**Table 3:** Spectroscopic and photometric $T_{\rm eff}$ for stars in selected fields.
		Spectroscopic information		Photometric information
Our Id	Reference Id	Spectral type	$\log T_{\rm eff}$	V	$\sigma_V$	$\log T_{\rm eff}$	$\chi$
14000005	p987	B0.5-0.7 I	4.35	11.835	0.012	4.48	3.2
14000008	p548	B0.7-1.5 I	4.32	12.079	0.006	4.50	3.1
14000020	p1257	B0 Ia	4.42	12.515	0.009	4.52	2.6
14000016	p1253	BN0.5 Ia	4.36	12.541	0.009	4.55	2.6
14000040	p488	B0.5-0.7 Ia	4.35	13.116	0.011	4.55	2.7
14000033	p1500	B0 Ib	4.42	13.147	0.007	4.51	2.2
14000034	p871	O3 V:	4.73	13.293	0.006	4.63	2.8
14000045	p1018	O3 If*/WN6-A	4.71	13.476	0.013	4.61	2.5
14000056	p643	ON9: I	4.52	13.550	0.013	4.65	2.7
14002516	p493	BC1 Ia	4.32	13.645	0.013	4.51	3.2
14001015	p1150	O4 III(f)	4.68	17.255	0.015	4.69	2.5
14000072	p930	OC9.7 Ib	4.46	13.820	0.005	4.60	2.4
14000081	p666	O3If*/WN7-A	4.71	13.826	0.013	4.52	2.8
14000065	p1311	O3 III(f*)	4.71	13.835	0.009	4.66	2.2
14001743	p1163	O3 V((f*))	4.73	14.040	0.008	4.65	2.3
14000097	p1531	O5: V	4.66	14.220	0.010	4.62	2.0
14000123	p724	O6: V:	4.64	14.396	0.011	4.64	2.0
14001394	p805	O5-6 V	4.65	14.526	0.016	4.66	2.9
14000124	p713	O3-6	4.68	14.680	0.018	4.68	2.8
14000184	p974	O5-6 III	4.64	14.826	0.012	4.71	1.9
14000822	p661	O5: V	4.66	16.620	0.014	4.70	2.2
14000183	p761	O3-6 V	4.68	14.858	0.014	4.70	2.2
14000194	p169	O9-B0 III	4.52	14.926	0.011	4.68	2.1
14000235	p974	O5-6 III	4.64	15.152	0.012	4.69	1.8
14000335	p538	B0-1 III	4.48	15.243	0.012	4.58	1.8
14000739	p700	O7: V((f))	4.61	16.441	0.018	4.68	1.6
14000009	p499	A0 Ia	3.99	11.802	0.008	4.23	3.3
14000111	p1350	O6 III(f*)	4.63	14.272	0.010	4.58	1.8
14000106	p1563	O7.5 II-III(f)	4.59	14.298	0.009	4.61	1.9
14000119	p1607	O7: If	4.59	14.336	0.009	4.58	1.8
14000160	p1317	O4 V	4.69	14.724	0.013	4.60	2.4
14000202	p1614	O5-6 V((f))	4.65	15.095	0.073	4.64	1.5
14000240	p977	O6: V	4.64	15.379	0.016	4.66	1.8
14000338	p615	O4-6 III(f)	4.66	15.656	0.018	4.67	2.0
14000359	p1209	O9-B0 V	4.54	15.729	0.027	4.65	2.9
14000043	wb3	A Ib (B3-5 I)	3.94	12.858	0.009	3.94	2.7
14000225	wb6	B2 III (O7-B0 V)	4.31	15.270	0.042	4.47	6.5
14000149	wb7	M I	3.56	14.168	0.008	3.63	2.0
14000197	wb8	B5:p (O9-B0)	4.19	14.931	0.009	4.41	1.7
14000155	wb9	B2 V (O5-6 III)	4.34	14.642	0.007	4.60	2.0
14002499	wb10	A0 Ib	3.99	13.240	0.009	4.12	3.3
14000128	wb11	A5 Ib (B1-1.5 V)	3.93	13.895	0.010	3.94	2.3
16000013	st4-54	O8 I(f)	4.55	13.111	0.008	4.60	2.3
16000021	st4-61	B1 I	4.32	13.289	0.008	4.07	2.1
16000028	st4-18	O5 I f	4.65	13.638	0.007	4.59	2.1
16000042	st4-26	O6.5 III((f))	4.62	14.042	0.009	4.59	2.0
16000051	st4-16	B1 I	4.32	13.951	0.011	4.49	2.2
16000070	st4-13	B1 I	4.32	14.235	0.008	4.55	1.7
16000071	st4-56	G3	3.77-3.71	13.491	0.008	3.81	1.9
16000074	st4-33	O7 V	4.61	14.362	0.010	4.51	1.8
16000099	st4-35	O8 V	4.59	14.720	0.009	4.51	1.7
16000122	st4-20	B1 III	4.41	15.076	0.011	4.46	1.7
