The Mrk 231 molecular outflow as seen in OH | Astronomy & Astrophysics (A&A)

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Volume 561 (January 2014)

A&A, 561 (2014) A27

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Table 1

Herschel/PACS observations of OH in Mrk 231.

Transition	Rest wavelengths^a	Program^b	Obs. ID^c	Number of	σ
	(μm)			spatial pixels^d	(Jy)

OH	119.233−119.441	GT	1342186811	1	0.29
OH	79.118−79.181	GT	1342186811	1	0.26
		GT	1342186811	1	0.26
		OT2	1342253536	1	0.23
OH	53.261−53.351	OT2	1342253530	1	0.24
OH	84.420−84.597	OT2	1342253537	3	0.50
OH	65.132−65.279	GT	1342207782	1	0.19
		GT	1342207782	3	0.24
		OT2	1342253532	3	0.25
OH	71.171−71.216	OT2	1342253534	3	0.36
OH	52.934−53.057	OT2	1342253530	1	0.24
OH	55.891−55.950	OT2	1342253531	3	0.19
OH	163.124−163.397	OT1	1342223369	1	0.25

Notes.

^(a)

The two values correspond to the two Λ-components of the doublets; each one is the average of the two hyperfine transitions that make up a component.

^(b)

GT and OT indicate “guaranteed time” and “open time”.

^(c)

Identification number.

^(d)

Number of spatial pixels used to generate the spectrum. In case of 1, the central pixel was used; in case of 3, the spectra from the three brightest spatial pixels were coadded. In all cases, the absolute fluxes were scaled to match the total flux as obtained by coadding the fluxes from the 25 pixels.

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