Discovery of very high energy γ-ray emission from the BL Lacertae object PKS 0301−243 with H.E.S.S.

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Volume 559 (November 2013)

A&A, 559 (2013) A136

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Table 3

Magnitudes^a at different epochs from Swift/UVOT data in all bands.

Observation ID	V	B	U	UVW1	UVM2	UVW2

00038098001	15.43 ± 0.07	15.77 ± 0.06	14.95 ± 0.06	14.83 ± 0.07	14.79 ± 0.07	14.92 ± 0.07
00038368001	15.43 ± 0.05	15.74 ± 0.05	14.83 ± 0.05	14.76 ± 0.06	14.76 ± 0.06	14.87 ± 0.06
00038098002	15.65 ± 0.06	15.96 ± 0.06	15.12 ± 0.06	15.03 ± 0.07	14.99 ± 0.07	15.10 ± 0.06
00038098003	15.18 ± 0.06	15.47 ± 0.06	14.47 ± 0.06	14.33 ± 0.06	14.29 ± 0.06	14.36 ± 0.06
00038098004	–^b	–^b	14.68 ± 0.05	14.58 ± 0.06	–^b	14.71 ± 0.06
00038098005	–^b	–^b	14.76 ± 0.05	14.69 ± 0.06	–^b	14.76 ± 0.06
00038098006	15.43 ± 0.05	15.66 ± 0.05	14.83 ± 0.05	14.61 ± 0.06	14.55 ± 0.06	14.67 ± 0.06

Notes.

^(a)

Not corrected for Galactic extinction.

^(b)

No observations were taken in these filters for these observation IDs. For the other reported measurements, the exposure varies for the different filters and observations but is of the order of a few hundred seconds in these cases.

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