Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network
A contact binary may be the progenitor of a red nova that eventually produces a merger event and have a cut-off period of around 0.2 days. Therefore, a large number of contact binaries is needed to search for the progenitor of red novae and to study the characteristics of short-period contact binari...
Main Authors: | Xu Ding, ZhiMing Song, ChuanJun Wang, KaiFan Ji |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astronomical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-3881/ad3048 |
Similar Items
-
Detection of Semidetached Eclipsing Binaries from TESS
by: Xu Ding, et al.
Published: (2025-01-01) -
Short-period Heartbeat Binaries from TESS Full-frame Images
by: Siddhant Solanki, et al.
Published: (2024-01-01) -
Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries
by: Xu-Zhi Li, et al.
Published: (2024-01-01) -
Photometric and Spectroscopic Analysis of Eight Totally Eclipsing Contact Binaries with Small Mass Ratios
by: Li-Heng Wang, et al.
Published: (2024-01-01) -
A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey
by: JinLiang Wang, et al.
Published: (2024-01-01)