Detection of new eruptions in the Magellanic Clouds luminous blue variables R 40 and R 110

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Table 1

High-resolution spectra used in our study.

Star	Inst.	Date	t_exp (s)
RMC 40	UVES	2000-07-09	1 × 600
	UVES	2002-05-06	1 × 360
	FEROS	2005-12-12*	2 × 450
	FEROS	2006-10-11	2 × 1000
	FEROS	2007-10-05*	2 × 450
	FEROS	2008-08-04	2 × 1800
	FEROS	2014-11-28*	2 × 700
	FEROS	2015-12-04*	2 × 500
	FEROS	2016-11-02*	2 × 500

RMC 110	FEROS	2005-12-12*	2 × 450
	FEROS	2007-02-20	7 × 200
	FEROS	2014-12-04*	2 × 400
	FEROS	2016-01-13*	2 × 700

Notes. The spectra marked with an asterisk were observed by us and the others were obtained from ESO public data archive. The exposure time is associated with the number of spectra obtained.

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