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Before Sputnik · source record · preprint

On the Image Profiles of Transients in the Palomar Sky Survey

Villarroel, B.; Solano, E.; Marcy, G. W. · 2025

AI-verified citationSRC-VILLARROEL-2025-PROFILES
identifier / locator
arXiv: 2507.15896 (July 2025)
url
https://arxiv.org/abs/2507.15896
verification note
arXiv record and abstract verified via the arXiv API (2026-08-22 batch).
reliability notes
  • The proponent response to the Hambly & Blair morphology argument: sub-second flashes are expected to be sharper and rounder than star images on long exposures.
  • Preprint; a physics argument, not a new measurement — no calibration of flash profiles on period emulsions exists yet.

Evidence drawn from this source

Qualifies· moderateTRN-E006

The proponent physics reply: flashes should be sharp

what the source states
Optical principles and atmospheric physics imply that unresolved flashes lasting less than a second naturally appear sharper and more circular than stellar images, particularly on long-exposure plates where stars are blurred by seeing and tracking errors; the sharp profiles are therefore consistent with the transient interpretation.
what we infer
This converts the sharpness observation from an artifact signature into an ambiguous one — but only argumentatively. No one has exposed period-appropriate emulsion to controlled sub-second flashes and measured whether real flash profiles match the nine marks (TRN-R002).
limitations
  • A physics argument, not a measurement; the two profile distributions (flash vs artifact) may overlap entirely, in which case sharpness discriminates nothing.
  • Proponent-team preprint, not peer reviewed.