机译:哈勃太空望远镜观测到的2个Pallas的形状和表面变化
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA;
Department of Astronomy, Cornell University, Ithaca, NY 14853, USA;
Jet Propulsion Laboratory, Pasadena, CA 91109, USA;
Department of Astronomy, University of Maryland, College Park, MD 20742, USA;
Department of Astronomy, University of Maryland, College Park, MD 20742, USA;
Space Telescope Science Institute (STScI), Baltimore, MD 80302, USA;
Hydraulx, Santa Monica, CA 90401, USA;
Applied Physics Laboratory, Laurel, MD 20723, USA;
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA;
Southwest Research Institute, Boulder, CO 80302, USA;
Southwest Research Institute, Boulder, CO 80302, USA;
机译:托尔曼表面亮度测试用于扩展的真实性。三,三个高红移星团中早期类型星系的哈勃空间望远镜轮廓和表面亮度数据
机译:哈勃太空望远镜微弱物体光谱仪对五个QSO的独特分组的观察:低zLyα森林吸收体的大小和形状*
机译:使用哈勃太空望远镜先进的照相机进行弱透镜应用的最佳星系形状测量
机译:哈勃遗产:通过哈勃太空望远镜的影像启发
机译:研究来自太空望远镜的弱透镜测量的波长依赖性,并估计哈勃太空望远镜边界平行场中减少的剪切信号
机译:BERT和PEGGY DUPONT演讲:哈勃太空望远镜的科学与文化
机译:使用哈勃太空望远镜高级相机进行测量的弱发射应用的最佳星系形状测量