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We report on the first detection of pulsed radio emission from a radio pulsarwith the ALMA telescope. The detection was made in the Band-3 frequency range(85-101 GHz) using ALMA in the phased-array mode developed for VLBIobservations. A software pipeline has been implemented to enable a regularpulsar observing mode in the future. We describe the pipeline and demonstratethe capability of ALMA to perform pulsar timing and searching. We also measurethe flux density and polarization properties of the Vela pulsar (PSRJ0835$-$4510) at mm-wavelengths, providing the first polarimetric study of anyordinary pulsar at frequencies above 32 GHz. Finally, we discuss the lessonslearned from the Vela observations for future pulsar studies with ALMA,particularly for searches near the supermassive black hole in the GalacticCenter, and the potential of using pulsars for polarization calibration ofALMA.

Detection of pulses from the Vela pulsar at millimeter wavelengths with phased ALMA