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Table 1

Parameters of our ATCA observations.

Source RA(J2000) Dec(J2000) Gain calibrator Beam size (arcsec) Beam p.a. (degree) Ton (hour) References
Sample 1

IRAS 15103–5754 15:14:18.397 −58:05:20.47 PMN J1515–5559 7.2 × 4.9 +85 0.65 1, 2
IRAS 16333–4807 16:37:06.601 −48:13:42.88 IERS B1646–506 8.0 × 4.6 +78 0.65 3, 4
IRAS 16372–4808 16:40:55.818 −48:13:59.93 IERS B1646–506 7.1 × 4.6 +82 0.65 5, 6
OH 341.6811+00.2634 16:51:53.640 −43:47:16.50 IERS B1646–506 9.5 × 4.1 +81 0.65 5
NGC 6302 17:13:44.489 −37:06:11.71 IERS B1729–373 6.9 × 4.3 +75 0.65 7, 8
IRAS 17347–3139 17:38:00.624 −31:40:54.91 IERS B1741–312 6.8 × 4.2 +75 0.66 9, 10
JaSt 23 17:40:23.067 −27:49:12.00 IERS B1741–312 6.5 × 4.1 +88 0.67 11, 12
IRAS 17393–2727 17:42:33.140 −27:28:24.70 IERS B1741–312 7.2 × 3.9 −88 0.65 13, 14
IRAS 18061–2505 180912.400 −25:04:34.50 IERS B1817–254 6.2 × 4.1 +72 0.65 15, 16
Vy 2–2 19:24:22.218 +09:53:56.33 IVS B1936+046 6.8 × 5.7 +78 1.24 17, 18
K 3–35 19:27:44.026 +21:30:03.57 IVS B1936+046 8.1 × 5.1 +31 0.66 19, 20

Sample 2

IRAS 17239–2812 17:27:05.030 −28:15:27.50 PKS 1710–269 0.76 × 0.18 +7 0.74 21, 22
IRAS 17390–3014 17:42:18.870 −30:15:29.00 PKS 1710–269 0.73 × 0.17 +6 0.74 23, 24
H 2–18 17:43:28.840 −21:09:52.50 PKS 1710–269 0.95 × 0.18 +3 0.74 25, 26
IRAS 18052–2016 18:08:16.380 −20:16:11.30 IERS B1829–207 1.37 × 0.17 +4 0.74 27, 28
IRAS 19508+2659 19:52:57.900 +27:07:44.70 VCS2 J1956+2820 1.12 × 0.16 +2 0.57 29, 30

Notes. Right ascension and declination represent the coordinates of the phase center of the observations. “Gain calibrator” is the complex-gain calibrator used for each target. Beam sizes (full width at half maximum) and beam position angles (p.a., measured north to east) are those of the continuum images at 43 GHz. Ton is the total integration time on each source. The coordinates of H 2–18 are those given in Gathier et al. (1983), since the position given in the SIMBAD database, at the time of our observations, actually corresponded to a different object, IRAS 17403–2107 (see Sect. 4.2.3). Sample 1 comprises PNe with known OH and/or H2O masers (Sect. 2.1). The references listed for this sample correspond to their identification as PNe and the report on the presence maser emission. Sample 2 includes single-dish SiO maser detections near PNe and radio continuum sources (Sect. 2.2). Their references correspond to their identification as PNe or the presence of radio continuum emission, and the single-dish reporting of maser emission. (1) Gómez et al. (2015), (2) Suárez et al. (2015), (3) Kimeswenger (2001), (4) Uscanga et al. (2014), (5) Cala et al. (2022), (6) Sevenster et al. (1997b), (7) Payne et al. (1988), (8) Henize (1967), (9) de Gregorio-Monsalvo et al. (2004), (10) Gómez et al. (2005), (11) Jacoby & Van de Steene (2004), (12) Sevenster et al. (1997a), (13) Pottasch et al. (1987), (14) García-Hernández et al. (2007), (15) Suárez et al. (2006), (16) Gómez et al. (2008), (17) Vyssotsky et al. (1945), (18) Seaquist & Davis (1983), (19) Miranda et al. (1998), (20) Miranda et al. (2001), (21) Hall et al. (1990), (22) Douglas et al. (1996), (23) Deguchi et al. (2004), (24) Condon et al. (1998), (25) Gathier et al. (1983), (26) Izumiura et al. (1995), (27) Deacon et al. (2007), (28) Garwood et al. (1988), (29) White et al. (2005), (30) Nakashima & Deguchi (2003a).

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