PDF-Published in "Galactic and Extragalactic Radio Astronomy", 1988, 2nd e

INTRODUCTION Optical Counterparts Radio Source Properties Radio Spectra Energy Considerations LOWLUMINOSITY SOURCES Spiral Seyfert and Irregular Galaxies Elliptical Galaxies COMPACT SOURCES SelfAb. Working Group. Report to C 40. IAU General . Asssembly. August 6, 2015. Honolulu, HI. Ken Kellermann. NRAO. Outline. Goals of the HRA WG . 2012-2015 . Triennial Report. Deceased . radio astronomers. Conferences. Al Wootten, ALMA/NA Project Scientist. Cometary Radio Astronomy. The push to Early Science…. ALMA is pushing to issue a Call for Early Science Proposals around the end of this year. This target is a key driver for the entire project at the moment. The Golden Anniversary of the 1960’s:. The Golden Years of Radio Astronomy. HRA - IAU GA Hawaii. 5. Aug 2015. Ron . Ekers. CSIRO. Australia. Overview. The discovery process. Specialized . . general purpose. a prospect from galaxy evolution. Cosmic Microwave Background Radiation and Its Foreground Interstellar Components, Tokyo. , . 17. th. February, 2010. Tsutomu T. TAKEUCHI. Institute for Advanced Research, Nagoya University, Japan. A CUDA Approach. Gary . Resnick. Scott . Badenhorst. Department of Computer Science. University of Cape Town. 17 March, 2010. Introduction. Approach. Plan. Outcomes. Overview. Radio Astronomy. Ken Tapping. Example Problems. 1 559-1 610 . MHz: . AERONAUTICAL . RADIONAVIGATION. RADIONAVIGATION-SATELLITE (space-to-Earth) (space-to-space. ). 1 610-1 . 610.6 MHz:. MOBILE-SATELLITE (. Earth-to-space) . Recommendations and Reports. Masatoshi . Ohishi. (NAOJ). Part of this . ppt. file was originally prepared by Prof. A. R. Thompson . 2010/06/01. IUCAF SS 2010. Recommendations. The ITU-R Recommendations provide a body of technical, operational and regulatory / procedural . Aka why you can detect any astronomical signals at all. Dr. Karen O’Neil. Green Bank Site Director. Frequency Management. Does it really matter?. Frequency Management. Does it really matter?. GBT observations with . Tomas Gergely. Glen Langston. National Academy of Sciences. Committee on Radio Frequencies. May 29, 2014. Spectrum Management Challenges 2014 - 2015. Spectrum protections and coordination for the new generation of broadband radio astronomy systems. Extragalactic radio . s. ources and their importance for astronomy. Leiden 10-13 June 2013. Ron Ekers. CSIRO, . Australia. George Miley. The largest, the furthest, the most powerful, and to some of us the most fascinating objects known in the Universe are to be found among the radio sources associated with some elliptical galaxies and QSO’s. In recent years it has become apparent that they are also objects of considerable beauty.. A New Detection of Extragalactic AME Eric J. Murphy Radio-to-FIR Spectrum of a Galaxy ~ν -0.8 ~ν -0.1 1.4 GHz 33 GHz ngVLA M51 Dumas et al. 2010 20 cm/1.4 GHz 3.6 cm/8.3GHz H α AME over the last 20 years Tasso Tzioumis, May 2020. Spectrum Management in Radio Astronomy. Why have I been going to Geneva so often?. 1.13 . radio astronomy. :.   . Astronomy based on the reception of. . radio waves. of cosmic origin.. Ken Tapping. Example Problems. 1 559-1 610 . MHz: . AERONAUTICAL . RADIONAVIGATION. RADIONAVIGATION-SATELLITE (space-to-Earth) (space-to-space. ). 1 610-1 . 610.6 MHz:. MOBILE-SATELLITE (. Earth-to-space) . Rachel Osten (. STScI. , JHU). Also . thanksk. to Gregg . Hallinan (. CalTech. ), Laura . Chomiuk. (MSU), . Shami. Chatterjee (Cornell), Joe Lazio (JPL), Tom . Maccarone. (TTU). Outline. Fundamental role of radio observations in transient follow-up; recent JVLA results, motivation for future Brave New Transient World.