On the properties of dust and gas in the environs of V838 Monocerotis

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Table 1

Herschel observations.

PACS

Date, epoch^a	Obs. id.^b	λ reference (μm)^c
m.d.20xx

05.07.11, 1	1342220129, 30	phot: 70, 160
	1342220131, 2	phot: 100, 160
	1342220136	spec: 79.36, 162.81
		165.95, 177.77
	1342220137	spec: 179.53, 180.78
		169.68, 71.07
	1342220138	spec: 118.58, 108.07
05.01.12, 2	1342245206, 7	phot: 70, 160
	1342245208, 9	phot: 100, 160
10.16.12, 3	1342253505, 6	phot: 70, 160
	1342253507, 8	phot: 100, 160

SPIRE

09.18.10, 1	1342204851	phot: 250, 350, 500
04.24.11, 1	1342219551	spec: 194–671
04.30.12, 2	1342245152	phot: 250, 350, 500
10.14.12, 3	1342253396	phot: 250, 350, 500

HIFI

		Setting; bandν (GHz)^d

09.13.11, 1.5	1342228563	A; 1b606.752-610.884
		618.745-622.877
09.30.11, 1.5	1342229897	B; 2a678.314-682.445
		690.307-694.439
09.14.11, 1.5	1342228604	C; 5a1149.527-1153.658
		1161.520-1165.651
10.09.11, 1.5	1342230404	D; 7a1759.995-1762.558
		1767.243-1769.806
09.29.11, 1.5	1342229843	E; 7b1789.211-1791.774
		1796.459-1799.022

Notes.

^(a)

Epoch: a counter based on the PACS observation dates; for SPIRE and HIFI the closest epoch to these is indicated.

^(b)

Obs. Id refers to the unique reference number given to all Herschel observations.

^(c)

phot = photometer, spec = spectrometer.

^(d)

WBS ranges in LSB and USB.

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