Datasets:
name stringlengths 1 479 | ra_deg float64 0 360 | dec_deg float64 -85.18 88.7 | lens_redshift float64 0 3 ⌀ | lens_type stringclasses 3
values | grading stringclasses 2
values | reference stringclasses 559
values |
|---|---|---|---|---|---|---|
MS2357.4-3520 | 0.00471 | -35.05971 | 0.508 | galaxy | probable | Gioia et al. (1990) - doi:10.1086/191426 |
NSCS J000001+051909 | 0.00504 | 5.31906 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000002+085519 | 0.00925 | 8.92179 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000006+081630 | 0.02512 | 8.27492 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.0254+21.6415 | 0.02542 | 21.6415 | 0.502973 | galaxy | probable | Huang et al. (2021) - arXiv:2005.04730 |
MS2357.5-6352 | 0.02858 | -63.59437 | 0.136 | galaxy | probable | Gioia et al. (1990) - doi:10.1086/191426 |
RXC J0000.1+0816 | 0.0295 | 8.2744 | 0.0396 | galaxy | probable | B\"ohringer et al. (2000) - arXiv:astro-ph/0003219 |
HATLASJ000007.4-334059 | 0.03083 | -33.68306 | null | galaxy | probable | Negrello et al. (2016) - arXiv:1611.03922 |
000008+022658 | 0.03524 | 2.44944 | 0.43 | galaxy | probable | https://arxiv.org/abs/2312.07333 |
DESI-000.0369+21.2841 | 0.03692 | 21.2841 | 0.357 | galaxy | probable | Huang et al. (2021) - arXiv:2005.04730 |
RXJ0000.1+0816 | 0.044 | 8.277 | 0.0396 | galaxy | probable | Ebeling et al. (1998) - arXiv:astro-ph/9812394 |
NSCS J000014+052333 | 0.05646 | 5.39243 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.0611-05.9508 | 0.06112 | -5.95079 | 0.637 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
HSCJ000018+001617 | 0.07883 | 0.27158 | 0.63 | galaxy | probable | Shu et al. (2022) - arXiv:2201.11135 |
HSCJ000020-002051 | 0.08679 | -0.3475 | 0.56 | galaxy | probable | Shu et al. (2022) - arXiv:2201.11135 |
DESI-000.1063-03.9559 | 0.10629 | -3.95586 | 0.86 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
J0000+2832 | 1091 | 0.10646 | 28.53665 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Talbot et al. (2020) - arXiv:2007.09006 |
NSCS J000026+103803 | 0.11 | 10.63405 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000028+065242 | 0.11467 | 6.87824 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000037+062335 | 0.15525 | 6.39299 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000039+070140 | 0.16071 | 7.0276 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000043+053335 | 0.17783 | 5.55952 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000044+052512 | 0.18404 | 5.4199 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000045+072119 | 0.18529 | 7.355 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.1963+28.2100 | 0.19625 | 28.21003 | 0.415 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
DESI-000.2017-46.0549 | 0.20167 | -46.05489 | 0.339 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
NSCS J000049+065420 | 0.20325 | 6.90546 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DES J000049-561046 | 0.20742 | -56.17966 | null | galaxy | probable | Rojas et al. (2021) - arXiv:2109.00014 |
000008+022659 | 0.21573 | -0.49349 | null | galaxy | probable | https://arxiv.org/abs/2312.07333 |
NSCS J000052+125539 | 0.21638 | 12.92726 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000052+004625 | 0.2165 | 0.77355 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000054+121452 | 0.22379 | 12.24766 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0000-3502 | 0.23792 | -35.04838 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
NSCS J000060+004916 | 0.24967 | 0.82091 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.2512-10.3396 | 0.25117 | -10.33961 | 0.687 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
J0001-3340 | 1678 | 0.25325 | -33.67316 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
SOGRAS0001+0020 | 0.25417 | 0.33806 | 0.538 | galaxy | probable | Furlanetto et al. (2012) - arXiv:1210.4136 |
DESI-000.2544-00.5579 | 0.25442 | -0.55785 | 0.5728 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
DESI-000.2616-37.3243 | 0.26158 | -37.32427 | 0.451 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
NSCS J000104+023240 | 0.26725 | 2.54415 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
14093927 | 0.27508 | 23.76815 | 0.638658 | galaxy | probable | Stein et al. (2021) - arXiv:2110.00023 |
000008+022660 | 0.277103 | 1.058266 | 0.721 | galaxy | probable | https://arxiv.org/abs/2203.12805 |
DESI-000.2881-10.5619 | 0.28808 | -10.5619 | 0.437964 | galaxy | probable | Huang et al. (2021) - arXiv:2005.04730 |
