Related Research Articles
The Max Planck Society for the Advancement of Science is a formally independent non-governmental and non-profit association of German research institutes. Founded in 1911 as the Kaiser Wilhelm Society, it was renamed to the Max Planck Society in 1948 in honor of its former president, theoretical physicist Max Planck. The society is funded by the federal and state governments of Germany.
The Max Planck Institute for Astrophysics (MPA) is a research institute located in Garching, just north of Munich, Bavaria, Germany. It is one of many scientific research institutes belonging to the Max Planck Society.
The Max Planck Institute for Extraterrestrial Physics is part of the Max Planck Society, located in Garching, near Munich, Germany. In 1991 the Max Planck Institute for Physics and Astrophysics split up into the Max Planck Institute for Extraterrestrial Physics, the Max Planck Institute for Physics and the Max Planck Institute for Astrophysics. The Max Planck Institute for Extraterrestrial Physics was founded as sub-institute in 1963. The scientific activities of the institute are mostly devoted to astrophysics with telescopes orbiting in space. A large amount of the resources are spent for studying black holes in the Milky Way Galaxy and in the remote universe.
The Max Planck Institute for Gravitational Physics is a Max Planck Institute whose research is aimed at investigating Einstein's theory of relativity and beyond: Mathematics, quantum gravity, astrophysical relativity, and gravitational-wave astronomy. The institute was founded in 1995 and is located in the Potsdam Science Park in Golm, Potsdam and in Hannover where it closely collaborates with the Leibniz University Hannover. Both the Potsdam and the Hannover parts of the institute are organized in three research departments and host a number of independent research groups.
The Max Planck Institute for Physics (MPP) is a research institute located in Garching, near Munich, Germany. It specializes in high energy physics and astroparticle physics. The MPP is part of the Max Planck Society and is also known as the Werner Heisenberg Institute, after its first director in its current location.
The Gottfried Wilhelm Leibniz Prize, or Leibniz Prize, is awarded by the German Research Foundation to "exceptional scientists and academics for their outstanding achievements in the field of research". Since 1986, up to ten prizes have been awarded annually to individuals or research groups working at a research institution in Germany or at a German research institution abroad. It is considered the most important research award in Germany.
The Alexander von Humboldt Foundation is a foundation that promotes international academic cooperation between excellent scientists and scholars from Germany and from abroad. It was established by the government of the Federal Republic of Germany and is funded by the Federal Foreign Office, the Federal Ministry of Education and Research, the Federal Ministry for Economic Cooperation and Development as well as other national and international partners.
The Gamma-Ray Burst Optical/Near-Infrared Detector (GROND) is an imaging instrument used to investigate Gamma-Ray Burst afterglows and for doing follow-up observations on exoplanets using transit photometry. It is operated at the 2.2-metre MPG/ESO telescope at ESO's La Silla Observatory in the southern part of the Atacama desert, about 600 kilometres north of Santiago de Chile and at an altitude of 2,400 metres.
The Alexander von Humboldt Foundation of Germany bestows the Sofia Kovalevskaya Award every two years. Sofia Kovalevskaya (1850–1891) was the first major Russian female mathematician, who made important contributions to mathematical analysis, differential equations and mechanics, and the first woman appointed to a full professorship in Northern Europe. This prestigious award named in her honor is given to promising young academics to pursue their line of research in the sciences or arts and humanities. The foundation encourages applications from all areas of the academy so long as the investigator received a Ph.D. in the last six years and may be categorized as "top flight" by their publications and experience as commensurate with age.
Donald Delbert Clayton was an American astrophysicist whose most visible achievement was the prediction from nucleosynthesis theory that supernovae are intensely radioactive. That earned Clayton the NASA Exceptional Scientific Achievement Medal (1992) for “theoretical astrophysics related to the formation of (chemical) elements in the explosions of stars and to the observable products of these explosions”. Supernovae thereafter became the most important stellar events in astronomy owing to their profoundly radioactive nature. Not only did Clayton discover radioactive nucleosynthesis during explosive silicon burning in stars but he also predicted a new type of astronomy based on it, namely the associated gamma-ray line radiation emitted by matter ejected from supernovae. That paper was selected as one of the fifty most influential papers in astronomy during the twentieth century for the Centennial Volume of the American Astronomical Society. He gathered support from influential astronomers and physicists for a new NASA budget item for a gamma-ray-observatory satellite, achieving successful funding for Compton Gamma Ray Observatory. With his focus on radioactive supernova gas Clayton discovered a new chemical pathway causing carbon dust to condense there by a process that is activated by the radioactivity.
eROSITA is an X-ray instrument built by the Max Planck Institute for Extraterrestrial Physics (MPE) in Germany. It is part of the Russian–German Spektr-RG space observatory, which also carries the Russian telescope ART-XC. It was launched by Roscosmos on 13 July 2019 from Baikonur, and deployed in a 6-month halo orbit around the second Lagrange point (L2). It began collecting data in October 2019. Due to the breakdown of institutional cooperation between Germany and Russia after the invasion of Ukraine, the instrument stopped collecting data on February 26, 2022.
