scholarly journals The Orbital Parameters of the Eclipsing High-mass X-Ray Binary Pulsar IGR J16493–4348 from Pulsar Timing

2019 ◽  
Vol 873 (1) ◽  
pp. 86 ◽  
Author(s):  
Aaron B. Pearlman ◽  
Joel B. Coley ◽  
Robin H. D. Corbet ◽  
Katja Pottschmidt
2002 ◽  
Vol 581 (2) ◽  
pp. 1293-1296 ◽  
Author(s):  
Paul S. Ray ◽  
Deepto Chakrabarty
Keyword(s):  
X Ray ◽  

2014 ◽  
Vol 335 (10) ◽  
pp. 1060-1063 ◽  
Author(s):  
K. A. Stoyanov ◽  
R. K. Zamanov ◽  
G. Y. Latev ◽  
A. Y. Abedin ◽  
N. A. Tomov
Keyword(s):  
X Ray ◽  

2021 ◽  
Vol 42 (2) ◽  
Author(s):  
Gaurava K. Jaisawal ◽  
Sachindra Naik ◽  
Prahlad R. Epili ◽  
Birendra Chhotaray ◽  
Arghajit Jana ◽  
...  
Keyword(s):  
X Ray ◽  

2005 ◽  
Vol 440 (3) ◽  
pp. 1033-1039 ◽  
Author(s):  
L. Sidoli ◽  
S. Mereghetti ◽  
S. Larsson ◽  
M. Chernyakova ◽  
I. Kreykenbohm ◽  
...  
Keyword(s):  
X Ray ◽  

2021 ◽  
Vol 42 (2) ◽  
Author(s):  
Parisee Shirke ◽  
Suman Bala ◽  
Jayashree Roy ◽  
Dipankar Bhattacharya
Keyword(s):  
X Ray ◽  

2004 ◽  
Vol 194 ◽  
pp. 220-220
Author(s):  
M. T. Menna ◽  
A. Papitto ◽  
L. Burderi ◽  
T. Di Salvo ◽  
L. Stella ◽  
...  

We analyzed RXTE data from the burst of the year 2000 of the X-ray millisecond binary pulsar SAX J 1808.4-3658 with the intent of determining the new orbital parameters.We used the observations of SAX J1808.4-3658 performed by the Rossi X-Ray Timing Explorer (RXTE) when the source was again detected in outburst during the period January-March 2000 (Wijnands et al. 2001). In particular we examined the data from the Proportional Counter Array (РСA) (Jahoda et al. 1996). We first applied barycentric correction to the data using the optical coordinates of the source (Roche et al. 98).


2011 ◽  
Vol 737 (2) ◽  
pp. 79 ◽  
Author(s):  
Sachindra Naik ◽  
Biswajit Paul ◽  
Zulfikar Ali
Keyword(s):  
X Ray ◽  

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