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Resolving the Decades-long Transient FIRST J141918.9+394036: An Orphan Long Gamma-Ray Burst or a Young Magnetar Nebula?

  • Authors: B. Marcote, K. Nimmo, O. S. Salafia, Z. Paragi, J. W. T. Hessels, E. Petroff, and R. Karuppusamy

2019 The Astrophysical Journal Letters 876 L14.

  • Provider: AAS Journals

Caption: Figure 1.

Obtained visibility data (amplitudes and phases) for the phase calibrator source, J1419+3821, after the original calibration (top) and in the alternate calibration where the gain calibration of the Tianma station was calibrated using a source model from only the stations with a robust amplitude calibration (bottom). See Section 2 for details. Red dots represent data from the baselines including the Tianma station. Blue lines represent the source model in each case.

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