Modelling telluric line spectra in the optical and infrared with an application to VLT/X-Shooter spectra

Free Access

Table 1

Objects and observational details for the objects discussed in this paper.


Object	m _J ^a	Start of observation	Mean	Mean	Exposure time [s]^b			Pipeline provided S/N
		(UTC)	seeing [′′]	airmass	UVB	VIS	NIR	UVB^c	VIS^d	NIR^e


EG 274	11.6	2010-May-05 03:24:44	0.68	1.26	1×90	1×120	1×120	299	190	71
MV Lup	9.6	2010-May-05 08:30:13	0.88	1.32	2×150	4×60	6×100	268	293	377
V895 Sco	10.1	2010-May-05 07:50:21	0.98	1.12	2×300	4×140	6×150	140	241	390
S CrA	8.2	2010-May-05 09:48:34	1.02	1.07	2×150	4×30	6×50	363	294	791

Notes.

^(a)

m_J from 2MASS (Skrutskie et al. 2006);

^(b)

except for EG 274 all observations were carried out in nodding mode, N× states the number of exposures taken in total at the different nodding positions;

^(c)

in region 4500−4700 Å;

^(d)

in region 7450−7560 Å;

^(c)

in region 15 140−15 480 Å.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.