6.50 × 10⁹ M☉ · a* 0.900
Platform
From the first photon captured to the final published model, every stage of the analysis lives in one reproducible workspace.
Every linked dish becomes one Earth-sized aperture. As the planet turns, each telescope pair sweeps a track through the uv-plane and fills in the synthesized image.
≈ 10,700 km
longest baseline
≈ 20 µas
angular resolution
Drag across the frame: an observed Einstein ring on the left, the source galaxy our inversion recovers on the right.
GRB 260918H · GRB
Short GRB · Swift/BAT trigger
GW260918_070054 · GW
BBH merger · 62 M☉ remnant
FRB 20260918C · FRB
Repeating burst · DM 412 pc cm⁻³
AT2026xqb · TDE
Tidal disruption flare · z = 0.021
GW260918_031204 · GW
Kilonova candidate · z = 0.04
Gravitational waves, tidal disruptions and bursts, classified and pushed in under 90 s.
Every calibrated frame catalogued and queryable. Time-travel across epochs without moving a byte.
14.2 PB
catalogued
3.1 B
sources
42 ms
p50 query
SELECT * FROM transients WHERE z < 0.05Shared notebooks, versioned models and review trails for multi-institution teams.
N. Adeyemi pushed lens-model v14 · 2m ago
212
research teams
31
countries
Pipeline
01
Raw visibilities and photometry stream in from federated arrays, time-stamped against hydrogen-maser clocks.
02
Atmospheric phase, instrument gain and RFI corrections are applied automatically and reproducibly.
03
General-relativistic ray tracing fits the observation, from photon ring to outer disk, in minutes.
# Fit a Kerr metric to tonight's VLBI run
from singularity import Observatory
obs = Observatory.connect("eht-federated")
run = obs.runs.latest(target="M87*")
model = run.resolve(metric="kerr", fit=["spin", "inclination"])
print(model.summary())Press run to resolve the target →
Early access is open to research institutions, observatories and independent researchers.