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Table A.2.

Details of the spectra of CSPNs observed with GMOS.

PN G Name Programme ID Grating Spectral range [Å] PA [°] Exptime [s] Bin [px]
000.2−01.9 M 2–19 GS-2008B-Q-65 B1200 4090–5540 90 3 × 1336 2 × 2
001.7−04.6 H 1–56 GS-2016A-Q-74 B1200 3950–5500 76 3 × 500† 1 × 1
001.8−02.0 PHR J1757–2824 GS-2009A-Q-35 B1200 4100–5530 120 2 × 1950† 1 × 2
001.8−03.7 PHR J1804–2913 GS-2009A-Q-35 B1200 4100–5530 90 1 × 1200† 1 × 2
003.3−04.6 Ap 1–12 GS-2016A-Q-101 B600 3500–6260 71 3 × 800 1 × 1
003.5−02.4 IC 4673 GS-2011A-Q-65 B1200 3830–5200 125 1 × 1800 1 × 2
005.0+03.0 Pe 1–9 GS-2009A-Q-35 B1200 4100–5530 45 1 × 2700† 1 × 2
007.8−04.4 H 1–65 GS-2011A-Q-65 B1200 4000–5200 270 1 × 900 1 × 2
011.3−09.4 H 2–48 GS-2016A-Q-101 B600 3500–6260 90 3 × 900† 1 × 1
012.1−11.2 PPA J1855–2328 GS-2015A-Q-98 B600 3750–6750 70 2 × 1000 2 × 2
013.1+05.0 Sa 3–96 GS-2015AQ-98 B600 3660–6750 55 3 × 600† 2 × 2
014.8−08.4 SB 20 GS-2015AQ-98 B600 3660–6750 90 3 × 1200 2 × 2
016.4−01.9 M 1–46 GS-2016A-Q-101 B600 3500–6260 64 3 × 600 1 × 1
017.6−10.2 A 51 GS-2016A-Q-101 B600 3500–6260 239 3 × 1000 1 × 1
020.7−05.9 Sa 1–8 GS-2016A-Q-101 B600 3500–6260 239 3 × 900 1 × 1
034.3+06.2 K 3–5 GN-2016A-Q-97 B600 3500–6000 309 3 × 900† 2 × 2
036.4−01.9 IPHAS 190438a GN-2015A-Q-405 B600 3850–6600 0 3 × 600 2 × 2
039.0−04.0 IPHAS 191716b GN-2015A-Q-405 B600 3850–6600 123 1 × 600† 2 × 2
051.3+01.8 PM 1–295 GN-2016A-Q-97 B600 3500–6000 282 3 × 1000 2 × 2
052.2+07.6 K 4–10 GN-2016A-Q-97 B600 3500–6000 266 3 × 1000 2 × 2
060.0−04.3 A 68 GN-2015A-Q-405 B600 3850–6600 120 3 × 1000† 2 × 2
066.8+02.9 IPHAS 194751c GN-2015A-Q-405 B600 3850–6600 80 3 × 1000 2 × 2
068.7+14.8 Sp 4–1 GN-2016A-Q-97 B600 3500–6000 37 3 × 900 2 × 2
075.7+35.8 Sa 4–1 GN-2015A-Q-405 B600 3850–6600 280 2 × 1200 2 × 2
075.9+11.6 AMU 1 GN-2012A-Q-124 B1200 4000–5500 147 4 × 360 2 × 2
078.5+18.7 A 50 GN-2016A-Q-97 B600 3500–6000 215 2 × 1000† 2 × 2
135.9+55.9 TS 01 GN-2006A-Q-82 B1200 3800–5000 25 8 × 700 2 × 2
211.2−03.5 M 1–6 GS-2015B-Q-103 B600 3500–6400 258 5 × 900 2 × 2
234.9−01.4 M 1–14 GS-2015B-Q-103 B600 3500–6400 0 2 × 770 2 × 2
236.9+08.6 PHR J0809–1650 GS-2015B-Q-103 B600 3500–6400 294 4 × 770 2 × 2
238.0+34.8 A 33 GS-2015B-Q-103 B600 3500–6400 207 5 × 450 2 × 2
249.8+07.1 PHR J0834–2819 GS-2016B-Q-65 B1200 4000–5500 50 3 × 950 2 × 2
250.3−05.4 PHR J0745–3535 GS-2015B-Q-103 B600 3500–6400 265 4 × 750 2 × 2
258.5−01.3 RCW 24 GS-2008B-Q-65 B1200 4090–5540 3 1 × 2400 2 × 2
273.6+06.1 HbDs 1 GS-2015B-Q-103 B600 3500–6400 0 3 × 400 2 × 2
