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Table B.1

H2O maser non-detections in our survey.

Source Type (FUor/EXor/ Gaia alert) R.A. (J2000) (h m s) Dec. (J2000) (° ′ ″) Upper limit(a) (Jy) Previous survey(b) (No/Yes/ Unknown) Date(c) (A/B/C) Classification (Class 0 –II) Ref. D(d) (pc)
V1180 Cas EXor 02 33 01.53 +72 43 26.8 0.17 Unk. – – 908 [51]
PP 13S FUor 04 10 41.09 +38 07 54.5 0.18 Yes [1] I 21 350
L1551 IRS 5 FUor 04 31 34.07 +18 08 04.9 0.17 No [2,3] I 22 –
XZ Tau EXor 04 31 40.08 +18 13 56.6 0.18 Unk. II 23 140
UZ Tau E EXor 04 32 43.02 +25 52 30.9 0.18 Unk. II 24 130[51]
LDN 1415 IRS EXor 04 41 37.50 +54 19 22.0 0.21 Unk. I 25 170
DR Tau EXor 04 47 06.21 +16 58 42.8 0.17 Unk. II 26 192 [51]
V582 Aur FUor 05 25 51.97 +34 52 30.0 0.15 Unk. II 27 2401 [52,53]
V1118 Ori EXor 05 3444.98 −05 33 41.3 0.21 Unk. II 28 414
Haro 5a IRS FUor 05 35 26.74 −05 03 55.0 0.21 Unk. 0/I 29 450
NY Ori EXor 05 35 36.00 −05 12 25.2 0.22 Unk. – – 403 [51]
V1143 Ori EXor 05 38 03.89 −04 16 42.8 0.22 Unk. II 30 395 [51]
V883 Ori FUor 05 38 18.09 −07 02 25.9 0.20 No [4,5] I 31 417 [54]
HBC 494 FUor 05 40 27.45 −07 27 30.0 0.21 Unk. I 32 –
V2775 Ori FUor 05 42 48.48 −08 16 34.7 0.25 No [6] late I 33 420
FU Ori FUor 05 45 22.37 +09 04 12.3 0.22 Unk. II 34 407 [51]
V1647 Ori FUor 05 46 13.13 −00 06 04.8 0.23 Unk. A I/II 35 412 [51]
AR 6A/6B FUor 06 40 59.30 +09 35 49.0 0.23 Unk. II 36 800
Parsamian 21 FUor 19 29 00.84 +09 38 43.4 0.16 Unk. I/II 37 400
I 18270-0153W FUor 18 29 36.90 −01 51 02.0 0.19 No [7] I 38 –
OO Ser FUor 18 29 49.13 +01 16 20.6 0.18 No [3,8] I 38 311
V371 Ser EXor 18 29 51.21 +01 16 39.4 0.18 No [3,8] – – 311
Gaia21aul Gaia alert 18 30 06.18 00 42 33.30 0.17 No [9,10] – – 378 [55]
I 18341-0113S FUor 18 36 45.70 −01 10 29.0 0.19 No [3,7] I 38 –
Gaia21aru Gaia alert 19 00 56.41 18 48 29.20 0.16 Unk. – – –
V1515 Cyg FUor 20 23 48.01 +42 12 25.7 0.18 Unk. – – 900 [55]
PV Cep EXor 20 45 53.90 +67 57 38.6 0.17 Yes [5,11] No [10,12,13,14,15] – – 325
V2492 Cyg EXor 20 51 26.23 +44 05 23.8 0.16 No [16] I 39 804 [51]
V1057 Cyg FUor 20 58 53.73 +44 15 28.4 0.17 Yes [11] No [3,10,12,13,14] II 40 891 [55]
HBC 722 FUor 20 58 17.00 +43 53 43.0 0.17 Unk. II 41 757 [55]
V2495 Cyg FUor 21 00 25.24 +52 30 16.9 0.16 No [9] I/II 42 800
RNO 127 FUor 21 00 31.80 +52 29 17.0 0.17 Unk. – – 800
CB 230 FUor 21 17 38.62 +68 17 34.0 0.15 No [3,7,17,18] 0/I 43 339 [18]
V1735 Cyg FUor 21 47 20.66 +47 32 03.8 0.18 No [1,3,12] II 43 663 [55]
V733 Cep FUor 22 53 33.25 +62 32 23.6 0.16 Unk. I/II 43 724 [55]
VY Tau EXor 04 39 17.42 +22 47 53.3 0.11 Unk. II 44 153 [55]
Gaia21arx Gaia alert 05 36 24.80 −06 17 30.52 0.15 Unk. – – 361 [55]
NGC 2071 FUor 05 47 09.80 +00 18 00.0 0.15 Yes [1,3,6] – – –
I 06297+1021W FUor 06 32 28.70 +10 19 0 0.16 Unk. B I 43 –
I 06393+0913 FUor 06 42 08.13 +09 10 30.0 0.15 Unk. I 43 –
Gaia18dvy FUor 20 05 06.02 +36 29 13.52 0.14 Unk. II 45 1880 [45]
Gaia19bpg Gaia alert 21 41 50.43 +51 55 45.48 0.12 Unk. – – –
V899 Mon FUor 06 09 19.24 −06 41 55.8 0.10 Unk. II 46 809 [51]
V900 Mon FUor 06 57 22.22 −08 23 17.6 0.13 Unk. I 47 1304 [51]
V960 Mon FUor 06 59 31.58 −04 05 27.7 0.12 Unk. C II 48 2189 [51]
iPTF 15AFQ FUor 07 09 21.39 −10 29 34.5 0.13 Unk. I 49 1315 [51]
Gaia20bdk Gaia alert 07 10 14.92 −18 27 01.04 0.15 Unk. – – –
0.05 A
RNO 1B/1C FUor 00 36 46.30 +63 28 54.0 0.04 No [1,7,8,10,19,20] B 1B: 0/I-II, 1C:II 50 965 [55]
0.04 C
0.05 D

