A new look at the long-period eclipsing binary V383 Scorpii

Free Access

Table 3

Frequencies and periods obtained with Fourier analysis of the out-of-eclipse V-band light curve.

Frequency [1/d]	Amplitude	Period [d]	σ [d]

0.00503	0.000375	198.8	4.8
0.01004	0.000262	99.6	1.5
0.01507	0.000182	66.36	0.49

Notes. The errors σ were estimated using the HWHM^* of peaks in the power spectrum.

^(*)

Half width at half maximum.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.