2011
DOI: 10.1051/0004-6361/201117841
|View full text |Cite
|
Sign up to set email alerts
|

A search for the near-infrared counterpart of the eclipsing millisecond X-ray pulsar Swift J1749.4–2807

Abstract: Context. Swift J1749.4-2807 is a transient accreting millisecond X-ray pulsars and the first to display X-ray eclipses. It therefore holds a strong potential for accurate mass measurements in a low-mass X-ray binary system. Aims. Determining the companion star's radial velocity would make it possible to fully resolve the system and to accurately measure the mass of the neutron star based on dynamical measurements. Unfortunately, no optical or near infrared (NIR) counterpart has been identified to date for this… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
4
0

Year Published

2012
2012
2022
2022

Publication Types

Select...
3
2
2

Relationship

0
7

Authors

Journals

citations
Cited by 9 publications
(5 citation statements)
references
References 34 publications
1
4
0
Order By: Relevance
“…Combining the 0.7 ′′ statistical uncertainty of the detection routine with the estimated 1.5 ′′ MOS systematic error (Watson et al 2009), yields a positional uncertainty of 1.7 ′′ (90% confidence). The XMM-Newton coordinates are offset by ≃2.9-3.3 ′′ from the 1.6-1.9 ′′ Swift localization (90% confidence; Yang et al 2010;D'Avanzo et al 2011), but consistent within the errors.…”
Section: X-ray Image and Light Curvesupporting
confidence: 56%
See 1 more Smart Citation
“…Combining the 0.7 ′′ statistical uncertainty of the detection routine with the estimated 1.5 ′′ MOS systematic error (Watson et al 2009), yields a positional uncertainty of 1.7 ′′ (90% confidence). The XMM-Newton coordinates are offset by ≃2.9-3.3 ′′ from the 1.6-1.9 ′′ Swift localization (90% confidence; Yang et al 2010;D'Avanzo et al 2011), but consistent within the errors.…”
Section: X-ray Image and Light Curvesupporting
confidence: 56%
“…The mass donor in Swift J1749.4-2807 is a main sequence star of spectral type K-G D'Avanzo et al 2011). This holds good prospects for studying the radial velocity curve of the companion in quiescence.…”
Section: Introductionmentioning
confidence: 99%
“…In several AMXPs, the optical counterpart during X-ray quiescence appears surprisingly luminous, inconsistent with both intrinsic emission from the companion star and X-ray reprocessing (e.g. [58,33,34]). In fact, the optical counterpart shows an approximately sinusoidal modulation with photometric minimum at the superior conjunction of the pulsar.…”
Section: Summary and Open Questionsmentioning
confidence: 94%
“…The X-ray light-curve showed an exponential decay with a Swift/XRT non detection after 11 days since its first 2010 observation. Due to the crowded field (the source is on the Galactic plane), no single counterpart has been identified in NIR counterpart searches [72]. More than forty counterparts were identified in the X-ray error circle with ESO's Very Large Telescope (VLT).…”
Section: Swift J17494-2807mentioning
confidence: 99%