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Cited article:

The Multi-INstrument Burst ARchive (MINBAR)

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The Astrophysical Journal Supplement Series 249 (2) 32 (2020)
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Insight-HXMT Observations of 4U 1636-536: Corona Cooling Revealed with Single Short Type-I X-Ray Burst

Y. P. Chen, S. Zhang, J. L. Qu, S. N. Zhang, L. Ji, L. D. Kong, X. L. Cao, Z. Chang, G. Chen, L. Chen, T. X. Chen, Y. Chen, Y. B. Chen, W. Cui, W. W. Cui, J. K. Deng, Y. W. Dong, Y. Y. Du, M. X. Fu, G. H. Gao, H. Gao, M. Gao, M. Y. Ge, Y. D. Gu, J. Guan, et al.
The Astrophysical Journal Letters 864 (2) L30 (2018)
https://doi.org/10.3847/2041-8213/aadc0e

Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra

J. Nättilä, M. C. Miller, A. W. Steiner, et al.
Astronomy & Astrophysics 608 A31 (2017)
https://doi.org/10.1051/0004-6361/201731082

Probing the accretion disc structure by the twin kHz QPOs and spins of neutron stars in LMXBs

D. H. Wang, C. M. Zhang, Y. J. Lei, et al.
Monthly Notices of the Royal Astronomical Society 466 (1) 1111 (2017)
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Probing the effects of a thermonuclear X-ray burst on the neutron star accretion flow withNuSTAR

N. Degenaar, K. I. I. Koljonen, D. Chakrabarty, et al.
Monthly Notices of the Royal Astronomical Society 456 (4) 4256 (2016)
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DETERMINING NEUTRON STAR PROPERTIES BY FITTING OBLATE-STAR WAVEFORM MODELS TO X-RAY BURST OSCILLATIONS

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The Astrophysical Journal 808 (1) 31 (2015)
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EVIDENCE FOR ENHANCED PERSISTENT EMISSION DURING SUB-EDDINGTON THERMONUCLEAR BURSTS

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The Astrophysical Journal 801 (1) 60 (2015)
https://doi.org/10.1088/0004-637X/801/1/60

The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

Jari J. E. Kajava, Joonas Nättilä, Outi-Marja Latvala, et al.
Monthly Notices of the Royal Astronomical Society 445 (4) 4218 (2014)
https://doi.org/10.1093/mnras/stu2073