Evolution of the stellar-merger red nova V1309 Scorpii: Spectral energy distribution analysis

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Table 1

Fluxes of V1309 Sco measured with Herschel in March 2012.

Instr.	PSF^a	Band	λ_eff^b	Δλ^c	Flux	Error^d
					density
	(′′)		(μm)		(mJy/beam)

PACS	5.5	blue 70 μm	68.3	21.4	1 249.9	14.7
PACS	6.7	green 100 μm	97.9	31.3	617.3	38.5
PACS	11.5	red 160 μm	153.9	69.8	216.2	46.8
SPIRE	18.2	PSW 250 μm	242.8	67.6	81.3	2.5
SPIRE	24.9	PMW 350 μm	340.9	95.8	43.4	2.9
SPIRE	36.3	PLW 500 μm	482.3	185.8	<56.1

Notes.

^(a)

Full-width at half-maximum of the point spread function.

^(b)

Effective wavelength of the band (calculated for the Vega spectrum).

^(c)

Equivalent width of the band.

^(d)

Approximate photometry error.

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