Fetching the paper…
Reading the bibliography…
The vast majority of known non-accreting neutron stars (NSs) are rotation-powered radio and/or gamma-ray pulsars.
J. M. Dickey, F. J. Lockman, ARA&A
1990
Earlier work this paper cites.
J. H. Taylor, J. M. Cordes, ApJ
1993
Earlier work this paper cites.
H. Ruder, G. Wunner, H. Herold, F. Geyer, Atoms in Strong Magnetic Fields. Quantum Mechanical Treatment and Applications in Astrophysics and Quantum Chaos
1994
Earlier work this paper cites.
G. G. Pavlov, Y. A. Shibanov, V. E. Zavlin, R. D. Meyer, The Lives of the Neutron Stars
1995
Earlier work this paper cites.
K. A. Arnaud, Astronomical Data Analysis Software and Systems V
1996
Earlier work this paper cites.
M. Rajagopal, R. W. Romani, ApJ
1997
Earlier work this paper cites.
M. A. McLaughlin, et al
2002
Earlier work this paper cites.
J. M. Cordes, T. J. W. Lazio, ArXiv Astrophysics e-prints
2002
Earlier work this paper cites.
G. G. Pavlov, V. E. Zavlin, D. Sanwal, Neutron Stars, Pulsars, and Supernova Remnants
2002
Earlier work this paper cites.
D. Sanwal, G. G. Pavlov, V. E. Zavlin, M. A. Teter, ApJ
2002
Earlier work this paper cites.
R. Protassov, D. A. van Dyk, A. Connors, V. L. Kashyap, A. Siemiginowska, ApJ
2002
Cited alongside, same era.
M. H. van Kerkwijk, D. L. Kaplan, M. Durant, S. R. Kulkarni, F. Paerels, ApJ
2004
Cited alongside, same era.
F. Haberl, V. E. Zavlin, J. Trümper, V. Burwitz, A&A
2004
Cited alongside, same era.
P. M. W. Kalberla, et al
2005
Cited alongside, same era.
A. De Luca, P. A. Caraveo, S. Mereghetti, M. Negroni, G. F. Bignami, ApJ
2005
Cited alongside, same era.
M. van Adelsberg, D. Lai, A. Y. Potekhin, P. Arras, ApJ
2005
Cited alongside, same era.
M. S. Jackson, J. P. Halpern, ApJ
K. Mori, W. C. G. Ho, MNRAS
2007
Later among the works it cites.
Q. Luo, D. Melrose, MNRAS
2007
Later among the works it cites.
O. Kargaltsev, Z. Misanovic, G. G. Pavlov, J. A. Wong, G. P. Garmire, ApJ
2008
Later among the works it cites.
E. V. Gotthelf, J. P. Halpern, ApJ
2009
Later among the works it cites.
V. M. Kaspi, Proceedings of the National Academy of Science
2010
Later among the works it cites.
D. L. Kaplan, A. Kamble, M. H. van Kerkwijk, W. C. G. Ho, ApJ
2011
Later among the works it cites.
V. Hambaryan, et al
2011
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
2005
Cited alongside, same era.
R. N. Manchester, G. B. Hobbs, A. Teoh, M. Hobbs, AJ
2005
Cited alongside, same era.
A. K. Harding, D. Lai, Reports on Progress in Physics
2006
Cited alongside, same era.
A simpler model, BB+PL, does not produce a satisfactory fit
Cited in the paper.
This N H N_{\rm H} value is used in all the subsequent phase-resolved spectral fits because having N H N_{\rm H} tied and fitting for it in the phase-resolved spectra results in a similar but more uncertain value
Cited in the paper.
N. Bucciantini, J. Arons, E. Amato, MNRAS
2011
Later among the works it cites.
V. F. Suleimanov, G. G. Pavlov, K. Werner, ApJ
2012
Closest in time.