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Observations of the 599 Hz Accreting X-Ray Pulsar IGR J00291+5934 during the 2004 Outburst and in Quiescence

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M. A. P. Torres1, P. G. Jonker1,2,3, D. Steeghs1, G. H. A. Roelofs4, J. S. Bloom5, J. Casares6, E. E. Falco1, M. R. Garcia1, T. R. Marsh7, M. Mendez2,3,8, J. M. Miller1,9, G. Nelemans4 and P. Rodríguez-Gil6

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[1]

A Double Outburst from IGR J00291+5934: Implications for Accretion Disk Instability Theory

Jacob M. Hartman et al.  The Astrophysical Journal 2011  726 26
IOPscience 
[2]

The Accreting Millisecond X-ray Pulsar IGR J00291+5934: Evidence for a Long Timescale Spin Evolution

Alessandro Patruno  The Astrophysical Journal 2010  722 909
IOPscience 
[3]

Further Constraints on Thermal Quiescent X-Ray Emission from SAX J1808.4-3658

C. O. Heinke et al.  The Astrophysical Journal 2009  691 1035
IOPscience 
[4]

XMM-Newton Observations of IGR J00291+5934: Signs of a Thermal Spectral Component during Quiescence

Sergio Campana et al  The Astrophysical Journal Letters 2008  689 L129
IOPscience 
[5]

Optical and X-Ray Observations of IGR J00291+5934 in Quiescence

P. G. Jonker et al.  The Astrophysical Journal 2008  680 615
IOPscience 
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