High-J CO survey of low-mass protostars observed with Herschel-HIFI

U. A. Yıldız; L. E. Kristensen; E. F. van Dishoeck; I. San José-García; A. Karska; D. Harsono; M. Tafalla; A. Fuente; R. Visser; J. K. Jørgensen; M. R. Hogerheijde

doi:10.1051/0004-6361/201220849

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Volume 556 (August 2013)

A&A, 556 (2013) A89

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Table C.1

Observed line intensities for L1448MM in all observed transitions.

Mol.	Transition	Telescope	Efficiency		T _peak	rms
			η	[K km s^-1]	[K]	[K]

CO	2–1	JCMT-RxA	0.69	59.71	8.26	0.10
	3–2	JCMT-HARPB	0.63	32.15	4.20	0.085
	4–3	JCMT	0.38	87.49	7.45	0.77
	6–5^a	APEX-CHAMP⁺	0.46	46.15	5.67	0.12
	10–9	Herschel-HIFI^b	0.64	21.53	...	0.15
¹³CO	2–1	JCMT-RxA	0.74	9.84	6.50	0.066
	3–2	JCMT-HARPB	0.63	5.74	2.70	0.065
	6–5	APEX-CHAMP⁺	0.48	2.88	2.69	0.34
	10–9	Herschel-HIFI^b	0.74	0.34	0.13	0.019
C¹⁸O	2–1	JCMT-RxA	0.69	3.53	2.35	0.061
	3–2	JCMT-HARPB	0.63	1.47	1.48	0.10
	5–4	Herschel-HIFI^b	0.76	0.42	0.45	0.018
	9–8	Herschel-HIFI^c	0.74	<0.052	...	0.023
	10–9	Herschel-HIFI^c	0.74	<0.055	...	0.024

Notes.

^(a)

Gomez-Ruiz et al. (in prep.)

^(b)

Only H-polarization observation is used.

^(c)

H- and V-polarization observations averaged.

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