The ESO SupJup Survey - I. Chemical and isotopic characterisation of the late L-dwarf DENIS J0255-4700 with CRIRES+

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Volume 688 (August 2024)

A&A, 688 (2024) A116

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Tab1e A.1

Targets observed as part of the ES0 SupJup Survey (Program ID: 1110.C-4264, PI: Sne11en), sorted by right ascension.

System Name	0n-S1it Targets	d (pc)	BANYAN Σ⁽¹⁾	Age (Myr)	SpType	m_J (mag)	m_K (mag)	M (M_Jup)	a (″/AU)	0bs. Date	Setting	A0	S1it	Exp. Time
HD 1160	HD 1160B,	120.9±0.5⁽²⁾	FIELD (99.9%)	10-20<³>	M5.5⁽⁴⁾,	15.83±0.10,	14.12±0.05,	20⁽³⁾,	0.78/80,	2022 11 01	K2166	Yes	0.4	45×300s = 3h45m
	HD 1160C				M3.5⁽⁵⁾	13.31±0.04⁽⁵⁾	12.18±0.06⁽⁵⁾	231±42⁽³⁾	5.15/530⁽⁵⁾

LSPM J0036+1821	LSPM J0036	8.74±0.01⁽²⁾	FIELD (99.9%)	-	L3.5⁽⁶⁾	12.47±0.03⁽⁷⁾	11.06±0.02⁽⁷⁾	-	-	2022 11 03	K2166	No	0.2	10×300s = 0h50m
										2022 11 04	J1226	No	0.2	14×300s = 1h10m
														2h00m

2MASS J01033563-5515561	2M 0103AB,	12.86±1.97⁽⁸⁾	THA (99.3%)	45±4	M5.5,	10.16±0.02⁽⁷⁾,	9.24±0.02⁽⁷⁾,	199/178±21,	1.72/84⁽¹⁰⁾	2022 11 04	K2166	No	0.4	34×300s = 2h50m
	2M 0103(AB)b				L⁽¹⁰⁾	15.4±0.3⁽¹⁰⁾	13.6±0.2⁽¹⁰⁾	13+1⁽¹⁰⁾

2MASS J01225093-2439505	2M 0122A,	33.74±0.03⁽²⁾	ABDMG (98.4%)	$149_{- 19}^{+ 51}$ $149_{ - 19}^{ + 51}$ (9)	M3.5⁽¹¹⁾,	10.02±0.03,	9.17±0.03,	419±52,	1.45/52±6⁽¹²⁾	2022 11 02	K2166	Yes	0.4	49×300s = 4h05m
	2M 0122B				L4-6⁽¹²⁾	16.81±0.14⁽¹²⁾	14.53±0.05⁽¹²⁾	23-27⁽¹²⁾
										2022 11 03	K2166	Yes	0.4	42×300s = 3h30m
														7h35m

2MASS J01415823-4633574	2M 0141	36.65±0.59⁽²⁾	THA (99.9%)	45±4⁹	L0⁽¹³⁾	14.83±0.04⁽⁷⁾	13.10±0.03⁽⁷⁾	-	-	2023 01 03	K2166	No	0.4	12×300s = 1h00m

2MASS J02192210-3925225	2M 0219A,	40.2±0.1⁽²⁾	THA (99.9%)	45±4⁹	M6,	11.32±0.03,	10.44±0.03,	113±12,	3.96/156±10⁽¹⁴⁾	2022 11 01	K2166	No	0.4	26×300s = 2h10m
	2M 0219B				L4⁽¹⁴⁾	15.54±0.10⁽¹⁴⁾	13.82±0.10⁽¹⁴⁾	13.9±1.1⁽¹⁴⁾
										2022 11 03	K2166	No	0.4	16×300s = 1h20m
										2022 11 04	K2166	No	0.4	32×300s = 2h40m
														6h10m

DENIS J025503.3-470049	DENIS J0255	4.868±0.004⁽²⁾	FIELD (99.9%)	-	L9⁽¹⁵⁾	13.24±0.03⁽⁷⁾	11.56±0.02⁽⁷⁾	-	-	2022 11 02	K2166	No	0.2	12×300s = 1h00m

2MASS J03552337+1133437	2M 0355	9.16±0.04⁽²⁾	ABDMG (99.9%)	149+51(9)	L5⁽¹³⁾	14.05±0.02⁽⁷⁾	11.53±0.02⁽⁷⁾	-	-	2022 11 02	K2166	No	0.2	10×300s = 0h50m