16000142	st4-46	A3 V	3.94	14.869	0.008	4.00	1.5
16000144	st4-45	B0.5 V	4.51	15.252	0.010	4.44	1.4
16000149	st4-27	B2 III	4.31	15.297	0.011	4.46	1.6
16000151	st4-30	B1 III	4.41	15.324	0.009	4.45	1.8
16000159	st4-55	B0 V	4.52	15.277	0.010	4.42	1.4
16000162	st4-63	B0.5 V	4.51	15.395	0.009	4.46	1.4
16000164	st4-50	B0.5 V	4.51	15.461	0.009	4.50	1.3
16000168	st4-39	B0 V	4.52	15.446	0.011	4.50	1.6
16000198	st4-1	B2 III	4.31	15.537	0.012	4.39	1.7
16000206	st4-4	B1 V	4.44	15.587	0.010	4.47	1.1
16000216	st4-28	B0.5 V	4.51	15.691	0.011	4.50	1.5
16000217	st4-11	B1 III	4.41	15.589	0.010	4.35	1.5
16000229	st4-43	B2 V	4.34	15.659	0.010	4.38	1.4
16000242	st4-21	B1 V	4.44	15.793	0.012	4.41	1.5
16000248	st4-29	B1 V	4.44	15.780	0.009	4.46	1.4
16000249	st4-44	B2 V	4.34	15.743	0.031	4.30	3.9
160002257	st4-23	B1 V	4.44	15.766	0.010	4.40	1.3
16002083	st4-24	B2 III	4.31	15.950	0.009	4.44	1.2
16000306	st4-67	B2 I	4.27	15.991	0.016	4.44	1.3
16000311	st4-2	B1 V	4.44	16.046	0.010	4.43	1.4
16000317	st4-3	B2 V	4.34	16.094	0.010	4.48	1.3
16000325	st4-15	B2 V	4.34	16.067	0.010	4.41	1.3
16000327	st4-48	G8 III	3.69	15.676	0.008	3.62	1.3
16000332	st4-69	G5:	3.76-3.69	16.107	0.011	4.42	1.4
16000345	st4-51	B2 III	4.31	16.228	0.012	4.41	1.3
16000352	st4-66	B2 III	4.31	16.175	0.012	4.40	1.4
16000353	st4-19	B1 V	4.44	16.258	0.101	4.40	9.8
16000408	st4-5	B2 V	4.34	16.319	0.011	4.37	1.3
16000443	st4-36	B2 III	4.31	16.517	0.017	4.43	1.6
16000458	st4-34	B0.5 V	4.51	16.553	0.013	4.44	1.3
16000492	st4-38	B1 V	4.44	16.677	0.012	4.44	1.2
16000518	st4-10	B2:	4.34-4.27	16.627	0.012	4.36	1.2
16000521	st4-7	B2 V	4.34	16.668	0.013	4.29	1.3
16000546	st4-60	F8 V	3.79	16.455	0.011	4.13	1.2
16000580	st4-37	B2 V	4.34	16.887	0.013	4.40	1.2
16000750	st4-31	B2 V	4.34	17.205	0.016	4.37	1.2
16000757	st4-14	B2 V	4.34	17.199	0.175	4.38	3.1
16000793	st4-8	B1:	4.44-4.32	17.291	0.014	4.39	1.1
16000796	st4-9	B1 V	4.44	17.255	0.019	4.25	1.3
16000959	st4-58	G8-K2	3.75-3.69	17.514	0.023	4.27	1.3
16001084	st4-53	B2:	4.34-4.27	17.678	0.022	4.37	1.3
16001127	st4-49	B2 V	4.34	17.701	0.019	4.28	1.1
16001150	st4-41	B0 V	4.52	17.419	0.012	3.81	1.6
16001198	st4-59	B2 V	4.34	17.690	0.021	4.32	1.1
16001211	st4-40	O8 V	4.59	17.816	0.021	4.33	1.2
16001268	st4-47	B1 I	4.32	17.827	0.011	4.25	1.3

Spectral types from several sources in the literature, the corresponding effective temperatures, the photometric effective temperature, and the goodness of the psf profile fit. The reference identification are from: p, Parker (1993); wb, Walborn & Blades (1997); st, Schild & Testor (1992). The spectral types are taken from the compilation in Paper II, for the neighborhood of the Tarantula; from Walborn & Blades for Hodge 301; and from Schild & Testor for LH104.

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data analysis
	3 The IMF of the field population
	4 Discussion
	References
	Online Material