Short-term variability and mass loss in Be stars - III. BRITE and SMEI satellite photometry of 28 Cygni

D. Baade; A. Pigulski; Th. Rivinius; A. C. Carciofi; D. Panoglou; M. R. Ghoreyshi; G. Handler; R. Kuschnig; A. F. J. Moffat; H. Pablo; A. Popowicz; G. A. Wade; W. W. Weiss; K. Zwintz

doi:10.1051/0004-6361/201731187

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Volume 610 (February 2018)

A&A, 610 (2018) A70

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Table 2

BRITE photometry of 28 Cyg with satellite BTr in 2015.

HJD − 2 457 000	Flux
[d]	[mag]
184.6737	+0.007
184.7420	–0.009
184.8098	–0.023
184.8782	–0.016
184.9476	–0.010

Notes. The zeropoint of the BRITE magnitude scale is arbitrary (complete table available from CDS).

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