FU Tau	FU Tau A,	127.6±1.2⁽²⁾	TAU (96.6%)	ļ.2(16)	M7.25,	10.78±0.03,	9.32±0.02,	52.4,	5.7/800⁽¹⁷⁾	2023 01 01	K2166	No	0.4	24×300s = 2h00m
	FU Tau B				M9.25⁽¹⁷⁾	15.04±0.12⁽⁷⁾	13.33±0.10⁽⁷⁾	15.7⁽¹⁷⁾

DH Tau	DH Tau A,	133.4±0.5⁽²⁾	TAU (99.8%)	1_2(i6)	M0.5,	9.77±0.02,	8.18±0.03,	670±42⁽¹⁹⁾,	2.34/328.2±0.4⁽²¹⁾	2022 12 31	K2166	No	0.4	16×300s = 1h20m
	DH Tau B				L2 ⁽¹⁸⁾	15.71±0.05⁽¹⁸⁾	14.19±0.02⁽¹⁵⁾	8-22⁽²⁰⁾
										2023 01 01	K2166	No	0.4	14×300s = 1h10m
														2h30m

2MASS J04341527+2250309	2M 0434	163±10⁽²⁾	TAU (87.8%)	1-2⁽¹⁶⁾	M7⁽²²⁾	13.74±0.03⁽⁷⁾	11.85±0.02⁽⁷⁾	-	-	2022 12 31	K2166	No	0.4	1×300s = 0h05m
										2023 02 01	K2166	No	0.4	22×300s = 1h50m
										2023 02 01	J1226	No	0.4	10×300s = 50m
														2h45m

2MASS J05002100+0330501	2M 0500	13.23±0.05⁽²⁾	FIELD (99.9%)	-	L4⁽²³⁾	13.67±0.02⁽⁷⁾	12.06±0.02⁽⁷⁾	-	-	2023 02 27	K2166	No	0.4	18x300 = 1h30m

2MASS J05012406-0010452	2M 0501	20.9±0.3⁽²⁾	FIELD (99.9%)	-	L4⁽¹³⁾	14.98±0.04⁽⁷⁾	12.96±0.04⁽⁷⁾	-	-	2022 12 31	K2166	No	0.4	3×300s = 0h15m
										2023 02 01	K2166	No	0.4	12×300s = 1h00m
														1h15m

2MASS J05233822-1403022	2M 0523	12.73±0.02⁽²⁾	FIELD (99.9%)	-	L2.5⁽²⁴⁾	13.08±0.02⁽⁷⁾	11.638±0.03⁽⁷⁾	-	-	2023 01 03	K2166	No	0.4	12×300s = 1h00m

β Pic	β Pic b	19.44±0.05⁽²⁾	β PMG (99.9%)	24±3<">	L2⁽²⁵⁾	14.00±0.08⁽²⁵⁾	12.30±0.15⁽²⁵⁾	${11.90}_{- 3.04}^{+ 2.93}$ $11.90_{ - 3.04}^{ + 2.93}$	~0.5/10.6±0.5⁽²⁷⁾	2023 01 02	K2166	Yes	0.2	210×120s = 7h00m

2MASS J05591914-1404488	2M 0559	10.50±0.08⁽²⁾	FIELD (99.9%)	-	T4.5⁽²⁸⁾	13.80±0.02⁽⁷⁾	13.58±0.05⁽⁷⁾	-	-	2023 02 01	K2166	No	0.4	16×300s = 1h20m
										2023 02 01	J1226	No	0.4	4×300s = 0h20m
														1h40m

DENIS J060852.8-275358	2M 0608	44.2±0.3⁽²⁾	FIELD (99.9%)	-	M9.6⁽²⁹⁾	13.60±0.03⁽⁷⁾	12.37±0.03⁽⁷⁾	-	-	2023 02 26	K2166	No	0.4	24×300s = 2h00m

