The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data

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Volume 611 (March 2018)

A&A, 611 (2018) A85

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Table 2

Time-series photometry.

Telescope/instrument	Observers	# runs	# hours
Previous data (1999–2006)¹		168	421.3

Loiano 1.5m/BFOSC	RS	20	75.4
Piszkéstető 1.0m/CCD	MP/LM	14	67.5
Moletai 1.6m/CCD	RJ	26	79.4
Wise 1.0m/CCD	EL	6	35.7
Lulin 1.0m/CCD	WSH	7	24.2
MDM 1.3m/CCD	MR	7	33.4
LOAO 1.0m/CCD	SLK	47	134.1
Monet-N 1.2m/CCD	SS/RL	20	55.0
Baker 0.6m??/CCD	MR	4	11.5
Mercator 1.2m/CCD	RØ+students	24	69.8
WHT 4.2m/ULTRACAM	TRM/VSD	7	36.7
NOT 2.6m/ALFOSC	RØ	3	11.2
TNG 3.6m/DOLORES	RS	8	18.7
Calar Alto 2.2m/CAFOS	SS/RL	10	25.9

Total new data (2007–2012)		203	644.9²
All data (1999–2012)		371	1066.2

Notes. ⁽¹⁾ See SSJ07 Supplementary Information for more details (a Monet-N run of November 2006 was added to that list). ⁽²⁾ This number is smaller than the sum of Col. 4 given that sometimes overlapping data from different telescopes were averaged using a weighted mean.

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