Infrared-excess sources in VVV: candidate debris discs, SED characterization, and variability analysis

arXiv:2609.03119 · astro-ph.SR, astro-ph.EP, astro-ph.GA · Submitted 2026-09-02 · Read on arXiv

astro-ph.SR, astro-ph.EP, astro-ph.GA

Submitted: 2026-09-02

Updated: 2026-09-02

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