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juliensimon/otter-tde-catalog

OTTER TDE Catalog Credit: NASA/ESA/Hubble Part of a dataset collection on Hugging Face. Dataset description All known tidal disruption events (TDEs) from the Open TDE Catalog — stars torn apart by supermassive black holes. A tidal disruption event (TDE) occurs when a star passes close enough to a supermassive black hole to be ripped apart by tidal forces, producing a luminous flare visible across the electromagnetic spectrum. The Open TDE Catalog… See the full description on the dataset page: https://huggingface.co/datasets/juliensimon/otter-tde-catalog.

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Dataset Card

OTTER TDE Catalog

<div align="center"> <img src="banner.jpg" alt="The Crab Nebula, a supernova remnant" width="400"> <p><em>Credit: NASA/ESA/Hubble</em></p> </div>

Part of a [dataset collection](https://huggingface.co/collections/juliensimon/astronomy-datasets-67c2e994a8b1a76b88ecfe22) on Hugging Face.

Dataset description

All known tidal disruption events (TDEs) from the Open TDE Catalog — stars torn apart by supermassive black holes.

A tidal disruption event (TDE) occurs when a star passes close enough to a supermassive black hole to be ripped apart by tidal forces, producing a luminous flare visible across the electromagnetic spectrum. The Open TDE Catalog aggregates all known TDE candidates with coordinates, redshifts, host galaxy identifications, and peak magnitudes.

Tidal disruption events provide a unique laboratory for studying supermassive black holes (SMBHs) that are otherwise quiescent and therefore undetectable. When a star on a low-angular-momentum orbit enters the tidal radius of an SMBH, the differential gravitational force across the star exceeds its self-gravity, shredding it into a stream of debris. Roughly half of this material becomes bound and accretes onto the black hole, producing a luminous flare that peaks in the UV/optical for lower-mass black holes (10^6--10^7 solar masses) and in the soft X-ray band for more massive ones. The light curve rise time, peak luminosity, and late-time decay rate (classically predicted to follow a t^(-5/3) power law) encode the black hole mass, the stellar mass and structure, and the orbital geometry.

The spectroscopic classification of TDEs into hydrogen-rich (TDE-H), helium-rich (TDE-He), and mixed subtypes reflects the composition of the disrupted star and the complex reprocessing of emission in the debris stream and outflows. Relativistic TDEs -- such as Swift J1644+57 -- launch powerful jets detectable at radio through hard X-ray wavelengths, providing probes of jet formation physics analogous to active galactic nuclei but in a time-resolved, 'clean' environment. The host galaxy properties (mass, morphology, nuclear activity) are critical for understanding the SMBH occupation fraction and the stellar dynamics that deliver stars to disruption orbits, with TDEs preferentially occurring in post-starburst ('E+A') galaxies for reasons that remain actively debated.

