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项目对53平方度的银道面内天区开展了重新成像工作，该天区同时也是作为斯隆三期、四期项目组成部分的APOGEE/APOGEE-2巡天的观测目标，此项工作旨在为数十万颗红巨星获取高分辨率H波段光谱。本数据集将与2004至2005年间获取的银道面原始GLIMPSE观测数据相结合，用于测算近十年来银道面沿线天体的自行运动。本数据集或相关服务由IPAC下属的红外科学档案（Infrared Science Archive, IRSA）对外提供，该机构由加州理工学院依据与美国国家航空航天局签订的合同开展运营。