281.0−05.6 IC 2501 GS-2015B-Q-103 B600 3500–6400 210 3 × 900 2 × 2
285.6−02.7 He 2–47 GS-2011A-Q-65 B1200 3900–5200d 90 1 × 1200 1 × 2
285.7−14.9 IC 2448 GS-2015B-Q-103 B600 3500–6400 61 1 × 770 2 × 2
288.7+08.1 ESO 216-2 GS-2015AQ-98 B600 3750–6750 90 3 × 1000 2 × 2
302.2−03.1 PHR J1244–6601 GS-2015AQ-98 B600 4000–6750 183 3 × 1000† 2 × 2
310.3+24.7 Lo 8 GS-2016A-Q-101 B600 3500–6260 277 3 × 600 1 × 1
312.6−01.8 He 2–107 GS-2011A-Q-65 B1200 3900–5200e 90 1 × 1800 1 × 2
315.4−08.4 PHR J1510–6754 GS-2012A-Q-85 B1200 4000–5450 337 2 × 600† 2 × 2
315.7+05.5 LoTr 8 GS-2011A-Q-65 B1200 3830–5200 134 1 × 2400 1 × 2
317.2+08.6 PHR J1424–5138 GS-2015A-Q-98 B600 3750–6750 282 3 × 600 2 × 2
323.6−04.5 WKK136–337 GS-2011A-Q-65 B1200 3800–5200 90 1 × 900 1 × 2
323.9+02.4 He 2–123 GS-2016A-Q-74 B1200 3950–5500 179 3 × 500 1 × 1
325.8−12.8 He 2–182 GS-2016A-Q-101 B600 3500–6260 310 3 × 900 1 × 1
326.0−06.5 He 2–151 GS-2016A-Q-101 B600 3500–6260 322 3 × 600 1 × 1
326.4+07.0 NeVe 3–2 GS-2011A-Q-65 B1200 3830–5200 225 1 × 1200 1 × 2
329.0+01.9 Sp 1 GS-2011A-Q-91 B1200 4000–5460 90 1 × 480 2 × 2
329.5+01.7 VBRC 7 GS-2015A-Q-98 B600 4000–6750 320 3 × 1200 2 × 2
331.4−03.5 He 2–162 GS-2016A-Q-101 B600 3500–6260 270 3 × 900 1 × 1
332.8−16.4 HaTr 6 GS-2015A-Q-98 B600 4000–5500 270 3 × 1000† 2 × 2
338.1−08.3 NGC 6326 GS-2009A-Q-35 B1200 4510–5960 90 1 × 1800† 1 × 2
349.3−04.2 Lo 16 GS-2009A-Q-35 B1200 4510–5960 100 1 × 1800 1 × 2
352.1−02.6 PHR J1736–3659 GS-2011A-Q-65 B1200 3830–5200 90 1 × 900 1 × 2
353.7+06.3 M 2–7 GS-2016A-Q-101 B600 3500–6260 90 3 × 900 1 × 1
354.5−03.9 SAB 41 GS-2008B-Q-65 B600 4260–7030 149 1 × 1800† 2 × 2
355.3−03.2 PPA J1747–3435 GS-2009A-Q-35 B1200 4100–5530 135 1 × 2400† 1 × 2
355.6−02.3 PHR J1744–3355 GS-2009A-Q-35 B1200 4100–5530 168 2 × 1950† 1 × 2
357.0−04.4 PHR J1756–3342 GS-2009A-Q-35 B1200 4100–5530 180 1 × 2400 1 × 2
357.1−05.3 BMP J1800–3408 GS-2009A-Q-35 B1200 4100–5530 35 1 × 2400 1 × 2
357.6−03.3 H 2–29 GS-2009A-Q-35 B1200 4100–5530 120 2 × 1950† 1 × 2
358.7−03.0 K 6–34 GS-2009A-Q-35 B1200 4100–5530 90 1 × 2400 1 × 2
359.1−02.3 M 3–16 GS-2008B-Q-65 B1200 4090–5540 90 4 × 1200 1 × 2

Notes. The PA column indicates the slit position angle in degrees, “exptime” is the integration time (underexposed spectra is denoted by †), and “bin” is the binning applied to the CCDs. (a)IPHASX J190438.6+021424, (b)IPHASX J191716.4+033447, (c)IPHASX J194751.9+311818, (d)4500–5900 Å, and (e)4500–5900 Å.

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