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Table A.1.
Details of the spectra of CSPN observed with the INT.
| PN G | Name | Date | PA [°] | Exptime [s] |
|---|---|---|---|---|
| 038.4−03.3 | K 4–19 | 07-28-2014 | 205 | 3 × 900 |
| 039.5−02.7 | M 2–47 | 09-01-2016 | 0 | 3 × 2100 |
| 042.0+05.4 | K 3–14 | 07-12-2016 | 300 | 3 × 1800 |
| 044.3−05.6 | K 3–36 | 09-01-2016 | 57 | 3 × 2100 |
| 047.1+04.1 | K 3–21 | 07-13-2016 | 300 | 2 × 1800 |
| 054.4−02.5 | M 1–72 | 05-21-2015 | 305 | 3 × 2100 |
| 055.6+02.1 | He 1–2 | 07-13-2016 | 290 | 3 × 1800 |
| 107.6−13.3 | Vy 2–3 | 08-17-2016 | 310 | 2 × 1200 |
| 167.4−09.1 | K 3–66 | 01-10-2014 | 120 | 3 × 1800 |
| 184.0−02.1 | M 1–5 | 11-12-2016 | 74 | 1 × 1200 |
| 199.4+14.3 | PM 1–29 | 02-25-2016 | 64 | 3 × 1200 |
| – | K 4–50 | 11-08-2014 | 0 | 2 × 1500 |
Notes. The PA and exptime columns are the same as in Table A.2. The object K 4–50 (PK 208+01.1) was classified as possible PN by Acker et al. (1992).
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