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Autori principali: Guo, Qi, Wei, Leyao, Luo, Wentao, Lin, Shurui, Li, Qinxun, Cai, YiFu, He, Di, Wang, Qingqing, Yang, Ruoxi
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2411.02161
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author Guo, Qi
Wei, Leyao
Luo, Wentao
Lin, Shurui
Li, Qinxun
Cai, YiFu
He, Di
Wang, Qingqing
Yang, Ruoxi
author_facet Guo, Qi
Wei, Leyao
Luo, Wentao
Lin, Shurui
Li, Qinxun
Cai, YiFu
He, Di
Wang, Qingqing
Yang, Ruoxi
contents We propose a novel microlensing event search method that differs from either the traditional time domain method, astrometric microlensing, or the parallax microlensing method. Our method assumes that stars with nearly identical "genes" - normalized Spectral Energy Distributions (SED) bear the same luminosity within the intrinsic scatter due to stellar properties. Given a sample of stars with similar normalized SEDs, the outliers in luminosity distribution can be considered microlensing events by excluding other possible variations. In this case, we can select microlensing events from archive data rather than time domain monitoring the sky, which we describe as static microlensing. Following this concept, we collect the data from Gaia DR3 and SDSS DR16 from the northern galactic cap at high galactic latitudes. This area is not preferable for normal microlensing search due to the low stellar density and, therefore, low discovery rate. By applying a similarity search algorithm, we find 5 microlensing candidates in the Galactic halo.
format Preprint
id arxiv_https___arxiv_org_abs_2411_02161
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Static Microlensing: Concept, Method and Candidates
Guo, Qi
Wei, Leyao
Luo, Wentao
Lin, Shurui
Li, Qinxun
Cai, YiFu
He, Di
Wang, Qingqing
Yang, Ruoxi
Astrophysics of Galaxies
We propose a novel microlensing event search method that differs from either the traditional time domain method, astrometric microlensing, or the parallax microlensing method. Our method assumes that stars with nearly identical "genes" - normalized Spectral Energy Distributions (SED) bear the same luminosity within the intrinsic scatter due to stellar properties. Given a sample of stars with similar normalized SEDs, the outliers in luminosity distribution can be considered microlensing events by excluding other possible variations. In this case, we can select microlensing events from archive data rather than time domain monitoring the sky, which we describe as static microlensing. Following this concept, we collect the data from Gaia DR3 and SDSS DR16 from the northern galactic cap at high galactic latitudes. This area is not preferable for normal microlensing search due to the low stellar density and, therefore, low discovery rate. By applying a similarity search algorithm, we find 5 microlensing candidates in the Galactic halo.
title Static Microlensing: Concept, Method and Candidates
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2411.02161