论文标题

詹姆斯·韦伯太空望远镜揭示的红移11至20的第一批候选星系早期发布观察结果

First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations

论文作者

Yan, Haojing, Ma, Zhiyuan, Ling, Chenxiaoji, Cheng, Cheng, Huang, Jia-sheng

论文摘要

2022年7月13日,美国宇航局向全世界发布了詹姆斯·韦伯太空望远镜(JWST)早期发布观测(ERO)获得的数据。这些是这个期待已久的设施中的第一组科学级数据,标志着天文学新时代的开始。在对早期宇宙的研究中,JWST将使我们能够超越Z〜11,这是哈勃太空望远镜(HST)的1.7 UM红色截止点以前施加的红移边界。相比之下,JWST的Nircam达到5 UM。在JWST ERO目标中,附近有一个Galaxy群集SMACS 0723-73,它是一个巨大的群集,长期以来一直被认为是在放大背景星系中的潜在“宇宙望远镜”。 ERO六波段Nircam对此目标的观察结果涵盖了一个不受重力镜头增强的侧翼场,这也远远超出了HST。在这里,我们使用这些ERO数据在z> 11处搜索候选对象的结果。总共有87个这样的对象,使用标准的“辍学”技术确定。这些对象都在多个频段中检测到,因此不能虚假。对于他们中的大多数,它们的多带颜色与已知类型的污染物不一致。如果将检测到的辍学签名解释为预期的Lyman-Break,则意味着这些对象在Z〜11--20处。从先前有利的预测和要求进一步调查的情况下,预计如此高的红移的此类候选物体数量很大。此类物体上的JWST光谱将是至关重要的。

On July 13, 2022, NASA released to the whole world the data obtained by the James Webb Space Telescope (JWST) Early Release Observations (ERO). These are the first set of science-grade data from this long-awaited facility, marking the beginning of a new era in astronomy. In the study of the early universe, JWST will allow us to push far beyond z ~ 11, the redshift boundary previously imposed by the 1.7 um red cut-off of the Hubble Space Telescope (HST). In contrast, JWST's NIRCam reaches 5 um. Among the JWST ERO targets there is a nearby galaxy cluster SMACS 0723-73, which is a massive cluster and has been long recognized as a potential "cosmic telescope" in amplifying background galaxies. The ERO six-band NIRCam observations on this target have covered an additional flanking field not boosted by gravitational lensing, which also sees far beyond HST. Here we report the result from our search of candidate objects at z > 11 using these ERO data. In total, there are 87 such objects identified by using the standard "dropout" technique. These objects are all detected in multiple bands and therefore cannot be spurious. For most of them, their multi-band colors are inconsistent with known types of contaminants. If the detected dropout signature is interpreted as the expected Lyman-break, it implies that these objects are at z ~ 11--20. The large number of such candidate objects at such high redshifts is not expected from the previously favored predictions and demands further investigations. JWST spectroscopy on such objects will be critical.

扫码加入交流群

加入微信交流群

微信交流群二维码

扫码加入学术交流群,获取更多资源