A concrete result · Scientific data becomes a teaching map

A complete ultraviolet sky map: observation and prediction

Follow the full-sky image and four build stages to see how Claude Science helped organize old observations and fill gaps—and why a complete map still needs provenance.

Anthropic published the creator’s account on October 8; the technical page dates the map September 16. We inspect the original images, method and current entry without rebuilding the map or using the creator’s account.

Far- and near-ultraviolet full-sky composite showing blue-violet clouds, starlight and the Galactic plane in one oval projection; the complete image includes predictions.
Original composite of far- and near-ultraviolet light, including statistical gap filling. Blue-violet indicates relatively stronger far-UV, not the sky’s naked-eye colour. Brice Ménard / Anthropic; GALEX, Swift-UVOT, FIMS/SPEAR, TD-1, Planck and Gaia. · Open full-size image
In this articleContents6

中文

Start with a map for teaching the sky

This oval map places the Galactic Centre in the middle. Ultraviolet reveals hot stars and dust illuminated by starlight, letting students explore familiar sky in another band. Astrophysicist Brice Ménard used Claude Science to complete a teaching resource he had long put aside.

The map is complete, but its support varies across the sky. Telescope observations and statistical predictions meet in one image; provenance determines what a region can help you understand.

Sources and further reading

中文

How the black gaps become a connected sky

GALEX gathered about 38,000 observations in 2003–2013, avoiding some bright stars and the Galactic plane to protect its detectors. Building the map required background cleaning, brightness calibration and common coordinates and resolution. The four stages make that work visible.

Gap filling uses statistical regression learned from existing dust, starlight and other data. Claude Science helped organize agents, processing and computation; the regression predicts ultraviolet brightness. The account does not identify a particular Claude model version.

Four original views of the same sky projection: GALEX gaps, cleaning and near-UV-informed far-UV, added coarse data, then the completed map.
Read top-left, top-right, bottom-left, bottom-right: GALEX observations → cleaning and near-UV-informed far-UV → coarse far-UV constraints across the plane → final map. Black marks a gap at that stage, not empty space. Original figure with its survey credits retained. · Open full-size image
Sources and further reading

中文

Complete coverage still needs provenance

The creator reports predicted finer structure over about 28% of the far-UV sky and 27% of the near-UV. Most of that far-UV region also has coarse FIMS/SPEAR constraints. A continuous image alone cannot distinguish direct imaging, cross-band inference, coarse constraints and prediction.

A local provenance example marks GALEX observations in blue and model-filled gaps in purple and red. The page explains per-pixel source weights. The overall structure supports teaching; predicted regions support neither new-star discovery nor an independent dust measurement.

Sources and further reading

中文

Hide observations to test the gap filling

The creator held out GALEX regions, predicted their ultraviolet values without seeing them, then compared with the observations. That tests gap filling in similar regions; it does not turn unobserved sky into new measurements.

For the gap-fill predictor, Section 6 says validation material informed development and parameter tuning, so there is no independent blind test. The October 2026 manuscript remains a draft in preparation, without human peer review. The visible map and method do not establish independently verified all-sky accuracy.

Sources and further reading

中文

A person spotted discs after two agent reviews

Ménard spotted faint discs in a dim field: backgrounds from individual GALEX pointings had not been fully removed. The issue was listed as a risk, yet survived two agent reviews. His observation sent the agents back to recalibrate about 38,000 pointings.

The same-contrast panels show a local improvement. The technical page still notes possible faint residual discs. The useful loop is visible: painstaking processing becomes an inspectable result, and a person finds what needs another correction.

Two sky fields, each shown in three panels at the same row contrast: pointing-disc traces, background calibration, then the further-calibrated and filled result.
Each row shows the same field at the same contrast. Disc boundaries diminish from left to right. The final column also adds predictions and Gaia stars, so disappearing holes cannot all be attributed to calibration. Original figure from GALEX and other survey data. · Open full-size image
Sources and further reading

中文

Explore the map before choosing a workbench

For a curious reader, start by comparing the sky across bands. The page says FITS, HiPS and documentation downloads will be added. Its provenance and uncertainty descriptions do not establish a full-map layer switch or complete data downloads today.

For your own scientific data and computations, explore Claude Science. Its current FAQ describes a beta workbench using your plan’s Claude models, on macOS, Windows and Linux for Pro, Max, Team and Enterprise; organization plans need admin enablement. We have not rebuilt this map.

Sources and further reading