Characterising the magnetospheric accretion process of DF Tauri’s primary

Open Access

Table 1.

ESPaDOnS observations of DF Tau.

Date	HJD	S/N_I	S/N_LSD	V_r
(2011)	(−2 450 000 d)			(km s⁻¹)
01 Nov	5866.98	113	2223	16.96 ± 0.28
05 Nov	5870.99	77	1211	18.15 ± 0.06
06 Nov	5871.96	31	714	15.68 ± 0.52
07 Nov	5873.01	77	1431	17.85 ± 0.13
09 Nov	5874.93	171	1718	19.92 ± 0.16
11 Nov	5876.97	154	2059	17.31 ± 0.30
13 Nov	5878.94	164	2097	13.20 ± 0.23
14 Nov	5879.90	173	2675	20.16 ± 0.05
15 Nov	5880.97	172	2990	14.99 ± 0.06
16 Nov	5882.07	166	2734	17.79 ± 0.16

Notes. S/N_I is the peak S/N by spectral pixel at order 31 (730 nm), S/N_LSD corresponds to the effective S/N of the LSD Stokes I profiles (see Sect. 3.3), and V_r corresponds to the radial velocity of the primary computed from the 2D CCF (see Sect. 3.1).

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.