CD-35 2722	CD-35 2722A,	22.36±0.01⁽²⁾	ABDMG (99.9%)	$149_{- 19}^{+ 51}$ $149_{ - 19}^{ + 51}$ ⁽⁹⁾	M1⁽³⁰⁾,	7.86±0.03,	7.03±0.05,	419±52,	3.14/67±4⁽³¹⁾	2022 12 31	K2166	No	0.4	8×300s = 0h40m
	CD-35 2722B				L4⁽³¹⁾	13.63±0.11⁽³¹⁾	12.01±0.07⁽³¹⁾	31±8⁽³¹⁾
										2023 01 03	K2166	No	0.4	24×300s = 2h00m
										2023 01 31	J1226	No	0.4	7×300s = 0h35m
														3h15m

AB Pic	AB Pic b	50.14±0.03⁽²⁾	CAR (99.7%)	${13.3}_{- 0.6}^{+ 1.1}$ $13.3_{ - 0.6}^{ + 1.1}$ ⁽³²⁾	L0-1⁽³³⁾	16.18±0.10⁽³⁴⁾	14.14±0.08⁽³⁴⁾	10±1⁽³⁵⁾	5.4/273±2⁽³⁴⁾	2022 11 01	K2166	Yes	0.4	22×300s = 1h50m
										2022 11 02	K2166	Yes	0.4	12×300s = 1h00m
										2022 11 03	K2166	Yes	0.4	16×300s = 1h20m
										2022 11 04	K2166	Yes	0.4	14×300s = 1h10m
														5h20m

2MASS J06244595-4521548	2M 0624	12.19±0.05⁽²⁾	ARG (93.5%)	40-50⁽³⁶⁾	L6.5⁽¹⁵⁾	14.48±0.03⁽⁷⁾	12.60±0.03⁽⁷⁾	-	-	2023 02 27	K2166	No	0.4	15×300 = 1h15m

SSSPM J0829-1309	2M 0829	11.68±0.02⁽²⁾	FIELD (99.9%)	-	L2⁽³⁷⁾	12.80±0.03⁽⁷⁾	11.30±0.02⁽⁷⁾	-	-	2023 01 03	K2166	No	0.4	12×300s = 1h00m

2MASS J08354256-0819237	2M 0835	7.23±0.01⁽²⁾	FIELD (95.1%)	-	L6.5⁽¹⁵⁾	13.17±0.02⁽⁷⁾	11.136±0.02⁽⁷⁾	-	-	2023 01 01	K2166	No	0.4	4×300s = 0h20m

HR 3549	HR 3549B	94.8±0.3⁽²⁾	FIELD (92.1%)	100-150⁽³⁸⁾	L0⁽³⁸⁾	15.94±0.06⁽³⁸⁾	-	40-50⁽³⁸⁾	0.9/80⁽³⁹⁾	2023 01 01	K2166	Yes	0.2	26×300s = 2h10m

2MASS J08561384-1342242	2M 0856	53.8±0.4⁽²⁾	FIELD (96.2%)	-	M8⁽²³⁾	13.60±0.03⁽⁷⁾	12.49±0.02⁽⁷⁾	-	-	2023 03 04	K2166	No	0.4	18×300s = 1h30m

2MASSI J0953212-101420	2M 0953	35.7±0.3⁽²⁾	FIELD (63.5%)	-	L0.0⁽²⁹⁾	13.47±0.03⁽⁷⁾	12.14±0.02⁽⁷⁾	-	-	2023 03 04	K2166	No	0.4	18×300s = 1h30m

Luhman 16	Luhman 16A,	2.02±0.15⁽²⁾	ARG (94.1 %)	40-50⁽³⁶⁾	L7.5,	11.53±0.04,	9.44±0.07,	33.5±0.3,	1.5/3.12±0.25⁽⁴⁰⁾	2022 12 31	K2166	No	0.2	4×300s = 0h20m
	Luhman 16B				T0.5⁽⁴¹⁾	11.22±0.04⁽⁴¹⁾	9.73±0.09⁽⁴¹⁾	28.6±0.3⁽⁴²⁾
										2023 01 01	K2166	No	0.4	4×300s = 0h20m
										2023 01 01	J1226	No	0.4	4×300s = 0h20m
														1h00m

TWA 28	TWA 28	59.2±0.4⁽²⁾	TWA (99.6%)	10±3⁽⁹⁾	M8.3⁽⁴³⁾	13.03±0.02⁽⁷⁾	11.89±0.02⁽⁷⁾	-	-	2023 03 03	K2166	No	0.4	14×300s = 1h10m

