Do siblings always form and evolve simultaneously? Testing the coevality of multiple protostellar systems through SEDs

N. M. Murillo; E. F. van Dishoeck; J. J. Tobin; D. Fedele

doi:10.1051/0004-6361/201628247

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Volume 592 (August 2016)

A&A, 592 (2016) A56

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Table 3

StarFinder photometry parameters.

Regions	Wavelength	Beam size^a	PSF aperture^b	FWHM ^c	Deblend^d	Flux uncertainty
	μm	″	″			mJy

NGC 1333, B1, IC 348	70	9.6	13.0	1.0	N	20–30
...	100	7.2	8.0	1.0	N	7–10
...	160	12.8	13.0	1.0	N	10–15
L1448, L1455	70	9.6	13.0	0.7	Y	24–34
...	100	7.2	8.0	0.7	Y	8–16
...	160	12.8	13.0	0.7	Y	11–20

Notes.

^(a)

Measured from the FWHM of the extracted PSF.

^(b)

This refers to the mask applied to the PSF to include the PSF sidelobes.

^(c)

Parameter to determine the smallest separation between close sources in terms of the FWHM.

^(d)

Switch parameter to set whether detected sources are deblended.

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