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 3

Summary of cross-correlation results.

Species	S/N	SYSREM iteration	Instruments included	Wavelength range (Å)
TiI	6.3	3	CV, CN, H, E	3700–17 100
VI	4.8	3	CV, H, E	3700–9600
OH	4.4	3	CN	9600–17 100
Fe i	7.9	10	CV, CN, H, E	3700–17 100
SiI	4.4	4	CN	9600–17 100
Ti ii	3.6	1	H	3830–6900
VII	No detection		H, E	3700–10500
Fe ii	No detection		H, E	3700–10500
SiII	No detection		H, E	3700–10500

Combined	8.5	9	CV, CN, H, E	3700–17 100

Notes. For each species, only those instruments predicted to have prominent emission lines in their wavelength range were included. We use the following abbreviations: CARMENES VIS (CV), CARMENES NIR (CN), HARPS-N (H), and ESPaDOnS (E).

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