Demographics of disks around young very low-mass stars and brown dwarfs in Lupus

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Volume 633 (January 2020)

A&A, 633 (2020) A114

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201936913e]

Table 2

Inferred fluxes for all the studied disks.

Object	F_cont	I_peak	rms
	[mJy]	[mJy beam⁻¹]	[mJy beam⁻¹]
BDs from this survey

J154518.5-342125	5.75	5.39	0.12
SONYC-Lup3-7	0.52	0.59	0.07
Lup706	0.79	0.70	0.10
AKC2006-18	<0.23	–	0.08
SONYC-Lup3-10	< 0.24	–	0.07

BDs from Lupus disks survey

Lup818s	7.44	7.40	0.24
J161019.8-383607	<1.24	–	0.23
J160855.3-384848	1.81	1.81	0.26
Lup607	<0.95	–	0.24

Disks from Lupus disks completion survey

Sz102	13.72	8.63	0.34
V1094 Sco	553.17	26.55	0.37
GQ Lup	78.43	44.91	0.34
Sz76	10.91	5.14	0.35
Sz77	4.88	3.73	0.20
RXJ1556.1-3655	56.39	18.93	0.35
EX Lup	43.47	11.11	0.35

Notes. From top to bottom: the nine protoplanetary disks around BDs (five from the new Lupus BDs disks survey) and seven additional disks from the Lupus disks completion survey. The columns are the total disk flux (F_cont), peak intensity (I_peak) of each object, and the rms of their continuum maps.

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