Satellite Streaks in HETDEX: Spectra, Orbital Identification, and Survey Impact
arXiv:2611.10301 · doi:10.3847/1538-3881/aeb0a7
Abstract
We present a spectroscopic database and analysis of satellite streaks in Public Data Release 1 (PDR1) from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), covering 6778 observations and 90 deg of sky from January 2017 to July 2024. We detect 527 streaks across 492 observations, a contamination fraction of 7.3% that rises to monthly values above 20% by 2023--2024, although the streaks mask only 0.09% of the survey area. Of the 527 streaks, 475 (90.1%) are identified with a cataloged object using archival two-line elements: 258 (54%) lie in low or Earth orbit and 217 (46%) are geostationary or highly elliptical. Only 35% were launched since 2010; the rest are spent rocket bodies, debris, and older spacecraft. This reflects HETDEX's sensitivity to faint objects and its 2017--2024 observing baseline. The Hobby-Eberly Telescope's large 10\,m aperture and HETDEX's 6\,minute exposures result in similar observed magnitudes for low Earth orbit (LEO) and geostationary Earth orbit (GEO) objects (median for LEO, for GEO). However, once transit time is corrected for, instantaneous magnitudes differ widely: for LEO versus for GEO objects, a difference of 5.6\,mag, while the exposure-averaged magnitudes differ by only 0.5 mag. Normalized to 550 km, the 34 Starlink streaks give , consistent with the mean reported for VisorSat-design spacecraft. The spectra are consistent with reflected sunlight, with modest, signal-to-noise-driven differences in slope. The catalog, spectra, and code are archived at https://doi.org/10.5281/zenodo.22962479.
arXiv comment15 pages, 5 figures, 1 table. Published at Mentuch Cooper et al., 2026, AJ, 172, 303. Data available at https://doi.org/10.5281/zenodo.22962479. Full workflow at https://github.com/eriniocentric/hetdex_sats
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