CD-33 7795	TWA 5A,	49.6±0.1⁽²⁾	TWA (99.9%)	10±3⁽⁹⁾	M1.5,	8.40±0.07,	7.39±0.04,	~419⁽⁴⁵⁾,	1.9/86±4⁽⁴⁶⁾	2023 02 26	K2166	Yes	0.2	16×300s = 1h20m
	TWA 5B				M8.5⁽⁴⁴⁾	12.6±0.2⁽¹⁸⁾	11.4±0.2⁽¹⁸⁾	$25_{- 20}^{+ 120}$ $25_{ - 20}^{ + 120}$ ⁽⁴⁶⁾

2MASS J11553952-3727350	2M 1155	11.80±0.02⁽²⁾	FIELD (99.9%)	-	L2⁽⁴⁷⁾	12.81 ±0.02⁽⁷⁾	11.46±0.02⁽⁷⁾	-	-	2023 02 01	K2166	No	0.4	4×300s = 0h20m
										2023 02 01	J1226	No	0.4	2×300s = 0h10m
														0h30m

2MASS J12003792-7845082	2M 1200	101.6±0.7⁽²⁾	EPSC (99.8%)	${3.7}_{- 1.4}^{+ 4.6}$ $3.7_{ - 1.4}^{ + 4.6}$ ⁽⁴⁸⁾	M6⁽⁴⁹⁾	12.52±0.02⁽⁷⁾	11.60±0.02⁽⁷⁾	-	-	2023 03 04	K2166	No	0.4	8×300s = 0h40m

HIP 64892	HIP 64892B	Π9.6±0.7⁽²⁾	LCC (74.0%)	15±3⁽⁵⁰⁾	M9⁽⁵¹⁾	14.85±0.15⁽⁵¹⁾	13.50±0.17⁽⁵¹⁾	33±4⁽⁵¹⁾	1.27/159±12⁽⁵¹⁾	2023 02 26	K2166	Yes	0.2	12×300s = 1h00m
										2023 03 03	K2166	Yes	0.2	5×300s = 0h25m
										2023 03 04	K2166	Yes	0.2	18×300s = 1h30m
														2h55m

YSES 1	YSES 1b,	94.2±0.1⁽²⁾	LCC (99.1%)	15±3⁽⁵⁰⁾	L0⁽⁵²⁾,	15.73±0.38⁽⁵²⁾,	14.70±0.14⁽⁵²⁾,	14±3⁽⁵²⁾,	1.71/162⁽⁵²⁾,	2023 02 26	K2166	Yes	0.2	22×600s = 3h40m
	YSES 1c				L7.5⁽⁵³⁾	21.50±0.13⁽⁵³⁾	18.13±0.13⁽⁵³⁾	6±1⁽⁵³⁾	3.37/320⁽⁵³⁾
										2023 02 27	K2166	Yes	0.2	10×600s = 1h40m
														5h20m

2MASS J14252798-3650229	2M 1425	11.85±0.04⁽²⁾	ABDMG (99.9%)	$149_{- 19}^{+ 51}$ $149_{ - 19}^{ + 51}$ ⁽⁹⁾	L4⁽²³⁾	13.75±0.03⁽⁷⁾	11.81±0.03⁽⁷⁾			2023 02 01	K2166	No	0.4	12×300s = 1h00m
										2023 02 01	J1226	No	0.4	4×300s = 0h20m
														1h20m

GQ Lup	GQ Lup A,	154.1 ±0.7⁽²⁾	UCL (99.4%)	16±2⁽⁵⁰⁾	K7⁽⁵⁴⁾,	8.69±0.04,	7.10±0.02,	1079±52⁽⁵⁶⁾,	0.7/105⁽¹⁸⁾	2023 02 27	K2166	Yes	0.2	61×180s = 3h03m
	GQ Lup b				L1⁽⁵⁵⁾	14.90±0.11⁽¹⁸⁾	13.34±0.13⁽¹⁸⁾	~30⁽⁵⁷⁾

R0Xs 12	R0Xs 12A,	138.6±0.3⁽²⁾	USC0 (97.6%)	10±3⁽⁵⁰⁾	M0,	10.28±0.02,	9.10±0.03,	911 ±84,	1.75/210±20⁽⁵⁹⁾	2023 03 03	K2166	No	0.4	2×450s = 0h15m
	R0Xs 12b				L0⁽⁵⁸⁾	15.82±0.03⁽⁵⁸⁾	14.14±0.03⁽⁵⁸⁾	16±4⁽⁵⁹⁾
										2023 03 04	K2166	No	0.4	22×600s = 3h40m
														3h55m

