A spectroscopic and kinematic survey of fast hot subdwarfs

Open Access

Table 1.

Summary of follow-up observations during the course of the MUCHFUSS project.

Date	Nights	Telescope & Instrument	Resolution [λ/Δλ]	Coverage [Å]	Observer
2015/08/20–2015/08/22	3	ING-WHT+ISIS	2000	3440–5270	T. K.
2015/09/04–2015/09/06	3	CAHA-3.5m+TWIN	4000	3460–5630	M.S., S.K.
2016/12/27–2016/12/31	3	ING-WHT+ISIS	2000	3440–5270	S. B.
2017/04/18–2017/04/21	4	ESO-NTT+EFOSC2	600	3270–5240	S. K.
2017/07/24–2017/07/26	3	ING-WHT+ISIS	2000	3440–5270	D.S., S.G.
2018/01/03–2018/01/05	3	ING-WHT+ISIS	2000	3440–5270	S. B.
2015, 2016, 2019	3.5	ESO-VLT+X-shooter	4000	3000–10 000	Service
2017/2018	2.5	GTC+OSIRIS	1000	3600–7500	Service
2018/05/15	1	Keck+ESI	7000	4000–10 000	T. K.

		Palomar-5m+DBSP ^(a)	1500	3800–5700	T. K.
		Keck+LRIS ^(a)	900	3200–5600	T. K.

Notes.

^(a)

Observations obtained as backup during other projects. The spectra were reduced with different standard software packages such as IRAF and MIDAS. The LRIS, ESI and X-shooter spectra were reduced using pipelines provided by the Mauna Kea observatory and ESO, respectively.

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