GRB 160625B was a bright gamma-ray burst (GRB) detected by NASA's Fermi Gamma-ray Space Telescope on 25 June 2016 and, three minutes later, by the Large Area Telescope. This was followed by a bright prompt optical flash, during which variable linear polarization was measured. This was the first time that these observations were made when the GRB was still bright and active. The source of the GRB was a possible black hole, within the Delphinus constellation, about 9 billion light-years (light travel distance) away (a redshift of z = 1.406). It had a fluence of 5.7×10−4 erg cm−2, and energy of 5 × 1054 erg.
Uwe Paul Erich Thumm is a German-American physicist with research interests in atomic, molecular, and optical physics and nanoscience. A distinguished physics professor at Kansas State University and the J. R. Macdonald Laboratory in Manhattan, Kansas his research team investigates the ultrafast dynamics of electrons and molecular fragments in laser-matter and particle-matter interactions, highly-charged-ion physics, electron–atom collisions, and plasmonic nanostructures. He is a Fellow of the American Physical Society and recipient of several awards, including the Senior Research Award of the Alexander von Humboldt Foundation.
Péter István Mészáros is a Hungarian-American theoretical astrophysicist, best known for the Mészáros effect in cosmology and for his work on gamma-ray bursts.
Sabine Schindler is a German astrophysicist whose research has involved both simulations and X-ray observations of galaxy clusters. She is a professor at the University of Innsbruck and rector of UMIT - Private University for Health Sciences, Medical Informatics and Technology, both in Austria.
Irene Tamborra is an Italian particle astrophysicist, specializing in the areas of neutrino astrophysics and cosmology as well as multi-messenger astronomy. She is professor of particle astrophysics at the Niels Bohr Institute, University of Copenhagen.
Maryam Modjaz is a German-American astrophysicist who is a professor and Director of Equity and Inclusion at the New York University. Her research considers the death of massive stars. She was awarded an Alexander von Humboldt Foundation Fellowship in 2018, which she spent at the Max Planck Institute for Astronomy.
Fiorenza Donato is an Italian theoretical astroparticle physicist whose research involves the study of cosmic rays and their use in understanding the nature of dark matter, the possible products of particle collisions involving dark matter, the creation and behavior of antimatter among high-energy cosmic particles, and gamma-ray astronomy. She is a full professor of theoretical physics at the University of Turin.
Paola Andrea Pinilla Ortiz is a Colombian astrophysicist whose research concerns the accretion of interplanetary dust clouds into protoplanetary disks as part of the formation of exoplanets. Educated in Colombia and Germany, she works in England as associate professor in exoplanets at the University College London Department of Space & Climate Physics, affiliated with the university's Mullard Space Science Laboratory.
Karin Lind is a Swedish astronomer whose research involves spectroscopy of stars in order to determine their chemical composition, and the use of this information to understand the origin of heavy elements in supernova explosions and the way radiation and energy moves through stellar atmospheres. Her work has in particular clarified the roles of Big Bang nucleosynthesis and supernovas in producing the quantities of lithium observed in early stars. She is an associate professor in the Department of Astronomy at Stockholm University, and a participant and survey builder in the GALAH collaboration, which uses the Anglo-Australian Telescope's HERMES instrument to map the chemical compositions of stars in the Milky Way.
References
- ↑ "Patricia Schady", Profiles, University of Bath, retrieved 2024-04-09
- 1 2 3 Sofia Kovalevskaya Award winners 2012, Alexander von Humboldt Foundation, retrieved 2024-04-09
- ↑ "Patricia Schady", AstroGen, American Astronomical Society, retrieved 2024-04-09
- ↑ Patricia Schady receives Sofja Kovalevskaja Prize, Max Planck Institute for Extraterrestrial Physics, 22 August 2012, retrieved 2024-04-09
| Authority control databases: Academics |
|---|
