机译:在高射频和局部的恒紫外线和局部突出者中的粉尘衰减:对宇宙星形成速率密度的影响
Max-Planck-Institut for Astrophysics D-85748 Garching Germany;
Department of Physics and Astronomy The Johns Hopkins University 3400 North Charles Street Baltimore MD 21218 USA;
Max-Planck-Institut for Astrophysics D-85748 Garching Germany;
Spitzer Science Center Caltech MS 220-6 Pasadena CA 91125 USA;
Laboratoire d'Astrophysique de Marseille OAMP Universite Aix-marseille CNRS 38 rue Frederic Joliot-Curie 13388 Marseille Cedex 13 France;
Spitzer Science Center Caltech MS 220-6 Pasadena CA 91125 USA;
ICRAR/University of Western Australia 35 Stirling Highway Crawley WA 6009 Australia;
Observatories of the Carnegie Institution of Washington 813 Santa Barbara Street Pasadena CA 91101 USA;
California Institute of Technology MS 249-17 Pasadena CA 91125 USA;
NASA Goddard Space Flight Center Laboratory for X-ray Astrophysics Greenbelt MD 20771 USA;
PMC Univ Paris 06 UMR7095 Institut d'Astrophysique de Paris F-75014 Paris France;
California Institute of Technology MS 249-17 Pasadena CA 91125 USA;
California Institute of Technology MS 249-17 Pasadena CA 91125 USA;
California Institute of Technology MS 249-17 Pasadena CA 91125 USA;
Department of Physics and Astronomy Division of Astronomy and Astrophysics University of California Los Angeles CA 90095-1562 USA;
National Optical Astronomical Observatories 950 N. Cherry Avenue Tucson AZ 85719 USA;
Department of Astronomy Columbia University MC 2457 550 West 120th Street New York NY 10027 USA;
dust; extinction; galaxies: high-redshift; galaxies: peculiar; galaxies: starburst;
机译:在高射频和局部的恒紫外线和局部突出者中的粉尘衰减:对宇宙星形成速率密度的影响
机译:星系中的“超混合”粉尘排放。 I.北部GOODS目录和红移形成的宇宙星形成率密度6
机译:Herschel PEP / HerMES:尘埃衰减和总(UV + IR)星形成速率密度的红移演变(0≤z≤4)
机译:在附近的明星成型和爆炸星系的星形成和尘埃灭绝
机译:Swift / UVOT观察本地和高射频星系中的星形形成和灰尘衰减
机译:使用磁化转移效应对磁共振成像信号(QUEST和QUESP)的饱和时间和饱和功率相关性来量化化学交换饱和转移剂中的交换率:聚-1-赖氨酸和Starburst树枝状聚合物的pH校准
机译:紫外线选择的starbursts在高红移时的尘埃衰减及其影响 当地同行:对宇宙恒星形成速率密度的影响
机译:直接测量z中的灰尘衰减来自3D-HsT的1.5颗恒星形成星系:对尘埃几何和恒星形成率的影响。