Table 1
Basic information of the program stars and spectra.
Stellar cluster | Star | Gaia DR3 ID | RA (deg) | Dec (deg) | G (mag) | S/N H-band | S/N K-band |
---|---|---|---|---|---|---|---|
NGC 7789 | N7789_1 | 1995061928762465536 | 359.263535573 | 56.766078036 | 9.75 | 359 | 327 |
Age = 1.55 Gyr | N7789_2 | 1995014409242207872 | 359.293345577 | 56.713695317 | 9.86 | 356 | 314 |
Rgc = 9.43 kpc | N7789_4 | 1995059592301326848 | 359.074303178 | 56.668800703 | 10.22 | 255 | 226 |
NGC 7044 | N7044_1 | 1969807040026523008 | 318.321873119 | 42.484572587 | 11.79 | 481 | 404 |
Age = 1.66 Gyr | N7044_2 | 1969807276235623552 | 318.330484209 | 42.507969696 | 11.90 | 426 | 327 |
Rgc = 8.73 kpc | N7044_3 | 1969806073644788992 | 318.397775571 | 42.460809968 | 12.20 | 388 | 346 |
N7044_4 | 1969800576086654592 | 318.256942841 | 42.403479143 | 12.21 | 412 | 328 | |
NGC 6819 | N6819_a | 2076394728016615680 | 295.479787235 | 40.239351300 | 10.07 | 655 | 519 |
Age = 2.24 Gyr | N6819_b | 2076582950658667264 | 295.284268649 | 40.325501253 | 10.13 | 519 | 364 |
Rgc = 8.03 kpc | |||||||
Ruprecht 171 | Rup171_1 | 4103073693495483904 | 277.989813692 | −15.980947363 | 10.01 | 397 | 336 |
Age = 2.75 Gyr | Rup171_2 | 4102882309792631552 | 278.022115687 | −16.133756431 | 10.45 | 383 | 311 |
Rgc = 6.90 kpc | |||||||
Trumpler 5 | Trumpler5_1 | 3326783231129992704 | 99.253875467 | 9.496152447 | 10.72 | 382 | 359 |
Age = 4.27 Gyr | |||||||
Rgc = 11.21 kpc | |||||||
King 11 | King11_1 | 2211216117949545216 | 356.988703461 | 68.595172524 | 11.66 | 372 | 355 |
Age = 4.47 Gyr | King11_2 | 2211121972266402304 | 356.899458081 | 68.559189268 | 12.04 | 395 | 348 |
Rgc = 10.21 kpc | King11_3 | 2211220211058075776 | 356.910794815 | 68.656763219 | 12.24 | 195 | 183 |
NGC 6791 | N6791_2 | 2051105616974709504 | 290.316961400 | 37.77952520 | 12.25 | 168 | 153 |
Age = 8.31 Gyr | N6791_3 | 2051287002031070208 | 290.207176626 | 37.72853365 | 12.39 | 159 | 138 |
Rgc = 7.94 kpc |
Notes. The ages and Rgc are from Cantat-Gaudin et al. (2020) except for NGC 6791 (Brogaard et al. 2021). The signal-to-noise ratios (S/N) were obtained from the fits header of each spectrum, using the value for order 48 as representative of the H-band and order 33 for the K-band.
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