Chemical composition of asymptotic giant branch stars in Galactic open clusters: Implications for the initial-final mass relation

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Table 4.

Absolute K_s and bolometric magnitudes of the stars derived using distances and extinctions from different cases.

Star	Case 1				Case 2		Case 3		Marigo et al. (2022)
	A_V	D	$M_{K_{s}}$ $M_{K_s}$	M_bol	$M_{K_{s}}$ $M_{K_s}$	M_bol	$M_{K_{s}}$ $M_{K_s}$	M_bol	$M_{K_{s}}$ $M_{K_s}$	M_bol
	(mag)	(pc)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
Case 63	2.45	1598	−7.65	−4.6	−7.84	−4.8	−7.87	−4.8	−7.86	−4.9
HD 292921	0.52	3542	−6.79	−4.2	−7.66	−5.3	−7.60	−5.2	−7.20	−4.7
IRAS 20540+5049	3.20	2730	−7.53	−4.4	−8.27	−5.4	−8.60	−4.8	−8.18	…
Case 473^★	3.49	3472	−8.15	−5.0	−8.33	−5.3	−8.67	−5.6	−8.35	−5.4
2MASS J20560894+505907^★	3.20	2813	−7.52	−4.3	−7.95	−5.1	−8.52	−5.5	−7.38	…
Case 121^★	1.13	3912	−8.13	−5.0	−8.78	−5.7	−9.06	−5.6	−8.73	−5.6
Case 588^★	0.87	3692	−8.03	−4.8	−8.09	−4.9	−8.09	−4.9	−8.17	−5.2
DH Mon^★	1.00	3223	−7.62	−4.5	−8.31	−5.1	−7.83	−4.7	…	…
IRAS 19582+2907	2.85	3830	−8.03	−4.8	−8.31	−4.7	−8.22	−5.1	−7.89	−5.4
HD 11800	1.46	1101	−7.15	−4.5	−7.06	−4.5	−7.47	−4.8	−7.28	…
[D75b] Star30^★	1.05	3120	−6.80	−3.8	−7.21	−4.7	−7.08	−4.5	−6.77	−3.9
BD +60 2534	1.60	1517	−6.83	−4.4	−6.82	−4.3	−6.86	−4.6	−7.05	…
MSB 75	0.78	1880	−8.28	−5.1	−8.38	−5.2	−8.41	−5.2	−8.49	−5.4
C* 908	1.71	3394	−7.50	−4.3	−8.16	−5.0	−7.69	−4.6	−7.78	−4.6
CSS 0291	0.30	2216	−7.48	−4.4	−7.59	−4.8	−7.63	−4.9	−7.72	−5.0
V493 Mon^★	1.11	2768	−7.41	−4.3	−7.85	−4.5	−7.61	−4.5	−7.40	−4.3

Notes. The extinction and distance values in case 1 are derived following the approximations made by Lallement et al. (2022) and Bailer-Jones et al. (2021), respectively (see text). The stars marked with an asterisk have a Gaia DR3 astrometry fidelity flag < 0.5. We include here the luminosities values derived in Marigo et al. (2022) for comparison.

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