Table 6.
Catalog of stars in field (i) with spectral type classification.
| ID | mF606W | RA | Dec | S/N | B | Teff | log g | [Fe/H] | vr | Δvr | Spectral type | P |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 80 | 20.28 | 0:54:40.2 | −37:41:54.9 | 22.9 | 1 | 7643 | 1.50 | 0.10 | 191 | 7 | F0II | 2 |
| 119 | 20.64 | 0:54:44.0 | −37:41:50.9 | 20.3 | 1 | 9377 | 1.50 | −0.10 | 149 | 18 | A1Ib … A5II | 2 |
| 123 | 20.61 | 0:54:41.2 | −37:41:34.2 | 8.2 | 2 | 17 629 | 2.70 | −0.20 | 186 | 28 | B3Ib | 1 |
| 151 | 20.78 | 0:54:43.4 | −37:41:51.1 | 23.3 | 1 | 9377 | 1.90 | −0.10 | 180 | 10 | A1Ib | 2 |
| 192 | 20.92 | 0:54:42.7 | −37:42:07.3 | 19.4 | 1 | 9377 | 1.90 | −0.10 | 157 | 26 | A1Ib | 2 |
| 201 | 21.15 | 0:54:44.7 | −37:41:48.3 | 15.0 | 1 | 4175 | 0.80 | −0.30 | 159 | 12 | K3Iab | 2 |
| 209 | 21.03 | 0:54:41.0 | −37:41:54.3 | 18.5 | 1 | 8357 | 1.80 | 0.10 | 147 | 9 | A5II … A1Ib | 2 |
| 216 | 21.28 | 0:54:43.0 | −37:41:50.5 | 13.9 | 0 | 3843 | 0.47 | −0.12 | 173 | 14 | M1Ia-ab … K3Iab | 2 |
| 223 | 21.05 | 0:54:42.1 | −37:41:36.1 | 14.7 | 1 | 9377 | 1.90 | −0.10 | 175 | 26 | A1Ib | 2 |
| 243 | 21.38 | 0:54:44.2 | −37:42:23.8 | 16.0 | 2 | 3845 | 0.34 | 0.10 | 168 | 19 | K3Iab … M1Ia-ab | 2 |
| 246 | 21.33 | 0:54:44.8 | −37:41:46.9 | 14.9 | 2 | 3838 | 0.55 | −0.11 | 157 | 6 | K3Iab … M1Ia-ab | 2 |
| 247 | 21.10 | 0:54:43.2 | −37:42:00.7 | 17.8 | 1 | 9377 | 1.90 | −0.10 | 157 | 32 | A1Ib | 2 |
| 252 | 21.13 | 0:54:41.5 | −37:41:41.1 | 17.5 | 1 | 17 629 | 2.70 | −0.20 | 187 | 11 | B3Ib | 2 |
| 260 | 21.38 | 0:54:41.7 | −37:41:54.0 | 15.7 | 1 | 3878 | 0.00 | −0.30 | 171 | 17 | K3Iab … K5I | 2 |
| 283 | 21.17 | 0:54:40.2 | −37:41:53.3 | 15.4 | 0 | 30 000 | 0.00 | 0.00 | 999 | 999 | OB | 0 |
| 301 | 21.56 | 0:54:42.1 | −37:41:51.7 | 14.5 | 2 | 3836 | 0.70 | −0.40 | 174 | 13 | K5III … M1Ia-ab | 2 |
| 352 | 21.40 | 0:54:41.2 | −37:41:36.8 | 14.9 | 1 | 8357 | 1.80 | 0.10 | 146 | 15 | A5II … A1Ib | 2 |
| 395 | 21.75 | 0:54:40.8 | −37:41:40.6 | 14.6 | 2 | 3894 | 0.40 | −0.30 | 183 | 2 | K3Iab … M1Ia-ab | 2 |
| 402 | 21.46 | 0:54:44.9 | −37:42:30.7 | 7.5 | 1 | 30 000 | 0.00 | 0.00 | 999 | 999 | OBem | 2 |
| 407 | 21.70 | 0:54:43.5 | −37:42:14.1 | 13.3 | 1 | 3775 | 0.80 | −0.30 | 166 | 21 | K2III … M1Iab | 2 |
| 435 | 21.51 | 0:54:41.6 | −37:41:58.6 | 15.4 | 1 | 9377 | 1.90 | −0.10 | 162 | 8 | A1Ib | 2 |
| 462 | 21.57 | 0:54:44.1 | −37:41:45.2 | 13.4 | 2 | 8357 | 1.80 | 0.10 | 152 | 14 | A5II … F6Iab | 1 |
| 468 | 21.61 | 0:54:41.7 | −37:41:50.4 | 13.2 | 1 | 8357 | 1.80 | 0.10 | 166 | 39 | A5II | 2 |
| 479 | 21.87 | 0:54:41.1 | −37:41:59.3 | 7.7 | 1 | 4175 | 0.80 | −0.30 | 161 | 25 | K2IIIb … K3Iab | 2 |
| 487 | 21.61 | 0:54:42.8 | −37:41:38.8 | 5.4 | 1 | 6011 | 1.50 | 0.10 | 184 | 9 | F6Iab | 1 |
| 488 | 21.82 | 0:54:39.9 | −37:41:54.5 | 9.9 | 0 | 4576 | 1.00 | 0.00 | 181 | 6 | K2I … M1Iab | 2 |
