...
首页> 外文期刊>Publications of the Astronomical Society of Japan >AKARI NEP field: Point source catalogs from GALEX and Herschel observations and selection of candidate lensed sub-millimeter galaxies
【24h】

AKARI NEP field: Point source catalogs from GALEX and Herschel observations and selection of candidate lensed sub-millimeter galaxies

机译:AKARI NEP领域:来自GALEX和Herschel观测的点源目录以及候选的亚毫米透镜透镜星系的选择

获取原文
获取原文并翻译 | 示例

摘要

The AKARI Wide North Ecliptic field is one of the most important cosmological fields because it lies in the continuous viewing zones for many space telescopes, e.g., Herschel, HST, and JWST, and it is also a natural high-visibility field from the L2 halo orbit. The field will be also the location of the deep survey for the Euclid mission. Finally, AKARI has made deep mid-IR observations using its nine continuous band filters in the North Ecliptic Pole (NEP) field. We analyzed GALEX and Herschel observations in the NEP field to build catalogs in seven bands: GALEX far UV and near UV, Herschel PACS 100 μm and 250 μm, and SPIRE 250 μm, 350 μm, and 500 μm with quality checks. The SPIRE catalogs are used to identify 61 (6 in a main list and 55 in a supplementary list) candidate lensed galaxies through red 350 μm to 500 μm colors. For the brightest of these candidates with 500 μm flux densities >100 mJy, follow-up observations in millimeter wavelengths have been carried out with the NOEMA interferometer. The high quality of these observations has allowed us to study and compare their morphology beyond that possible using Herschel data alone. We find that the majority of them appear as multiple objects. The redshift distribution of the sources in the main list is found to be in the range 1.5 < $z$ < 2.3. Their IR luminosities confirm that these sources are very likely strongly lensed galaxies.
机译:AKARI宽北黄道场是最重要的宇宙学场之一,因为它位于许多太空望远镜(例如Herschel,HST和JWST)的连续视区中,并且还是L2晕圈中的自然高可见性场轨道。该领域还将成为Euclid任务的深层调查的地点。最终,AKARI使用其在北黄极(NEP)场中的九个连续频带滤波器进行了深层中红外观测。我们分析了NEP领域中的GALEX和Herschel观测值,以建立七个波段的目录:GALEX远紫外线和近紫外线,Herschel PACS 100μm和250μm以及SPIRE 250μm,350μm和500μm,并进行了质量检查。 SPIRE目录用于通过350μm至500μm红色来识别61个(主列表中为6个,补充列表中为55个)候选透镜星系。对于这些最亮的,通量密度大于500μm且大于100μmJy的候选透镜,已使用NOEMA干涉仪进行了毫米波长的后续观察。这些观测结果的高质量使我们能够研究和比较其形态,而不仅仅是单独使用Herschel数据。我们发现它们大多数都显示为多个对象。发现主列表中源的红移分布在1.5 < $ z $ <2.3。它们的红外光度证实了这些来源很可能是强透镜星系。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号