False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise

We report observations of four asteroid-crossing events in Transiting Exoplanet Survey Satellite light curves masquerading as self-lensing pulses from binary systems containing main-sequence stars and black hole or neutron-star companions. The observed changes in flux and the durations of the events...

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Main Authors: Nicholas M. Sorabella, Silas G. T. Laycock, Liam J. Neeley, Dimitris M. Christodoulou, Sayantan Bhattacharya
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ace9df
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author Nicholas M. Sorabella
Silas G. T. Laycock
Liam J. Neeley
Dimitris M. Christodoulou
Sayantan Bhattacharya
author_facet Nicholas M. Sorabella
Silas G. T. Laycock
Liam J. Neeley
Dimitris M. Christodoulou
Sayantan Bhattacharya
author_sort Nicholas M. Sorabella
collection DOAJ
description We report observations of four asteroid-crossing events in Transiting Exoplanet Survey Satellite light curves masquerading as self-lensing pulses from binary systems containing main-sequence stars and black hole or neutron-star companions. The observed changes in flux and the durations of the events appear to be consistent with self-lensing pulses provided that (a) the compact-object mass is greater than 2 solar masses, and (b) the transit is not a perfect alignment, i.e., the center of the lens is not passing directly in front of the center of the source. We examine the relationship between the physical characteristics of these asteroid crossings and the derived parameters of our self-lensing model fits to the data sets. As the search for new self-lensing systems continues, we caution observers about such false-positive signals imitating real self-lensing pulses.
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spelling doaj.art-a0701a0fd59f4d98a895191e4a12a8862023-09-03T13:24:42ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0195415910.3847/1538-4357/ace9dfFalse-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in DisguiseNicholas M. Sorabella0https://orcid.org/0000-0002-3562-9699Silas G. T. Laycock1https://orcid.org/0000-0002-8427-0766Liam J. Neeley2https://orcid.org/0000-0002-4993-992XDimitris M. Christodoulou3https://orcid.org/0000-0002-7652-2206Sayantan Bhattacharya4https://orcid.org/0000-0001-8572-8241Lowell Center for Space Science and Technology , Lowell, MA 01854, USA ; nicholas_sorabella@student.uml.edu; Department of Physics and Applied Physics, University of Massachusetts Lowell , Lowell, MA 01854, USALowell Center for Space Science and Technology , Lowell, MA 01854, USA ; nicholas_sorabella@student.uml.edu; Department of Physics and Applied Physics, University of Massachusetts Lowell , Lowell, MA 01854, USALowell Center for Space Science and Technology , Lowell, MA 01854, USA ; nicholas_sorabella@student.uml.edu; Department of Physics and Applied Physics, University of Massachusetts Lowell , Lowell, MA 01854, USALowell Center for Space Science and Technology , Lowell, MA 01854, USA ; nicholas_sorabella@student.uml.eduLowell Center for Space Science and Technology , Lowell, MA 01854, USA ; nicholas_sorabella@student.uml.edu; Department of Physics and Applied Physics, University of Massachusetts Lowell , Lowell, MA 01854, USAWe report observations of four asteroid-crossing events in Transiting Exoplanet Survey Satellite light curves masquerading as self-lensing pulses from binary systems containing main-sequence stars and black hole or neutron-star companions. The observed changes in flux and the durations of the events appear to be consistent with self-lensing pulses provided that (a) the compact-object mass is greater than 2 solar masses, and (b) the transit is not a perfect alignment, i.e., the center of the lens is not passing directly in front of the center of the source. We examine the relationship between the physical characteristics of these asteroid crossings and the derived parameters of our self-lensing model fits to the data sets. As the search for new self-lensing systems continues, we caution observers about such false-positive signals imitating real self-lensing pulses.https://doi.org/10.3847/1538-4357/ace9dfAsteroidsCompact binary starsGravitational microlensing
spellingShingle Nicholas M. Sorabella
Silas G. T. Laycock
Liam J. Neeley
Dimitris M. Christodoulou
Sayantan Bhattacharya
False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
The Astrophysical Journal
Asteroids
Compact binary stars
Gravitational microlensing
title False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
title_full False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
title_fullStr False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
title_full_unstemmed False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
title_short False-positive Self-lensing Events: TESS Observing Asteroid-crossing Events in Disguise
title_sort false positive self lensing events tess observing asteroid crossing events in disguise
topic Asteroids
Compact binary stars
Gravitational microlensing
url https://doi.org/10.3847/1538-4357/ace9df
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