Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)

Home

All issues

Volume 559 (November 2013)

A&A, 559 (2013) A47

Full HTML

Highlight

Free Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201321096e]

Table 111

Number of detected lines and fraction of identified lines compared to previous surveys of Sgr B2.

Survey^a	Telescope	Source	Coverage^b	N_det^c	N_id^d	n_det^e	n_id^f	n_u^g	f_id^h
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)

C86	BTL 7 m	OH	72–144 (49)	457	426	9.3	8.7	0.6	0.93
T89	NRAO 11 m	OH	70–115 (45)	641	470	14.2	10.4	3.8	0.73
S91	CSO 10.4 m	M	330–355 (25)	128	127	5.1	5.1	0.0	0.99
N98	SEST 15 m	M	218–264 (45)	660	609	14.7	13.5	1.2	0.92
B13	IRAM 30 m	M	80–116 (36)	945	444	26.3	12.3	14.0	0.47

N98	SEST 15 m	N	218–264 (45)	1730	1393	38.4	31.0	7.4	0.81
F04	BIMA	N	86–113 (3.6)	218	98	60.6	27.2	33.4	0.45
B13	IRAM 30 m	N	80–116 (36)	3675	2573	102.1	71.5	30.6	0.70

Notes.

^(a)

See footnote of Table 110. The large telescope beams of the C86 and T89 surveys pointed toward Sgr B2(OH) include Sgr B2(M) (see Fig. 1 of Friedel et al. 2004).

^(b)

The edges of the observed band are given in GHz. Since the band was not always fully covered, the effective bandwidth is given in parentheses.

^(c)

Total number of detected lines.

^(d)

Total number of identified lines.

^(e)

Average number of detected lines per GHz.

^(f)

Average number of identified lines per GHz.

^(g)

Average number of unidentified lines per GHz.

^(h)

Fraction of identified lines.

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.