APOGLIMPSE Archive

The APOGLIMPSE project re-images 53 square degrees of the inner Galactic plane that have also been targeted by the APOGEE/APOGEE-2 surveys - Sloan III and IV programs to obtain high resolution H band spectroscopy for hundreds of thousands of red giants. The data will be combined with the original GLIMPSE observations of the Galactic plane in 2004-2005 to measure the proper motions of the sources along the Galactic plane over the past decade. This dataset or service is made available by the Infrared Science Archive (IRSA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

APOGLIMPSE项目（APOGLIMPSE）对银道面内侧53平方度的天区进行了重新成像，该天区同时也是APOGEE/APOGEE-2巡天（APOGEE/APOGEE-2）——斯隆第三、第四期计划——的观测目标，此类巡天项目旨在为数十万颗红巨星获取高分辨率H波段光谱。该项目获取的数据将与2004至2005年间GLIMPSE巡天（GLIMPSE）获取的银道面原始观测数据相结合，以测算近十年来银道面天区内各天体的自行。本数据集或服务由IPAC下属的红外科学档案馆（Infrared Science Archive, IRSA）提供，IPAC由加州理工学院（California Institute of Technology）根据与美国国家航空航天局（National Aeronautics and Space Administration）签订的合同开展运营。