| … | ||||||||||||
| 1003 | 22.82 | 0:54:43.3 | −37:41:53.7 | 0 | 0 | 0 | 9.99 | 9.99 | 999 | 999 | PER | 0 |
| … | ||||||||||||
| 26 377 | 24.33 | 0:54:43.6 | −37:41:41.2 | 3.4 | 2 | 3969 | 1.30 | −0.30 | 168 | 14 | K4III−K5III | 1 |
| 26 433 | 24.27 | 0:54:42.5 | −37:41:40.1 | 4.0 | 1 | 3810 | 1.10 | 0.00 | 157 | 17 | M0III | 1 |
| 26 596 | 24.26 | 0:54:43.9 | −37:41:55.7 | 3.2 | 2 | 3915 | 1.46 | 0.25 | 193 | 10 | K5III | 0 |
| 26 762 | 24.34 | 0:54:41.5 | −37:42:01.8 | 3.1 | 1 | 3810 | 1.10 | 0.00 | 207 | 32 | M0III | 1 |
| 26 771 | 24.05 | 0:54:42.8 | −37:41:53.2 | 4.2 | 1 | 4379 | 2.60 | −0.10 | 197 | 8 | K2IIIb | 1 |
| 27 053 | 24.19 | 0:54:44.6 | −37:42:14.0 | 3.0 | 2 | 4159 | 1.90 | 0.10 | 151 | 19 | K4III | 1 |
| 27 597 | 24.20 | 0:54:44.5 | −37:41:45.9 | 3.4 | 2 | 3900 | 1.60 | −0.40 | 999 | 999 | K5III | 0 |
| 27 794 | 24.32 | 0:54:42.8 | −37:42:02.0 | 4.3 | 0 | 3939 | 1.80 | −0.30 | 183 | 90 | K3.5III | 0 |
| 28 087 | 24.09 | 0:54:43.2 | −37:42:09.3 | 3.1 | 0 | 0 | 9.99 | 9.99 | 999 | 999 | None | 0 |
| 29 133 | 24.36 | 0:54:44.2 | −37:41:45.5 | 3.8 | 0 | 3810 | 1.10 | 0.00 | 176 | 51 | M0III | 2 |
| 29 326 | 24.44 | 0:54:43.8 | −37:42:17.7 | 3.5 | 2 | 3915 | 1.46 | 0.25 | 175 | 19 | K5III | 1 |
| 29 932 | 24.30 | 0:54:42.6 | −37:41:57.5 | 3.0 | 2 | 3900 | 1.60 | −0.40 | 171 | 58 | K5III | 1 |
| 30 791 | 24.52 | 0:54:43.4 | −37:41:59.9 | 3.1 | 0 | 3915 | 1.46 | 0.25 | 166 | 17 | K5III | 0 |
| 30 801 | 24.94 | 0:54:41.4 | −37:41:39.8 | 3.2 | 2 | 3810 | 1.10 | 0.00 | 101 | 48 | M0III | 1 |
| 30 878 | 23.88 | 0:54:42.8 | −37:42:06.6 | 3.4 | 1 | 3244 | 0.20 | 0.00 | 169 | 14 | M6III | 2 |
| 32 224 | 24.25 | 0:54:43.3 | −37:41:54.3 | 9.1 | 1 | 3481 | 4.40 | −0.70 | 66 | 7 | K5V | 2 |
| 32 522 | 24.87 | 0:54:41.1 | −37:41:57.7 | 4.1 | 1 | 3665 | 1.20 | −0.20 | 163 | 35 | M3III | 1 |
| … |
Notes. Excerpt of catalog for field (i) with spectral type classification for spectra extracted with PampelMUSE, covering ranges of brighter and fainter F606W magnitudes (full table available at the CDS). Column 1, ANGST catalog ID; Col. 2, F606W magnitude; Col. 3, right ascension (J2000); Col. 4, declination (J2000); Col. 5, S/N estimate from PampelMUSE; Col. 6, flag “blending”: 2 = not obvious, 1 = minor, 0 = significant; Col. 7, effective temperature of best fit [K]; Col. 8, gravity of best fit; Col. 9, metallicity of best fit; Col. 10, radial velocity [km s−1]; Col. 11, radial velocity uncertainty [km s−1]; Col. 12, spectral type of best fit, or probable range of spectral type for ambiguous cases; Col. 13: flag “plausibility of fit”: 2 = very plausible, 1 = marginal, 0 = uncertain. “999” in Cols. 10 and 11 indicate uncertain results. Hot stars assigned OB, Teff is set to 30 000. PER: peculiar red star visible in HST image, not detected in MUSE cube.
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