Identification of new transitional disk candidates in Lupus with Herschel

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Volume 578 (June 2015)

A&A, 578 (2015) A23

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Table 4

Same as Table 3, but with MIPS70 possible contamination.

Object	F_source/F_aper	N	Companion distance (′′)	Band


Sz66	468.^mJy	1	6.2	PACS70
Sz98²	0.2	1	26.3	SPIRE350
Sz100²	0.7	1	32.3	SPIRE500
Sz103¹	1.4	1	23.2	SPIRE350
Sz104¹	0.7	1	23.2	SPIRE350
Sz108B	212.^mJy	1	9.7	PACS70
2MASSJ1608537^*	119.0^mJy	1	6.9	PACS70
Sz112²	0.7	1	28.6	SPIRE350

Notes.

⁽¹⁾

The MIPS70 contamination in Sz103 is caused by Sz104, and vice versa, as can be seen in Fig. 4. This is taken into account in the photometry analysis.

⁽²⁾

Objects with sufficiently low contamination from nearby sources so as to not affect our Herschel measurements.

^(*)

This is the only object that has been removed from the list of detected sources, because its Herschel photometry cannot be unequivocally associated with it.

^(mJy)

In these cases the MIPS photometry of the target was not available, but that of the companions was. Therefore, we present the actual flux of the objects inside the search radius instead of the percentage.

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