Notes. Source types and coordinates are taken from Audard et al. (2014), except for Gaia alerts, whose positions are taken from the Gaia alerts system. (a)Upper limits are 3 × RMS. (b)Previous surveys: No – Source was observed, but no H2O maser detected; Yes – H2O maser detected; Unk. (Unknown) – To our knowledge, previously not searched for water masers. (c)Our observations were carried out on: A – 2021-11-18; B – 2021-11-23; C – 2022-01-25.; D – 2022-02-05. (d)Distance – the default values are from Audard et al. (2014), but in case of more recent data (i.e. Gaia), the values are then updated with references.

References. 1 – Wouterloot et al. (1993); 2 – Claussen et al. (1996); 3 – Sunada et al. (2007); 4 – Deguchi et al. (1989); 5 – Takaba et al. (2001); 6 – Kang et al. (2013); 7 – Codella et al. (1995); 8 – Furuya et al. (2003); 9 – Yung et al. (2013); 10 – Bae et al. (2011); 11 – Cesaroni et al. (1988); 12 – Felli et al. (1992); 13 – Palagi et al. (1993), 14 – Palla & Prusti (1993); 15 – Valdettaro et al. (2001); 16 – Urquhart et al. (2011); 17 – Gómez et al. (2006); 18 – Brand et al. (2019); 19 – Henning et al. (1992); 20 – Fiebig (1995); 21 – Sandell & Weintraub (2001); 22 – Fuller et al. (1995); 23 – Zapata et al. (2015); 24 – Mathieu et al. (1996); 25 – Stecklum et al. (2007); 26 – Banzatti et al. (2014); 27 - Ábrahám et al. (2018); 28 – Giannini et al. (2016); 29 – Kóspál et al. (2017); 30 – Parsamian & Mujica (2004); 31 – White et al. (2019); 32 – Ruíz-Rodríguez et al. (2017); 33 – Zurlo et al. (2017); 34 – Herbig (1977); 35 – Principe et al. (2018); 36 – Moriarty-Schieven et al. (2008); 37 – Kóspál et al. (2008); 38 – Connelley & Greene (2010); 39 – Hillenbrand et al. (2013); 40 – Fehér et al. (2017); 41 – Kóspál et al. (2016); 42 – Liu et al. (2018); 43 – Connelley & Reipurth (2018); 44 – Herbig (1990); 45 – Szegedi-Elek et al. (2020); 46 – Park et al. (2021); 47 – Takami et al. (2019); 48 – Kóspál et al. (2015); 49 – Miller et al. (2015); 50 – Quanz et al. (2007); 51 – Gaia Collaboration (2022); 52 – Bailer-Jones et al. (2018); 53 –Zsidi et al. (2019); 54 – Menten et al. (2007); 55 – Bailer-Jones et al. (2021)

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