From the Editors
Happy Solstice to our readers! Here's a quick round-up of recent papers relevant to FRBs. Please keep sending in your items of interest, and we hope this newsletter continues to be useful and informative.
Papers of Interest
Observational Results
- A Radio Continuum Study of NGC 2082; Balzan et al., arXiv: 2205.11144
- The Apertif Radio Transient System (ARTS): Design, Commissioning, Data Release, and Detection of the first 5 Fast Radio Bursts; van Leeuwen et al., arXiv: 2205.12362
- First Discoveries and Localisations of Fast Radio Bursts with MeerTRAP: A Real-Time, Commensal MeerKAT Survey; Rajwade et al., arXiv: 2205.14600
- A Burst Storm from the Repeating FRB 20200120E in an M81 Globular Cluster; Nimmo et al., arXiv: 2206.03759
Theory and Modeling
- Searching for Quasi-Periodic Oscillations in Astrophysical Transients using Gaussian Processes; Hubner et al., arXiv: 2205.12716
- Faraday Conversion in Pair-Symmetric Winds of Magnetars and Fast Radio Bursts; Lyutikov, arXiv: 2205.13435
- Precession and Jitter in FRB 180916B; Katz, arXiv: 2205.15385
- Constraints on the Helium Abundance from Fast Radio Bursts; Liang Jing & Jun-Qing Xia, arXiv: 2206.04553
- A Heuristic Account of the Radiation by the Superluminally Moving Current Sheet in the Magnetosphere of a Neutron Star; Ardavan, arXiv: 2206.02729
- Radio Nebulae from Hyper-Accreting X-ray Binaries as Common Envelope Precursors and Persistent Counterparts of Fast Radio Bursts; Sridhar & Metzger, arXiv: 2206.10486
- On the Relation Between Duration and Energy of Non-Repeating Fast Radio Bursts: Census with the CHIME Data; Seong Jin Kim et al., arXiv: 2206.11330
- Thermodynamics of Magnetized Dense Neutron-Rich Matter; Diener, arXiv: 2206.04433
Algorithms and Instrumentation
- Mitigating Radio Frequency Interference in CHIME/FRB Real-Time Intensity Data; Rafiei-Ravandi & Smith, arXiv: 2206.07292
- BURSTT: Bustling Universe Radio Survey Telescope for Taiwan; Hsiu-Hsien Lin et al., arXiv: 2206.08983
- The GMRT High Resolution Southern Sky Survey for Pulsars and Transients -- III: Searching for Long Period Pulsars; Singh et al., arXiv: 2206.00427
Magnetars and other relevant results
- Looking at Luminous Fast Blue Optical Transients through Neutrino Glasses; Guarini, Tamborra & Raffaella Margutti; arXiv: 2205.12282
- Discovery of a Radio Emitting Neutron Star with an Ultra-Long Spin Period of 76 Seconds; Caleb et al., arXiv: 2206.01346; Nature Astronomy DOI: s41550-022-01688-x
- Independent Discovery of a Nulling Pulsar with Unusual Sub-Pulse Drifting Properties with the Murchison Widefield Array; McSweeney et al., arXiv: 2206.00805
- MeerKAT Observations of the Reversing Drifting Subpulses in PSR J1750-3503; Szary et al., arXiv: 2206.02382
- The Discovery of a Rotating Radio Transient J1918-0449 with Intriguing Emission Properties with the Five Hundred Meter Aperture Spherical Radio Telescope; J. L. Chen et al., arXiv: 2206.03091
- Magnetar Engines in Fast Blue Optical Transients and Their Connections with SLSNe, SNe Ic-BL, and lGRBs; Jian-Feng Liu et al., arXiv: 2206.03303
- Tangled magnetic field model of QPOs; Bretz, van Eysden & Link, arXiv: 2206.09544
- Detection of Quasi-Periodic Micro-Structure in Three Millisecond Pulsars with the Large European Array for Pulsars; Liu et al., arXiv: 2206.10045
We also discuss a possible link of micro-structure to the properties of some of the recently discovered fast radio bursts which exhibit a very similar emission morphology.
- A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula; Dong & Hallinan, arXiv: 2206.11911
Upcoming Meetings and Conferences
IAU GA 2022 / FRB2022: The IAU General Assembly in Busan, South Korea is coming soon, with the symposium on Fast Radio Bursts scheduled for 2-4 August 2022.
Relevant Job Listings
-- Research Software Developers for CHIME/FRB and CHIME Slow Pulsar at McGill University. Closing 30 June, 2022. International applicants welcome! McGill Workday Listing 1 & Listing 2.
Do you have an item for future newsletters? Please send these via email to the editors (Emily and Shami) to be included in an upcoming issue.
|