Schema

ColumnTypeDescriptionSampleNull %
nameobjectPrimary TDE designation (e.g., 'ASASSN-14li', 'AT2019qiz', 'Swift J1644+57'); modern transients use AT prefix until spectroscopically confirmed2MASX J02490.0%
aliasesobjectComma-separated list of alternative designations from different surveys or reporting telegrams; null if no aliases recorded2XMMi J184725.1-63172483.3%
ra_hmsobjectRight ascension of the TDE / host nucleus in sexagesimal format (HH:MM:SS.ss)02:49:17.2813.3%
dec_dmsobjectDeclination of the TDE / host nucleus in sexagesimal format (+DD:MM:SS.ss)-04:12:5413.3%
rafloat64Right ascension in decimal degrees (J2000.0 ICRS); range 0-360; null for ~10% of entries lacking coordinates42.32214.4%
decfloat64Declination in decimal degrees (J2000.0 ICRS); range -90 to +90; null when ra is null-4.21513.3%
redshiftfloat64Host galaxy spectroscopic redshift; TDE surveys typically probe 0.01 < z < 1; null for ~40% of entries; range ~0.001 (very nearby) to ~10.01866.7%
claimed_typeobjectSpectroscopic classification: 'TDE' (confirmed), 'TDE?' (candidate), 'TDE-H' (hydrogen-dominated spectrum), 'TDE-He' (helium-dominated), 'TDE-H+He' (mixed), 'TDE-featureless'; null for unclassified candidatesTDE58.9%
host_galaxyobjectName of the host galaxy where the TDE occurred; TDEs preferentially occur in post-starburst ('E+A') galaxies; null for ~30% of entries2MASX J02491731-04125217.8%
host_rafloat64Host galaxy nucleus right ascension in decimal degrees; may differ slightly from TDE position for well-resolved hosts42.3221678.9%
host_decfloat64Host galaxy nucleus declination in decimal degrees-4.21457.8%
host_offset_arcsecfloat64Angular offset between the TDE position and the host nucleus in arcseconds; genuine TDEs should be coincident with the nucleus (offset < 1 arcsec for high-z events); null for most entries1.89720.0%
peak_magfloat64Peak apparent magnitude (filter unspecified, typically optical/UV); null for ~60% of entries15.652.2%
peak_abs_magfloat64Peak absolute magnitude; typical TDE: -17 to -21 mag; null for entries lacking redshift or peak apparent magnitude-20.85555.6%
peak_datedatetime64[ns]UTC date of peak brightness; null for events where the light curve peak was not well-constrained2014-04-04 00:00:0053.3%
discovery_datedatetime64[ns]UTC date the transient was first reported; format YYYY-MM-DD2006-07-14 00:00:0027.8%
luminosity_distance_mpcfloat64Luminosity distance in megaparsecs, computed from redshift; null when redshift is unavailable83.56.7%
velocity_km_sfloat64Host galaxy recession velocity in km/s (v = cz); null when redshift is unavailable5520.06.7%
ebvfloat64Milky Way line-of-sight dust reddening E(B-V) in magnitudes from the Schlegel/Schlafly dust maps; used to correct observed magnitudes for extinction0.026714.4%
instrumentsobjectInstruments or facilities used for observations (e.g., 'ZTF', 'Swift-XRT', 'SDSS'); null for many entriesPN, PSPC, XRT18.9%
discovery_yearInt64Year of discovery; derived from discoverydate; null when discoverydate is unavailable200627.8%

Quick stats

  • —90 tidal disruption events (1990--2018)
  • —77 with sky coordinates
  • —84 with redshift measurements
  • —37 with spectroscopic classification
  • —83 with identified host galaxy
  • —43 with peak magnitude

Classifications

TypeCount
TDE?14
MS + SMBH8
TDE6
AGN?3
Candidate2
WD + IMBH1
Planet + WD1
Low-mass TDE1
SLSN-I?1

Usage

python
from datasets import load_dataset
import matplotlib.pyplot as plt

ds = load_dataset("juliensimon/otter-tde-catalog", split="train")
df = ds.to_pandas()

# All confirmed TDEs
confirmed = df[df["claimed_type"] == "TDE"]

# TDEs with redshift
with_z = df[df["redshift"].notna()].sort_values("redshift")

# Nearby TDEs (z < 0.05)
nearby = df[df["redshift"] < 0.05].sort_values("redshift")

# Discoveries per year
per_year = df["discovery_year"].dropna().value_counts().sort_index()
plt.figure(figsize=(10, 5))
plt.bar(per_year.index, per_year.values, color="steelblue")
plt.xlabel("Year")
plt.ylabel("Number of TDEs discovered")
plt.title("TDE Discoveries per Year")
plt.tight_layout()
plt.show()

Data source

https://github.com/astrocatalogs/tidaldisruptions

Related datasets

Citation

bibtex
@dataset{otter_tde_catalog,
  title = {OTTER TDE Catalog},
  author = {Simon, Julien},
  year = {2026},
  url = {https://huggingface.co/datasets/juliensimon/otter-tde-catalog},
  publisher = {Hugging Face},
  note = {Derived from the project's GitHub repository, https://github.com/astrocatalogs/tidaldisruptions}
}

License

CC-BY-4.0