Table 2: Stars in 30 Doradus used for calibration. Bright, isolated stars were chosen from the SPIREX image and used to calibrate the remaining stars in the image. Their L-band magnitudes and errors were determined from the standard star.
id RA (J2000) Dec (J2000) m_L

(h m s) (d m s) mag

11 05 38 06.6 -69 03 45.0 9.3 $\pm$ 0.2

14 05 38 09.6 -69 06 21.2 8.7 $\pm$ 0.1

26 05 38 16.7 -69 04 14.2 8.3 $\pm$ 0.1

28 05 38 17.0 -69 04 00.8 8.7 $\pm$ 0.2

29 05 38 17.6 -69 04 12.0 9.6 $\pm$ 0.1

**Table 2:** Stars in 30 Doradus used for calibration. Bright, isolated stars were chosen from the SPIREX image and used to calibrate the remaining stars in the image. Their L-band magnitudes and errors were determined from the standard star.
id	RA (J2000)	Dec (J2000)	m_L
	(h m s)	(d m s)	mag
11	05 38 06.6	-69 03 45.0	9.3 $\pm$ 0.2
14	05 38 09.6	-69 06 21.2	8.7 $\pm$ 0.1
26	05 38 16.7	-69 04 14.2	8.3 $\pm$ 0.1
28	05 38 17.0	-69 04 00.8	8.7 $\pm$ 0.2
29	05 38 17.6	-69 04 12.0	9.6 $\pm$ 0.1

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Results
	4 Analysis
	5 Discussion
	6 Conclusions
	References