VLBA observations of radio faint Fermi-LAT sources above 10 GeV

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Volume 594 (October 2016)

A&A, 594 (2016) A60

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Table 2

Modelfit details for the extended sources.

1FHL name	Component	S^a	σ _S	a ^b	b ^b	D _core ^c	Orientation^d
		mJy	mJy	mas	mas	mas	deg


J0338.4+1304	Core	6.33	0.29	0.80	0.00	−	−
	C1	3.94	0.29	0.39	0.00	1.46	−28.0
J1315.0+2346	Core	51.27	0.12	0.22	0.00	−	−
	C1	30.57	0.33	1.76	0.72	0.50	−49.1
J1809.3+2040	Core	26.82	0.20	0.67	0.00	−	−
	C1	14.48	0.72	5.02	1.46	1.36	−18.7
J1942.8+1034	Core	53.30	0.78	0.73	0.52	−	−
	C1	13.07	0.41	1.06	0.00	0.72	89.0
J2223.4+0104	Core	6.80	0.24	0.96	0.30	−	−
	C1	3.41	0.13	0.88	0.00	1.35	157.4

Notes.

^(a)

Fitted core flux density at 5 GHz.

^(b)

a and b are the nominal FWHM of the major and minor axes of the deconvolved elliptical Gaussian component measured in mas.

^(c)

Distance from the core of the C1 Gaussian component.

^(d)

Orientation of the extended structure. Angles are measured from north through east.

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