Detection of Pulses from the Vela Pulsar at Millimeter Wavelengths with Phased ALMA

We report on the first detection of pulsed radio emission from a radio pulsar with the Atacama Large Millimeter/submillimeter Array (ALMA) telescope. The detection was made in the Band-3 frequency range (85-101 GHz) using ALMA in the phased-array mode developed for VLBI observations. A software pipe...

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Veröffentlicht in:	Astrophysical journal. Letters 2019-11, Vol.885 (1), p.L10
Hauptverfasser:	Liu, Kuo, Young, André, Wharton, Robert, Blackburn, Lindy, Cappallo, Roger, Chatterjee, Shami, Cordes, James M., Crew, Geoffrey B., Desvignes, Gregory, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Goddi, Ciriaco, Johnson, Michael D., Johnston, Simon, Karuppusamy, Ramesh, Kramer, Michael, Matthews, Lynn D., Ransom, Scott M., Rezzolla, Luciano, Rottmann, Helge, Tilanus, Remo P. J., Torne, Pablo
Format:	Artikel
Sprache:	eng
Schlagworte:	Arrays Astrophysics Calibration Flux density Frequency ranges Interferometry Millimeter astronomy Physics Polarimetry Polarization Pulsars Radio emission Radio telescopes Supermassive black holes Wavelengths
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