NSCS J000111+010332 | 0.29754 | 1.05861 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0001-3321 | 741 | 0.30467 | -33.36632 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
HSCJ000114+001619 | 0.31062 | 0.27214 | 0.664 | galaxy | probable | Shu et al. (2022) - arXiv:2201.11135 |
NSCS J000116+054751 | 0.31783 | 5.79725 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0001-3010 | 2694 | 0.31829 | -30.17678 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
J0001-3208 | 742 | 0.3185 | -32.14243 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
NSCS J000118-013102 | 0.323 | -1.51734 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
Q0957+561 | 0.336667 | 55.897056 | 0.356 | galaxy | confident | https://web.physics.ucsb.edu/~tt/LSD/ |
NSCS J000122-000104 | 0.3395 | -0.01787 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
AGEL 010128-334319 | 0.365833 | -33.722 | 0.5811 | galaxy | confident | https://arxiv.org/ftp/arxiv/papers/2205/2205.05307.pdf |
DESI-000.3685-57.8585 | 24007270 | 0.36854 | -57.85849 | null | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 | Stein et al. (2021) - arXiv:2110.00023 |
J0001-5549 | 0.37075 | -55.83308 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
000008+022661 | 0.3735 | -0.0449 | 0.247 | cluster | probable | https://arxiv.org/abs/2002.01611 |
DESI-000.3785-13.3998 | 0.37854 | -13.39983 | 0.612 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
J0001-3221 | 2866 | 0.38696 | -32.36279 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
NSCS J000136+080725 | 0.40179 | 8.12349 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.4022-04.0111 | 0.40221 | -4.0111 | 0.723671 | galaxy | probable | Huang et al. (2021) - arXiv:2005.04730 |
CS82SL00:01:40-00:33:50 | 0.41738 | -0.56404 | 0.247 | galaxy | probable | Moraes et al. (2014) - adsabs:2014RMxAC..44..202M |
NSCS J000150+103550 | 0.45733 | 10.59712 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000153+120347 | 0.47187 | 12.06287 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
NSCS J000156+124542 | 0.48217 | 12.76138 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
SOGRAS0001+0047 | 0.48333 | 0.78917 | 0.527 | galaxy | probable | Furlanetto et al. (2012) - arXiv:1210.4136 |
RXC J0001.9+1204 | 0.48771 | 12.073 | 0.2033 | galaxy | probable | B\"ohringer et al. (2000) - arXiv:astro-ph/0003219 |
NSCS J000158+054219 | 0.49267 | 5.70521 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
000008+022662 | 0.492786 | 4.577447 | 0.675 | galaxy | probable | https://arxiv.org/abs/2203.12805 |
DESI-000.5014-46.7212 | 0.49929 | -46.7225 | 0.538 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
J0002+2531 | 1211 | 0.51579 | 25.52364 | null | galaxy | confident | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Talbot et al. (2020) - arXiv:2007.09006 |
DESJ0002-3332 | 0.52721 | -33.54406 | 0.5 | galaxy | probable | O'Donnell et al. (2021) - arXiv:2110.02418 |
DESI-000.5290-37.6745 | DES J000206-374028 | 0.52896 | -37.67453 | null | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 | Rojas et al. (2021) - arXiv:2109.00014 |
1270 | J0002+3124 | 0.53579 | 31.4033 | null | galaxy | confident | Talbot et al. (2020) - arXiv:2007.09006 | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
1280 | J0002-0712 | 0.53912 | -7.21173 | null | galaxy | probable | Talbot et al. (2020) - arXiv:2007.09006 | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
J0002-3303 | 135 | 0.53929 | -33.05526 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
NSCS J000210+060257 | 0.543 | 6.04907 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0002+1330 | 778 | 0.54467 | 13.50404 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Talbot et al. (2020) - arXiv:2007.09006 |
J0002-0128 | 0.56625 | -1.47472 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
NSCS J000219-013216 | 0.57788 | -1.53778 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DES J000220-444333 | 0.584 | -44.72591 | null | galaxy | probable | Rojas et al. (2021) - arXiv:2109.00014 |
000008+022663 | 0.595733 | 4.357103 | 0.707 | galaxy | probable | https://arxiv.org/abs/2203.12805 |
DESJ0002-3507 | 0.59845 | -35.12122 | 0.51 | galaxy | probable | https://iopscience.iop.org/article/10.3847/1538-4365/ab26b6#apjsab26b6t5 |
NSCS J000228+014342 | 0.61842 | 1.72816 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0002-5229 | 0.62358 | -52.48886 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
J0002-3026 | 2544 | 0.62767 | -30.43883 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
0302+006 | 0.62875 | 0.100583 | 0.938 | galaxy | confident | https://web.physics.ucsb.edu/~tt/LSD/ |
