DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs

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Volume 685 (May 2024)

A&A, 685 (2024) A65

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Table 3

Catalogue of ALMA observations on which we applied DBNets.

Disc name	Star mass (M_⊙)	Distance (pc)	Inclination (º)	Position angle (º)	Resolution(1) (a)	ALMA band	Gap radial location(s) a (au)	Data references	Properties references	Bae et al. (2023) M_P (M_J)	DBNets M_P (M_J)
AS 209	0.83	121	35	86	0.22, 0.02	6	9, 99	a	1	0.083, 2.05	${1.20}_{- 0.38}^{+ 0.50},^{()} {0.54}_{- 0.25}^{+ 0.43}$ $1.20_{ - 0.38}^{ + 0.50}{,^{()}}0.54_{ - 0.25}^{ + 0.43}$
Elias 2-24	0.78	136	29	46	0.04	6	57	a	1	0.17	${0.38}_{- 0.12}^{+ 0.17}$ $0.38_{ - 0.12}^{ + 0.17}$
Elias 2-27	0.49	140	56	117	0.04	6	69	a	1	0.06	${0.40}_{- 0.16}^{+ 0.23}$ $0.40_{ - 0.16}^{ + 0.23}$
GW Lup	0.46	155	39	38	0.04	6	74	a	1	0.03	$^{()} {0.14}_{- 0.06}^{+ 0.11}$ $^{()}0.14_{ - 0.06}^{ + 0.11}$
HD 142666	1.58	148	62	162	0.13	6	16	a	1	0.3	${0.59}_{- 0.21}^{+ 0.28}$ $0.59_{ - 0.21}^{ + 0.28}$
HD 143006	1.78	165	19	169	0.15, 0.06	6	22, 51	a	1	19.91, 0.33	${7.38}_{- 1.93}^{+ 2.56}, {1.16}_{- 0.44}^{+ 0.71}$ $7.38_{ - 1.93}^{ + 2.56},1.16_{ - 0.44}^{ + 0.71}$
HD 163296	2.04	101	48	133	0.21, 0.04, 0.02	6	10, 48, 86	a	1	0.71, 2.18, 1	${1.05}_{- 0.45}^{+ 0.68}, {1.92}_{- 0.59}^{+ 0.77},^{()} {0.19}_{- 0.10}^{+ 0.20}$ $1.05_{ - 0.45}^{ + 0.68},1.92_{ - 0.59}^{ + 0.77}{,^{()}}0.19_{ - 0.10}^{ + 0.20}$
SR 4	0.68	134	22	18	0.18	6	11	a	1	2.16	${1.47}_{- 0.37}^{+ 0.49}$ $1.47_{ - 0.37}^{ + 0.49}$
DoAr 25	0.95	138	67	111	0.02	6	111	a	1	0.73	${0.24}_{- 0.10}^{+ 0.16}$ $0.24_{ - 0.10}^{ + 0.16}$
Elias 2-20	0.48	138	49	153	0.08	6	25	a	1	0.57	${0.22}_{- 0.08}^{+ 0.11}$ $0.22_{ - 0.08}^{ + 0.11}$
RU Lup	0.63	154	19	121	0.06	6	29	a	1	1.18	${0.29}_{- 0.10}^{+ 0.16}$ $0.29_{ - 0.10}^{ + 0.16}$
IM Lup	0.89	158	48	143	0.03	6	117	a	1	0.039	$^{()} {0.21}_{- 0.09}^{+ 0.16}$ $^{()}0.21_{ - 0.09}^{ + 0.16}$
Sz 114	0.17	162	21	165	0.19	6	24	a	1	0.02	$^{()} {0.06}_{- 0.03}^{+ 0.04}$ $^{()}0.06_{ - 0.03}^{ + 0.04}$
Sz 129	0.83	161	34	151	0.07	6	41	a	1	0.03	${0.16}_{- 0.06}^{+ 0.09}$ $0.16_{ - 0.06}^{ + 0.09}$
HL Tau	1	140	47	138	0.14, 0.05, 0.03	7	13.1, 33, 68.6	b	2	0.35, 0.17, 0.26	${1.01}_{- 0.32}^{+ 0.42}, {0.82}_{- 0.31}^{+ 0.43}, {0.55}_{- 0.20}^{+ 0.31}$ $1.01_{ - 0.32}^{ + 0.42},0.82_{ - 0.31}^{ + 0.43},0.55_{ - 0.20}^{ + 0.31}$
HD 169142	1.65	117	5	13	0.08, 0.03, 0.02	6	17, 50, 64	d	4,5,6,7,8	2.4, 2.4, 0.03	$() {7.57}_{- 3.82}^{+ 5.59}, {0.68}_{- 0.25}^{+ 0.38},^{()} {0.96}_{- 0.51}^{+ 0.85}$ ${\rm{()}}7.57_{ - 3.82}^{ + 5.59},0.68_{ - 0.25}^{ + 0.38}{,^{()}}0.96_{ - 0.51}^{ + 0.85}$
HD 97048	2.5	183	40	3	0.07	7	130	c	7,8	2	${0.82}_{- 0.26}^{+ 0.38}$ $0.82_{ - 0.26}^{ + 0.38}$
Lk Ca 15	1.25	159	50	62	0.11, 0.06	6	36, 70	e	3, 9	0.47, 0.02	${3.45}_{- 0.86}^{+ 1.13}, {0.71}_{- 0.27}^{+ 0.33}$ $3.45_{ - 0.86}^{ + 1.13},0.71_{ - 0.27}^{ + 0.33}$
TW Hya	0.8	56	56	-8	0.03, 0.01	7	20, 81	f	3	0.15, 0.08	${0.80}_{- 0.26}^{+ 0.39},^{()} {2.77}_{- 1.80}^{+ 5.89}$ $0.80_{ - 0.26}^{ + 0.39}{,^{()}}2.77_{ - 1.80}^{ + 5.89}$
CI Tau	0.9	159	50	11	0.24, 0.08, 0.03	6	14, 43, 119	g	10	0.75, 0.15, 0.4	${3.10}_{- 0.79}^{+ 1.14}, {0.70}_{- 0.25}^{+ 0.32}, {0.56}_{- 0.21}^{+ 0.31}$ $3.10_{ - 0.79}^{ + 1.14},0.70_{ - 0.25}^{ + 0.32},0.56_{ - 0.21}^{ + 0.31}$
CR Cha	1.5	187	31	36	0.08	6	90	h	11	0.31	$^{()} {0.58}_{- 0.27}^{+ 0.46}$ $^{()}0.58_{ - 0.27}^{ + 0.46}$
DS Tau	0.83	159	65	-19	0.29	6	33	i	12	3.5	${1.28}_{- 0.43}^{+ 0.51}$ $1.28_{ - 0.43}^{ + 0.51}$
DM Tau	0.5	145	33	-25	0.03	3	70	l	13	0.333	${0.26}_{- 0.10}^{+ 0.15}$ $0.26_{ - 0.10}^{ + 0.15}$
DL Tau	0.98	159	45	52	0.24, 0.14, 0.11	6	39, 67, 89	i	14	0.11, 0.08, 0.33	${0.17}_{- 0.07}^{+ 0.10}, {1.23}_{- 0.49}^{+ 0.67}, {0.55}_{- 0.22}^{+ 0.32}$ $0.17_{ - 0.07}^{ + 0.10},1.23_{ - 0.49}^{ + 0.67},0.55_{ - 0.22}^{ + 0.32}$
DN Tau	0.52	128	35	79	0.19	6	49	i	14	0.009	$^{()} {0.20}_{- 0.09}^{+ 0.15}$ $^{()}0.20_{ - 0.09}^{ + 0.15}$
FT Tau	0.34	127	35	122	0.28	6	25	i	14	0.15	${0.19}_{- 0.07}^{+ 0.11}$ $0.19_{ - 0.07}^{ + 0.11}$
GM Aur	1.32	159	53	57	0.05	6	67	m	15	0.1	${0.29}_{- 0.09}^{+ 0.13}$ $0.29_{ - 0.09}^{ + 0.13}$
GO Tau	0.36	144	54	21	0.15, 0.10	6	59,87	i	14	0.057, 0.07	${0.22}_{- 0.08}^{+ 0.14},^{()} {0.12}_{- 0.06}^{+ 0.13}$ $0.22_{ - 0.08}^{ + 0.14}{,^{()}}0.12_{ - 0.06}^{ + 0.13}$
HD 107146⁽²⁾	1	27.5	19	153	0.12	6	80	n	16	0.1	${0.76}_{- 0.31}^{+ 0.50}$ $0.76_{ - 0.31}^{ + 0.50}$
IQ Tau	0.5	131	62	42	0.22	6	41	i	14	0.065	${0.11}_{- 0.05}^{+ 0.06}$ $0.11_{ - 0.05}^{ + 0.06}$
MWC 480	1.91	161	36.5	147.5	0.16	6	73	i	14	1.3	${1.06}_{- 0.36}^{+ 0.45}$ $1.06_{ - 0.36}^{ + 0.45}$
MWC 758	1.5	160	21	62	0.10	7	30	o	17	1.5	${7.85}_{- 2.19}^{+ 2.88}$ $7.85_{ - 2.19}^{ + 2.88}$
UZ Tau	0.39	131	56	90	0.10	6	69	i	14	0.023	${0.15}_{- 0.06}^{+ 0.10}$ $0.15_{ - 0.06}^{ + 0.10}$

