Discovery of a bright radio transient in M 82: a new radio supernova? | A&A

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Table 1:

Details of the detected compact sources in our VLA observations with statistical errors on the 22.2 GHz flux densities.
Source	Date	Peak flux	Integrated flux
		[mJy beam^-1]	[mJy]
M 82 transient	24/03/2008	104.4 $\pm$ 1.3	99.6 $\pm$ 2.3
(42.82+59.54)	03/05/2008	89.9 $\pm$ 0.1	88.4 $\pm$ 0.2
	08/04/2009	11.1 $\pm$ 0.1	9.2 $\pm$ 0.2
44.0+59.6	28/01/2007	15.0 $\pm$ 0.2	77.8 $\pm$ 1.0
	03/05/2008	12.5 $\pm$ 0.1	11.0 $\pm$ 0.2
	08/04/2009	14.7 $\pm$ 0.1	12.4 $\pm$ 0.2
M 81*	28/01/2007	71 $\pm$ 1	72 $\pm$ 1
	03/05/2008	150	150
	08/04/2009	195 $\pm$ 3	179 $\pm$ 5
0945+6924	28/01/2007	14.3 $\pm$ 0.2	14.4 $\pm$ 0.3
	03/05/2008	14.8 $\pm$ 0.1	14.7 $\pm$ 0.2
	08/04/2009	13.8 $\pm$ 0.2	12.2 $\pm$ 0.3
0948+6848	28/01/2007	22.5 $\pm$ 0.2	24.3 $\pm$ 0.3
	03/05/2008	59.1 $\pm$ 0.2	59.8 $\pm$ 0.3
	08/04/2009	63.6 $\pm$ 0.4	56.3 $\pm$ 0.6
1004+6936	28/01/2007	31.0 $\pm$ 0.2	30.8 $\pm$ 0.3
	03/05/2008	30.9 $\pm$ 0.2	30.4 $\pm$ 0.2
	08/04/2009	34.6 $\pm$ 0.3	30.8 $\pm$ 0.4

Source LaTeX | All tables | In the text