Fazari Sky Explorer

Evidence

Is it right? Check our numbers.

We measured how far each target moved between two SPHEREx observing seasons, from the images alone. Then we compared that with the best independent prediction: Gaia DR3, or published astrometry where Gaia has none. Here is every target, including the ones we could not measure.

Numbered tests: was it tested, and is it right?

Each test was run in a separate test round on the final code. The pass thresholds were fixed before the run. Tests that did not pass stay in the list, in their place; a re-test will update this page.

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Measured motion against the catalogue

One row per target. The big numbers are the speed per year: our fit of all images against the catalogue. The small lines give the shift between two seasons seen with the same telescope orientation, about a year apart; the pass rule (fixed before testing) is on that shift.

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Known asteroids found blindly

We searched 24 ecliptic fields without being told where to look, then matched what we found to the known asteroids (SkyBoT, positions moved to where SPHEREx was). 217 known asteroids recovered: V<17 47 of 53, V<18 101 of 132. Median position offset 0.68″. 47 objects were linked into tracks; their speed agrees with the orbit prediction to a median 0.36 %. All asteroid results.

What we cannot explain yet

These are open questions, not results. We list them so you can judge the numbers above.