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arXiv 0902.3326astro-ph.GA
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UKIRT红外深空巡天深河外巡天数据发布2中的两颗遥远棕矮星

Two distant brown dwarfs in the UKIRT Infrared Deep Sky Survey Deep Extragalactic Survey Data Release 2

N. Lodieu, P. D. Dobbie, N. R. Deacon, B. P. Venemans, M. Durant

摘要:

我们在UKIRT红外深空巡天(UKIDSS)深河外巡天(DXS)数据发布2中发现了两颗棕矮星。这两个物体都是从DXS中的6平方度光度选择的,因为它们的蓝色J-K颜色和斯隆数字巡天(SDSS)条纹82中缺乏光学对应物。加拿大-法国-夏威夷望远镜遗产巡天(CFHT-LS)提供的额外光学测光证实了这些候选者可能的亚恒星性。随后对UDXS J221611.51+003308.1和UDXS J221903.10+002418.2进行的甲烷成像证实了它们是T7 $\pm$ 1和T6 $\pm$ 1矮星,测光距离为81(52-118 pc)和60(44-87 pc; 2 sigma置信水平)。在超深调查的第二次数据发布中,在较小的区域(0.77平方度)和较浅的深度进行了类似的搜索,没有返回任何晚T矮星候选者。考虑到DXS和UDS目前的面积和深度,我们研究中晚T矮星的数量与质量下降函数大致一致。这些棕矮星是在VIMOS 4领域中首次发现的,也是少数几个在射电望远镜中发现的T矮星之一。它们对研究T型矮星的标度高度具有重要的意义。

英文摘要:

We present the discovery of two brown dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Deep Extragalactic Survey (DXS) Data Release 2. Both objects were selected photometrically from six square degrees in DXS for their blue J-K colour and the lack of optical counterparts in the Sloan Digital Sky Survey (SDSS) Stripe 82. Additional optical photometry provided by the Canada-France-Hawaii Telescope Legacy Survey (CFHT-LS) corroborated the possible substellarity of these candidates. Subsequent methane imaging of UDXS J221611.51+003308.1 and UDXS J221903.10+002418.2, has confirmed them as T7$\pm$1 and T6$\pm$1 dwarfs at photometric distances of 81 (52-118 pc) and 60 (44-87 pc; 2 sigma confidence level). A similar search in the second data release of the Ultra Deep Survey over a smaller area (0.77 square degree) and shallower depth didn't return any late-T dwarf candidate. The numbers of late-T dwarfs in our study are broadly in line with a declining mass function when considering the current area and depth of the DXS and UDS. These brown dwarfs are the first discovered in the VIMOS 4 field and among the few T dwarfs found in pencil-beam surveys. They are valuable to investigate the scale height of T dwarfs.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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