J0002-3229 | 831 | 0.64117 | -32.49791 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
NSCS J000234-003335 | 0.64246 | -0.55973 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0002-3209 | 3447 | 0.65762 | -32.15828 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
AGEL 010238+015857 | 0.659583 | 0.982417 | null | galaxy | confident | https://arxiv.org/ftp/arxiv/papers/2205/2205.05307.pdf |
J0002+0248 | 0.67137 | 2.81468 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
1092 | J0002+2436 | 0.67362 | 24.60354 | null | galaxy | confident | Talbot et al. (2020) - arXiv:2007.09006 | Moustakas et al. (2012) - adsabs:2012hst..prop12833M |
NSCS J000242+003732 | 0.67517 | 0.62544 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
985915 | 0.67633 | -0.2222 | 0.298873 | galaxy | probable | Stein et al. (2021) - arXiv:2110.00023 |
NSCS J000245-003129 | 0.68617 | -0.52486 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
J0002-3412 | 2710 | 0.68758 | -34.20733 | null | galaxy | probable | Moustakas et al. (2012) - adsabs:2012hst..prop12833M | Petrillo et al. (2018) - arXiv:1812.03168 |
NSCS J000247+042404 | 0.69383 | 4.40097 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.6943+27.0894 | 0.69429 | 27.0894 | 0.584073 | galaxy | probable | Huang et al. (2021) - arXiv:2005.04730 |
NSCS J000250+055424 | 0.70842 | 5.90643 | null | galaxy | probable | Lopes et al. (2004) - doi:10.1086/423038 |
DESI-000.7092-55.6288 | 0.70917 | -55.62876 | 0.422 | galaxy | probable | Storfer et al. (2022) - arXiv:2206.02764 |
Strong Gravitational Lens Catalog
Part of the Astronomy Datasets collection on Hugging Face.
A comprehensive catalog of 32,838 confirmed and probable strong gravitational lenses compiled by the lenscat project. Covers both galaxy-scale and cluster-scale lenses drawn from dozens of surveys and publications.
Dataset description
Strong gravitational lensing occurs when a massive foreground object (a galaxy or galaxy cluster) bends the light of a background source so severely that multiple images, arcs, or Einstein rings are produced. This catalog consolidates discoveries from major surveys including SDSS, DES, HSC, CLASH, RELICS, and many others into a single machine-readable table.
Each entry records the lens name, sky coordinates, lens redshift (when measured), morphological type (galaxy or cluster), a confidence grading, and a literature reference.
Schema
| Column | Type | Description |
|---|---|---|
name |
string | Lens system name / identifier |
ra_deg |
float64 | Right ascension (J2000, degrees) |
dec_deg |
float64 | Declination (J2000, degrees) |
lens_redshift |
float64 | Spectroscopic redshift of the lens (null if unmeasured) |
lens_type |
string | Morphological type: "galaxy" or "cluster" |
grading |
string | Confidence level: "confident" or "probable" |
reference |
string | Discovery / catalog reference (URL or bibcode) |
Quick stats
- 32,838 strong gravitational lenses
- 31,755 galaxy-scale lenses, 1,023 cluster-scale lenses
- 2,309 confident, 30,529 probable
- 13,974 lenses with measured redshifts (range 0.000 -- 3.000, median 0.480)
Usage
from datasets import load_dataset
ds = load_dataset("juliensimon/gravitational-lenses", split="train")
df = ds.to_pandas()
# Sky distribution
import matplotlib.pyplot as plt
plt.scatter(df["ra_deg"], df["dec_deg"], s=0.2, alpha=0.3)
plt.xlabel("RA (deg)")
plt.ylabel("Dec (deg)")
plt.title("Strong Gravitational Lenses -- Sky Distribution")
plt.gca().invert_xaxis()
plt.show()
# Redshift distribution
df["lens_redshift"].dropna().hist(bins=60)
plt.xlabel("Lens Redshift")
plt.ylabel("Count")
plt.title("Lens Redshift Distribution")
plt.show()
# Galaxy vs cluster breakdown
df["lens_type"].value_counts().plot.bar()
plt.title("Lens Type Distribution")
plt.show()
# Confident vs probable by type
df.groupby(["lens_type", "grading"]).size().unstack().plot.bar()
plt.title("Grading by Lens Type")
plt.show()
Data source
Compiled by the lenscat project, which consolidates strong lens discoveries from the literature into a single catalog. See the project repository for the full list of contributing surveys and references.
Pipeline
Source code: juliensimon/space-datasets
Citation
@dataset{gravitational_lenses,
author = {Simon, Julien},
title = {Strong Gravitational Lens Catalog},
year = {2026},
publisher = {Hugging Face},
url = {https://huggingface.co/datasets/juliensimon/gravitational-lenses},
note = {Based on the lenscat project (https://github.com/lenscat/lenscat)}
}
License
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