Atmospheric characterization of the ultra-hot Jupiter WASP-33b - Detection of Ti and V emission lines and retrieval of a broadened line profile

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Table 2

Observation log and instrument characteristics.

Instrument	Spectral resolution (R)	Wavelength range (Å)	Date	Phase coverage	Exposure time (s)	N_spectra
CARMENES	94 600 (VIS)	5200–9600	2017-11-15	0.29–0.65	300	95^(a)
	80400 (NIR)	9600–17100	2017-11-15	0.29–0.63	300	88^(a)

HARPS-N	115 000	3830–6900	2020-10-15	0.43–0.70	200	125
			2020-11-07	0.24–0.57	200	155

ESPaDOnS	68000	3700–10500	2013-09-15	0.30–0.44	90	110
			2013-09-26	0.37–0.44	90	55
			2014-09-04	0.56–0.69	90	110
			2014-09-15	0.55–0.68	90	110
			2014-11-05	0.31–0.38	90	55

Notes.^(a) Total number of CARMENES spectra was 105; due to their poor quality ten spectra were removed from the time series of the VIS channel and 17 spectra were removed from the time series of the NIR channel.

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