MAXI J1820+070 with NuSTAR I. An increase in variability frequency but a stable reflection spectrum: coronal properties and implications for the inner disc in black hole binaries. Buisson, D., Fabian, A., Barret, D., Fürst, F., Gandhi, P., Garcı́a, J.~A., Kara, E., Madsen, K., Miller, J., Parker, M., Shaw, A., Tomsick, J., & Walton, D. \mnras, 490(1):1350-1362, November, 2019. doi bibtex @ARTICLE{2019MNRAS.490.1350B,
author = {{Buisson}, D.~J.~K. and {Fabian}, A.~C. and {Barret}, D. and {F{\"u}rst}, F. and {Gandhi}, P. and {Garc{\'\i}a}, J.~A. and {Kara}, E. and {Madsen}, K.~K. and {Miller}, J.~M. and {Parker}, M.~L. and {Shaw}, A.~W. and {Tomsick}, J.~A. and {Walton}, D.~J.},
title = "{MAXI J1820+070 with NuSTAR I. An increase in variability frequency but a stable reflection spectrum: coronal properties and implications for the inner disc in black hole binaries}",
journal = {\mnras},
keywords = {accretion, accretion discs, black hole physics, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena},
year = 2019,
month = nov,
volume = {490},
number = {1},
pages = {1350-1362},
doi = {10.1093/mnras/stz2681},
archivePrefix = {arXiv},
eprint = {1909.04688},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.1350B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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