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


Table 3

Results from the modeling of the studied disks, together with inferred sizes (R68% and R95%, in au), and total diskdust mass (Mdust).

Object log10 (I0) σ i PA ΔRA ΔDec R68% R95% Mdust
[Jy sr−1] [arcsec] [deg] [deg] [arcsec] [arcsec] [au] [au] [M]
BDs from this survey

J154518.5–342125 2.3 ± 0.2
                         
SONYC-Lup3–7 <17.5 <28.3 0.21 ± 0.02
                         
Lup706 <56.4 <91.4 0.35 ± 0.04
                         
AKC2006–18 <0.06
                         
SONYC-Lup3-10 <0.08

BDs from Lupus disks survey

Lup818s <12.1 <19.7 3.2 ± 0.3
                         
J161019.8-383607 <0.45
                         
J160855.3-384848 <21.7 <35.2 0.79 ± 0.08
                         
Lup607 <0.38


Object ρt γ β log10α Ftot i PA ΔRA ΔDec R68% R95% Mdust
[arcsec] [–] [–] [–] [mJy] [deg] [deg] [arcsec] [arcsec] [au] [au] [M]

Disks from Lupus disks completion survey

Sz102 6.1 ± 0.6
                         
V1094 Sco 230 ± 23
                         
GQ Lup 31.8 ± 3.2
                         
Sz76 4.9 ± 0.5
                         
Sz77 <55.5 <136 2.1 ± 0.2
                         
RXJ1556.1-3655 24.8 ± 2.5
                         
EX Lup 19.1 ± 1.9

Notes. The first 9 objects are the full list of known BDs in Lupus, fitted to a Gaussian model. The six free parameters are: normalization factor of the emission profile log I0, standard deviation of the Gaussian profile σ, inclination i, position angle PA, and right ascension and declination off-sets to the phase center of the observations ΔRA and ΔDec. The last 7 disks were fitted to a Nuker profile. The nine free parameters of these fits are: transition radius ρt, inner and outer slopes γ and β, smoothness parameter α, total disk flux density Ftot, and the geometrical parameters of the observation i, PA, ΔRA and ΔDec.

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