论文标题
Lick天文台的研究成果1965- 2019年
Research Output from Lick Observatory for 1965-2019
论文作者
论文摘要
从1965年到2019年，舔观测站（LO）的生产力进行了审查，这是55年的时间，这是Shane 3 M望远镜是世界第二大天文反射器，但过渡到10 m地面光学望远镜的时代。此处使用的生产率度量是每年的裁判次数，其中提出的结果至少部分基于汉密尔顿山上的LO望远镜进行的观察结果。规定了指导该指标计数的标准。已经编译了与Lick天文台观察有关的论文参考书目，并通过NASA ADS库提供。 在1975年至1982年之间，天文台的总体生产率（计数所有望远镜）都达到了广泛的最大最大值。这一时期也对应于Shane 3 M望远镜的最高生产率。作者网络表明，这一时期是通过LO引入数字探测器系统的参与，尤其是在Shane望远镜上。 1983年之后，LO的整体生产率显示出净长期降低，但在此减少的情况下叠加了另外两个较小的峰值。 1996年左右发生了一个稍小的峰值，并且与Shane望远镜的Cassegrain和CoudéFoci的CCD光谱仪相关。 2012年左右的第三个较小的峰值可以归因于加州大学伯克利分校源自加州大学的超新星研究的增加。作者网络有助于记录在这些高峰时段使用LO望远镜的UC天文社区。记录了第一作者的机构隶属关系。
The productivity of Lick Observatory (LO) is reviewed over the years from 1965 to 2019, a 55 yr period which commences with the Shane 3 m telescope being the second-largest astronomical reflector in the world, but transitions into the era of 10 m ground-based optical telescopes. The metric of productivity used here is the annual number of refereed papers within which are presented results that are based at least in part on observations made with the telescopes of LO on Mount Hamilton. Criteria are set forth that have guided the counting of this metric. A bibliography of papers pertinent to observations from Lick Observatory has been compiled, and is made available through a NASA ADS library. The overall productivity of the observatory, counting all telescopes, went through a broad maximum between the years 1975 and 1982. This period also corresponds to a maximum in productivity of the Shane 3 m telescope. An author network shows that this period is attended by the introduction of digital detector systems at LO, particularly at the Shane telescope. Following 1983 the overall productivity of LO shows a net long-term decrease but with two other lesser peaks superimposed on that decrease. A slightly smaller peak occurs around 1996 and is associated with programs taking advantage of CCD spectrometers at both cassegrain and coudé foci of the Shane telescope. A third lesser peak around 2012 can be attributed to a rise in extragalactic supernova studies originating out of UC Berkeley. Author networks serve to document the UC astronomical communities that were using LO telescopes at these peak times. Institutional affiliations of first authors are documented.
