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Degeneracy between Lensing and Occultation in the Analysis of Self-lensing Phenomena

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arxiv 1603.03500 v1 pith:Z67DWAXW submitted 2016-03-11 astro-ph.SR astro-ph.IM

Degeneracy between Lensing and Occultation in the Analysis of Self-lensing Phenomena

classification astro-ph.SR astro-ph.IM
keywords self-lensingdegeneracylensinglightbinariesbinarycurvesmagnification
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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More than 40 years after the first discussion, it was recently reported the detection of a self-lensing phenomenon within a binary system where the brightness of a background star is magnified by its foreground companion. It is expected that the number of self-lensing binary detections will be increased in a wealth of data from current and future survey experiments. In this paper, we introduce a degeneracy in the interpretation of self-lensing light curves. The degeneracy is intrinsic to self-lensing binaries for which both magnification by lensing and de-magnification by occultation occur simultaneously and is caused by the difficulty in separating the contribution of the lensing-induced magnification from the observed light curve. We demonstrate the severity of the degeneracy by presenting example self-lensing light curves suffering from the degeneracy. We also present the relation between the lensing parameters of the degenerate solutions. The degeneracy would pose as an important obstacle in accurately determine self-lensing parameters and thus to characterize binaries.

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Cited by 2 Pith papers

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  1. Microlensing Detection and Inference via Learned Bayes Factors

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    A unified transformer-based pipeline detects 99.9% of recoverable simulated microlensing events and outperforms literature hard cuts in the short-duration finite-source regime with amortized neural posterior inference.

  2. Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy

    astro-ph.HE 2025-12 conditional novelty 5.0

    Self-lensing of a moving GW chirp by an orbiting black hole yields a curve width and interference beats that together give the orbital distance and the black hole mass.