PZ Tel	PZ Tel B	47.25±0.05⁽²⁾	βPMG (97.2%)	24±3⁽⁹⁾	M7⁽⁶⁰⁾	12.26±0.14⁽⁶¹⁾	11.42±0.15⁽⁶¹⁾	$27_{- 9}^{+ 25}$ $27_{ - 9}^{ + 25}$ (62)	0.48/~25⁽⁶⁰⁾	2022 11 02	K2166	Yes	0.2	8×300s = 0h40m
	PZ Tel A,				G9⁽⁶³⁾,	6.86±0.02⁽⁷⁾,	6.38±0.02⁽⁷⁾,	H84±3l⁽⁶⁴⁾,	0.48/~25⁽⁶⁰⁾	2022 11 03	K2166	Yes	0.2	22×150s = 0h55m
	PZ Tel B				M7⁽⁶⁰⁾	12.26±0.14⁽⁶¹⁾	11.42±0.15⁽⁶¹⁾	$27_{- 9}^{+ 25}$ $27_{ - 9}^{ + 25}$ (62)
														1h35m

36 systems	49 on-slit,
	19 companions

Notes. As a consequence of the degeneracy between the ages and masses of isolated, field sub-stellar objects, these parameters are not listed. The BANYAN Σ association (Gagné et al. 2018) with the highest membership probability (in parentheses) is shown. The full names of these identifiers are field (FIELD), Tucana-Horologium association (THA), AB Doradus (ABDMG), Taurus (TAU), β Pictoris (βPMG), Carina (CAR), Argus (ARG), TW Hya (TWA), є Chamaeleontis (EPSC), Lower Centaurus Crux (LCC), Upper Centaurus Lupus (UCL), and Upper Scorpius (USCO).

References. (1) Gagné et al. (2018); (2) Gaia Collaboration (2020); (3) Mesa et al. (2020); (4) Garcia et al. (2017); (5) Nielsen et al. (2012); (6) Reid et al. (2000); (7) Cutri et al. (2003); (8) Riedel et al. (2014); (9) Bell et al. (2015); (10) Delorme et al. (2013); (11) Riaz et al. (2006); (12) Bowler et al. (2013); (13) Cruz et al. (2009); (14) Artigau et al. (2015); (15) Burgasser et al. (2006); (16) Kenyon & Hartmann (1995); (17) Luhman et al. (2009); (18) Patience et al. (2012); (19) Xuan et al. (2020); (20) Luhman et al. (2006); (21) Itoh et al. (2005); (22) Monin et al. (2010); (23) Gagné et al. (2015); (24) Cruz et al. (2003); (25) Chilcote et al. (2017); (26) Lacour et al. (2021); (27) GRAVITY Collaboration et al. (2020); (28) Geballe et al. (2002); (29) Bardalez Gagliuffi et al. (2014); (30) Torres et al. (2006); (31) Wahhaj et al. (2011); (32) Booth et al. (2021); (33) Bonnefoy et al. (2010); (34) Chauvin et al. (2005); (35) Palma-Bifani et al. (2023); (36) Zuckerman (2019); (37) Scholz & Meusinger (2002); (38) Mesa et al. (2016); (39) Mawet et al. (2015); (40) Luhman (2013); (41) Burgasser et al. (2013); (42) Lazorenko & Sahlmann (2018); (43) Faherty et al. (2016); (44) Lowrance et al. (1999); (45) Faherty et al. (2010); (46) Neuhäuser et al. (2010); (47) Gizis (2002); (48) Murphy et al. (2013); (49) Schutte et al. (2020); (50) Pecaut & Mamajek (2016); (51) Cheetham et al. (2018); (52) Bohn et al. (2020a); (53) Bohn et al. (2020b); (54) Herbig (1977); (55) Lavigne et al. (2009); (56) MacGregor et al. (2017); (57) Stalker et al. (2021); (58) Bowler et al. (2017); (59) Kraus et al. (2014); (60) Maire et al. (2016); (61) Biller et al. (2010); (62) Franson & Bowler (2023); (63) Stalker et al. (2020); (64) Jenkins et al. (2012)

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