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Daylight Photometry of C/2006 P1

机译:C / 2006 P1的日光光度法

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摘要

On 2007 Jan. 15.479 UT, ten co-added 0.12-sec unfiltered CCD exposures of comet C/2006 P1 (McNaught) were taken by J. Srba and E. Brezina (Vsetin Observatory 6.3-cm f/8 Maksutov-Cassegrain telescope + SBIG ST-7 CCD camera + neutral-density filter; shielded to 120 square mm of active telescope area) during broad daylight, The CCD frames, which were processed using standard reduction procedures, were measured in a variety of circular apertures (centered on the central condensation of the coma) for brightness and were corrected for atmospheric extinction. The comparison object was Venus (assuming mag -3.9).
机译:2007年1月15.UT(UT),J.Srba和E.Brezina(维塞丁天文台6.3-cm f / 8马克苏托夫-卡塞格林望远镜+)共拍摄了10张共加0.12秒未经过滤的CCD彗星C / 2006 P1(McNaught)。 SBIG ST-7 CCD摄像机+中性密度滤镜;在白天时被屏蔽到120平方毫米的活动望远镜区域),使用标准缩小程序处理的CCD镜框在各种圆形光圈(以中心昏迷)的亮度,并针对大气消光进行了校正。比较对象是金星(假设mag -3.9)。

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