u'", "u'...
264.617432
61.03714
SN Ic
SN2008an
730,465,052,017,719,200
{ "band": [ "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "H", "H", "H", ...
196.445709
27.73567
SN Ic
SN2005az
737,167,435,107,677,600
{ "band": [ "B", "B", "H", "H", "I", "I", "J", "J", "Ks", "Ks", "R", "R", "U", "U", "V", "V", "i'", "i'", "r'", "r'", "u'", "u'" ], "time": [ 52266.5234375, 52320.46484375, 0, 0, 52266.53125, 52320.4687...
198.349533
36.638248
SN IIb
SN2001gd
742,844,162,613,118,200
{ "band": [ "B", "B", "B", "B", "B", "B", "H", "H", "H", "H", "H", "H", "I", "I", "I", "I", "I", "I", "J", "J", "J", "J", "J", "J", "Ks", "Ks", "Ks", "Ks", "Ks", "Ks", "R", "R", "R", ...
214.132507
39.587749
SN Ib
SN2006cb
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mmu_cfa_seccsn HATS Catalog Collection

This is the collection of HATS catalogs representing mmu_cfa_seccsn.

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_cfa_seccsn")
# One-degree cone.
catalog = lsdb.open_catalog(
    "https://huggingface.co/datasets/UniverseTBD/mmu_cfa_seccsn",
    search_filter=lsdb.ConeSearch(ra=41.0, dec=37.0, 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_cfa_seccsn � 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_cfa_seccsn_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
64 5 62 192.4 MiB hats-import v0.7.3, hats v0.7.3

Catalog columns

The main HATS catalog contains the following columns:

Name _healpix_29 lightcurve.band lightcurve.time lightcurve.mag lightcurve.mag_err ra dec obj_type object_id
Data Type int64 list[string] list[float] list[float] list[float] double double string string
Nested? lightcurve lightcurve lightcurve lightcurve
Value count 64 16,291 16,291 16,291 16,291 64 64 64 64
Example row 166916028924337739 [B, B, B, B, B, B, B, B, B, B, B, � (748 total)] [5.435e+04, 5.435e+04, 5.435e+04, � (748 total)] [14.11, 14.23, 14.35, 14.73, 14.85, � (748 total)] [0.014, 0.014, 0.014, 0.014, 0.014, � (748 total)] 40.87 37.35 SN Ib/c SN2007gr
Minimum value 27677490352178670 B -0.0 -0.0 -0.0 0.3315800130367279 -25.708139419555664 SN II-pec SN2001ej
Maximum value 2870298439381265425 u' 55244.17578125 22.079999923706055 0.7300000190734863 350.2640686035156 74.57247161865234 SN Ic-pec SN2009jf

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

crossmatched = mmu_cfa_seccsn.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 Harvard-Smithsonian Center for Astrophysics (CfA) Supernova Group observations and contains light curves of stripped-envelope core-collapse supernovae observed between 2000 and 2011.

Data modality
The dataset consists of light curve data for 64 stripped-envelope core-collapse supernovae in the u’UBVRIr’i’JHKs bands. Each sample includes sky coordinates (ra, dec), object identifiers and classification, and a light curve with time (modified Julian date), band, magnitude (mag), and magnitude error (mag_err).

Typical use cases
The dataset is used in studies of core-collapse supernovae and their observational properties.

Caveats
The dataset follows the CfA data structure. The flux and flux_err fields are replaced by mag and mag_err fields, which present the original photometric measurements in the standard photometric system. It represents a specific class of supernovae (stripped-envelope core-collapse), which differs from Type Ia samples.

Citation
Data are obtained from the CfA Supernova Archive. Users should cite the corresponding CfA-SECCSN publication and follow the archive acknowledgement guidelines.

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