Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method

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Table C.1

Gaia EDR3 parallaxes and photometric and astrometric measurements for OB stars in the Rosette nebula cluster NGC 2244.

Name	ϖ(mas)	µ_α(masyr⁻¹)	µ_δ(masyr⁻¹)	G(mag)	RUWE
HD 46150	0.6431 ± 0.0340	−2.096 ± 0.031	−0.196 ± 0.030	6.7138	1.04
HD 46223	0.6968 ± 0.0264	−1.605 ± 0.026	0.111 ± 0.023	7.1998	1.06
HD 46149	0.6385 ± 0.0323	−1.608 ± 0.032	0.310 ± 0.028	7.5508	1.06
HD 46484	0.7025 ± 0.0279	−0.957 ± 0.028	1.153 ± 0.025	7.6406	1.11
HD 46106	0.6468 ± 0.0388	−2.006 ± 0.035	0.316 ± 0.029	7.8970	0.81
HD 46202	0.7087 ± 0.1148	−1.929 ± 0.110	−0.223 ± 0.110	8.1580	4.98
HD 46485	0.7713 ± 0.0236	−1.639 ± 0.027	0.198 ± 0.024	8.1657	0.90
HD 46056	0.6744 ± 0.0265	−1.861 ± 0.026	0.095 ± 0.024	8.1836	0.94
HD 259135	0.6499 ± 0.0396	−1.762 ± 0.038	0.559 ± 0.034	8.5275	1.31
HD 259012	1.3861 ± 0.1309	−2.647 ± 0.140	0.459 ± 0.124	9.2978	6.00
HD 259105	0.7132 ± 0.0244	−1.744 ± 0.022	0.081 ± 0.021	9.3355	1.16
HD 258691	0.6396 ± 0.1001	−2.215 ± 0.100	−0.609 ± 0.090	9.5245	6.97
GSC 00154-02337	0.6991 ± 0.0220	−1.547 ± 0.020	0.288 ± 0.018	9.6817	0.97
GSC 00154-02504	0.7163 ± 0.0303	−1.932 ± 0.033	0.265 ± 0.032	10.5832	0.99
HD 259172	0.7800 ± 0.0430	−1.707 ± 0.041	0.789 ± 0.035	10.6365	2.11
HD 259300	0.6971 ± 0.0326	−1.795 ± 0.030	0.235 ± 0.029	10.6983	2.06
NGC 2244 193	0.5579 ± 0.1402	−1.353 ± 0.120	0.255 ± 0.107	10.7182	5.58
HD 259238	0.6460 ± 0.0278	−1.458 ± 0.026	0.588 ± 0.024	11.0311	1.34
GSC 00154-01247	0.6486 ± 0.0218	−0.966 ± 0.025	0.609 ± 0.021	11.0388	1.04
GSC 00154-01007	0.6727 ± 0.0193	−1.473 ± 0.019	0.700 ± 0.017	11.1379	0.84
GSC 00154-02187	0.6883 ± 0.0186	−0.428 ± 0.017	0.389 ± 0.016	11.1721	0.90
HD259268	0.4636 ± 0.1233	−1.449 ± 0.091	0.277 ± 0.090	11.1782	3.50
GSC 00154-01016	0.6706 ± 0.0213	−1.440 ± 0.020	0.075 ± 0.020	11.3139	0.87
GSC 00154-00234	0.4683 ± 0.0200	−0.901 ± 0.020	−0.071 ± 0.017	11.4294	1.15
GSC 00154-02141	0.7172 ± 0.0199	−1.779 ± 0.026	0.272 ± 0.022	11.5531	1.11
GSC 00154-01753	0.6008 ± 0.0226	−1.731 ± 0.021	0.193 ± 0.020	11.8841	1.17
GSC 00154-02247	0.6644 ± 0.0155	−1.806 ± 0.016	0.427 ± 0.014	12.7080	1.00
GSC 00154-02164	0.6654 ± 0.0231	−2.042 ± 0.023	−0.268 ± 0.021	12.7863	1.24
ALS 15339	0.2269 ± 0.0264	−0.361 ± 0.027	−0.102 ± 0.024	14.5999	1.09
ALS 15335	0.1942 ± 0.0247	0.073 ± 0.026	0.542 ± 0.023	14.6297	1.02
ALS 15336	0.1959 ± 0.0324	0.072 ± 0.029	0.591 ± 0.027	15.0479	0.90

Notes. The names of objects used for the distance estimate of the cluster are in bold. We rejected the other objects based on their RUWE factor, discrepant distance or discrepant proper motions.

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