Notes. ⁽*⁾Unreliable DBNets mass estimates.⁽¹⁾ This column is aimed at allowing a comparison with the resolution of the synthetic observations (0.12a). We report the major standard deviations of the two-dimensional Gaussians that approximate the observational beams. Values are expressed in units of the gap radial location a. ⁽²⁾Note that, unlike the others, this is a debris disc. Data references: (a) DSHARP Data Release (https://almascience.eso.org/almadata/lp/DSHARP/), (b) ALMA Science Verification Data (https://almascience.eso.org/alma-data/science-verification), (c) Pinte (2019), (d) Pérez et al. (2019), (e) Facchini et al. (2020), (f) Andrews et al. (2016), (g) Clarke et al. (2018), (h) Kim et al. (2020), (i) Long et al. (2018), (l) Hashimoto et al. (2021), (m) Huang et al. (2020a), (n) Marino (2021), (o) Baruteau et al. (2019). Properties references: (1) Zhang et al. (2018), (2) Lodato et al. (2019), (3) Dong & Fung (2017), (4) Toci et al. (2019), (5) Pérez et al. (2019), (6) Gratton et al. (2019), (7) Pinte et al. (2019), (8) NASA exoplanets catalogue (https://exoplanets.nasa.gov/), (9) Facchini et al. (2020), (10) Clarke et al. (2018), (11) Kim et al. (2020), (12) Veronesi et al. (2020), (13) Wang et al. (2021), (14) Long et al. (2018), (15) Huang et al. (2020b), (16) Marino (2021), (17) Dong et al. (2018).

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