It’s a bird! It’s a plane! It’s a neutrino observatory calibration source!

It’s a bird! It’s a plane! It’s a neutrino observatory calibration source!

Title: Radio emission from airplanes as observed with RNO-G Authors: The RNO-G Collaboration S. Agarwal, J. A. Aguilar, N. Alden, S. Ali, P. Allison, M. Betts, D. Besson, A. Bishop, O. Botner, S. Bouma, S. Buitink, R. Camphyn, J. Chan, S. Chiche, B. A. Clark, A. Coleman, K. Couberly, S. de Kockere, K. D. de Vries, C. Deaconu, P. Giri, C. Glaser, T. Glüsenkamp, H. Gui, A. Hallgren, S. Hallmann, J. C. Hanson, K. Helbing, B. Hendricks, J. Henrichs, N. Heyer, C. Hornhuber, E. Huesca Santiago, K. Hughes, A. Jaitly, T. Karg, A. Karle, J. L. Kelley, J. Kimo, C. Kopper, M. Korntheuer, M. Kowalski, I. Kravchenko, R. Krebs, M. Kugelmeier, R. Lahmann, C.-H. Liu, M. J. Marsee, Z. S. Meyers, K. Mulrey, M. Muzio, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, N. Punsuebsay, L. Pyras, M. Ravn, A. Rifaie, D. Ryckbosch, O. Schlemper, F. Schlüter, O. Scholten, D. Seckel, M. F. H. Seikh, J. Stachurska,  J. Stoffels, S. Toscano, D. Tosi, J. Tutt, D. J. Van Den Broeck, N. van Eijndhoven, A. G. Vieregg, A. Vijai, C. Welling, D. R. Williams, P. Windischhofer, S. Wissel, R. Young, A. Zink First Author’s Institution: Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander-University Erlangen-Nürnberg; Deutsches Elektronen-Synchrotron DESY Status: Published in the Journal of Instrumentation [open access] Neutrinos: Long-Distance Travelers If, in the middle of an intercontinental flight, you’ve ever looked out your window over, say, Greenland and wondered how this trip still isn’t over…just remember that your long-distance travels have nothing on the neutrino’s. This particle only very rarely interacts with other matter, so it can travel far across...
Low, Low, and Lower: A Binary Ultracool Dwarf System is Detected at 340 MHz

Low, Low, and Lower: A Binary Ultracool Dwarf System is Detected at 340 MHz

The lowest mass stars have been well-studied across the mid and high frequency radio bands. However, lower frequencies can reveal larger-scale magnetic structures and may even be the key to the first direct radio detection of an exoplanet. Learn about the first detection of a low-mass ultracool dwarf–one or both stars in a binary system–at the low frequency of 340 MHz!