Investigating the 1L2S Degeneracy for Wide-Orbit Planets

Fuente: arXiv
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Autori principali: Sangtarash, Parisa, Yee, Jennifer C.
Natura: Preprint
Pubblicazione: 2025
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author Sangtarash, Parisa
Yee, Jennifer C.
author_facet Sangtarash, Parisa
Yee, Jennifer C.
contents Wide-orbit planets are particularly sensitive to detection by the Roman Galactic Bulge Time Domain Survey (GBTDS). This study investigates the degeneracy of these events with binary sources, focusing on how observation cadence affects the resolution of these degeneracies. We analyzed the impact of various cadences from (3.6 min)^(-1) to (5 hr)^(-1), which encompasses planned cadences for both the GBTDS and cadences used by ground-based surveys like KMTNet. The results show that a $\sim (15 min)^(-1) cadence is generally sufficient to resolve this degeneracy unless the source star is a giant (rho >~ 0.01).
format Preprint
id arxiv_https___arxiv_org_abs_2503_11768
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Investigating the 1L2S Degeneracy for Wide-Orbit Planets
Sangtarash, Parisa
Yee, Jennifer C.
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
Wide-orbit planets are particularly sensitive to detection by the Roman Galactic Bulge Time Domain Survey (GBTDS). This study investigates the degeneracy of these events with binary sources, focusing on how observation cadence affects the resolution of these degeneracies. We analyzed the impact of various cadences from (3.6 min)^(-1) to (5 hr)^(-1), which encompasses planned cadences for both the GBTDS and cadences used by ground-based surveys like KMTNet. The results show that a $\sim (15 min)^(-1) cadence is generally sufficient to resolve this degeneracy unless the source star is a giant (rho >~ 0.01).
title Investigating the 1L2S Degeneracy for Wide-Orbit Planets
topic Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2503.11768