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Table 1.

Main data of our observational sample.

PN G Usual name RA(J2000) Dec(J2000) Status (a) Morph (a) MajDiam (a) Exposure Seeing (b)
(h m s) (° ′ ″) (arcsec) (sec) (arcsec)
015.5+02.8 BMP J1808−1406 18 08 35.09 −14 06 42.9 T Rar 470 3×830 (c) 0.90(g)
023.8−06.2 BMP J1857−1054 18 57 09.82 −10 54 51.1 L Bap 195 5×830 (c) 1.04(g)
231.1+03.9 BMP J0739−1418 07 39 50.55 −14 18 25.8 L Ras 153 3×738 (d) 0.82(r)
234.3−07.2 MPA J0704−2221 07 04 22.98 −22 21 51.9 L Ra 190 4×870 (d) 0.55(r)
234.9−09.7 MPA J0656−2356 06 55 59.95 −23 56 49.4 L R 170 2×900 (e) 0.85(r)
237.3−08.4 BMP J0705−2528 07 05 45.54 −25 28 49.5 L Bs 124 2×900 (e) 0.58(r)
247.5−04.7 FEGU 248-5 07 42 24.03 −32 47 47.4 T Es 181 3×910 (f) 0.69(r)
328.5+06.2 PHR J1533−4824 15 33 06.87 −48 24 44.6 T A 200 3×1350 (g) 1.07(g)
344.9+03.0 BMP J1651−3930 16 51 41.31 −39 30 27.5 T Eas/Isa 315 3×999 (f) 0.87(r)
355.3+03.8 MPA J1719−3043 17 19 20.07 −30 43 40.3 L R 65 3×1100 (g) 0.74(g)

Notes. The star coordinates are from Gaia DR3.

(a)

PN status (T = true, L = likely), morphological classification, and major diameter are from the HASH catalogues.

(b)

The seeing is measured on the acquisition image. The Sloan photometric band of the image is given in brackets.

(c)

Programme GS-2021A-Q-226.

(d)

Programme GS-2021B-Q-227.

(e)

Programme GS-2020B-Q-228.

(f)

Programme GS-2020A-Q-203.

(g)

Programme GS-2022A-Q-318.

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