... minutes, the resolution is 1", limiting star magnitude is 23m, the field of view is ... angular size of the image element - 0.23"), limiting stellar magnitude is 23.5-24 ... The resolution (seeing) is 0.9" with limiting stellar magnitude of 22 m . ...
... The upper limits on afterglow magnitude in R band were obtained. Observations of GRB afterglows with Russian-Turkish 1.5-m Telescope (RTT150) . ...
... As other blazars, 3C 279 light curve is expected to show microvariability (around 0.05 magnitudes in a short time scale), flares (around 1 magnitude in one week) and outbursts (many magnitudes in months or years). ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E32_Risquez01-27Apr07_17:23:54.pdf -- 503.2 Кб -- 27.04.2007 Похожие документы
... counterparts, in many cases brighter than magnitude 18, and (2) a significant ... sources are usually optically bright with magnitudes 10 ... 18 and can be easily and ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E37_Hudec01-16Feb07_17:08:21.pdf -- 742.0 Кб -- 16.02.2007 Похожие документы
... The OMC is able to measure variations in V smaller than 0.1 mag for objects brighter than magnitude 16-17 (depending on background) and smaller than 0.03 mag for objects brighter than magnitude 14, as listed in Table 2. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/J31_Mas-Hesse01-14Jun07_18:37:37.pdf -- 759.1 Кб -- 14.06.2007 Похожие документы
... This resulted in the magnitudes quoted in Table 1. 2.2. ... The magnitudes listed are B2 = 13.17, R2 = 12.95, i = 11.61. ... The magnitudes of this object are listed in Table 1. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G52_Torrejon01-26Apr07_13:48:22.pdf -- 108.1 Кб -- 26.04.2007 Похожие документы
... V band) should be up to 0.5 magnitudes (depending on the inclination of the system ... in V band) should be up to 0.5 magnitude (depending on the inclination of the system ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F40_Ziolkowski01-03Mar07_22:49:23.pdf -- 1545.4 Кб -- 03.03.2007 Похожие документы
... 10-8 s s-1 ; § 1) is 3 order of magnitude smaller than the Doppler effect due to the ... as previous values measured when the source was two order of magnitude more luminous ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G40_Enoto01-27Feb07_08:17:04.pdf -- 196.5 Кб -- 27.02.2007 Похожие документы