2022RAA....22l5018L


Query : 2022RAA....22l5018L

2022RAA....22l5018L - Research in Astron. and astroph., 22, part no 12, 5018 (2022/December-1)

Machine Learning to Search for Accreting Neutron Star Binary Candidates Using Chinese Space Station Telescope Photometric System.

LAN S.-Y., JI K.-F. and MENG X.-C.

Abstract (from CDS):

Accreting neutron star binary (ANSB) systems can provide some important information about neutron stars (NSs), especially on the structure and the equation of state of NSs. However, only a few ANSBs are known so far. The upcoming Chinese Space Station Telescope (CSST) provides an opportunity to search for a large number of ANSB candidates. We aim to investigate whether or not a machine learning method may efficiently search for ANSBs based on CSST photometric system. In this paper, we generate some ANSBs and normal binaries under CSST photometric system by binary evolution and binary population synthesis method and use a machine learning method to train a classification model. We consider the classical multi-color disk and the irradiated accretion disk, then compare their effects on the classification results. We find that no matter whether the X-ray reprocessing effect is included or not, the machine learning classification accuracy is always very high, i.e., higher than 96%. If a significant magnitude difference exists between the accretion disk and the companion of an ANSB, machine learning may not distinguish it from some normal stars such as massive main sequence stars, white dwarf binaries, etc. False classifications of the ANSBs and the normal stars highly overlap in a color-color diagram. Our results indicate that machine learning would be a powerful way to search for potential ANSB candidates from the CSST survey.

Abstract Copyright: © 2022. National Astronomical Observatories

Journal keyword(s): stars: neutron - X-rays: binaries - methods: analytical

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0

Query : 2022RAA....22l5018L

Basic data :
SAX J1808.4-3658 -- Low Mass X-ray Binary
Other object types:
otypes_help
X (2022MNRAS,PBC,...), LXB (2013ApJS), * (2008ApJ,[RCM98]), Psr (PSR), N* (2014MNRAS), V* (V*), gam (INTREF), Rad ([GSG99])
ICRS coord. (ep=J2000) :
18 08 27.58 -36 58 43.9 (X-ray) [ 1500 1500 90 ] D 2020A&A...641A.136W
FK4 coord. (ep=B1950 eq=1950) :
18 05 03.50 -36 59 13.4 [ 1500 1500 90 ]
Gal coord. (ep=J2000) :
355.38517 -08.14832 [ 1500 1500 90 ]
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Identifiers (14) :
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INTREF 881 SWIFT J1808.5-3655 V* V4580 Sgr [GSG99] J180827.6-365843.9
PBC J1808.3-3656 SwXF4 J180827.6-365842 2XMM J180827.7-365841 [RCM98] J180827.5-365842
PSR J1808-3658 1SXPS J180827.6-365843 4XMM J180827.5-365843
SAX J1808.4-3658 2SXPS J180827.5-365842 XTE J1808-369

References (1051 between 1850 and 2026) (Total 1051)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Observing logs

XMM : 4   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : SAX J1808.4-3658

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V* V4580 Sgr

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