FRB Newsletter Volume 05, Issue 11 — November 2024 Total FRB count: 802 (2 new) Repeaters: 56 Host galaxies: 93 (1 new) TNS FRB Search From the Editors Now that the excitement of FRB2024 is behind us, it is time to reset your countdown clock for FRB2025 in Montreal. We will pass along a link to the talk recordings from FRB2024, and more details of FRB2025, when those are available. Meanwhile, here is a round up of the latest from ArXiv - enjoy! Papers of Interest Reviews Cosmology with Fast Radio Bursts; Glowacki & Lee, arXiv: 2410.24072 Observational Results Investigating the sightline of a highly scattered FRB through a filamentary structure in the local Universe; Shin et al., arXiv: 2410.07307 The Massive and Quiescent Elliptical Host Galaxy of the Repeating Fast Radio Burst FRB20240209A; Eftekhari et al., arXiv: 2410.23336 A repeating fast radio burst source in the outskirts of a quiescent galaxy; Shah et al., arXiv: 2410.23374 Separating repeating fast radio bursts using the minimum spanning tree as an unsupervised methodology; Garcia et al., arXiv: 2411.02216 Constraining the Hubble constant with scattering in host galaxies of fast radio bursts; Yang et al., arXiv: 2411.02249 Morphology of 32 Repeating Fast Radio Burst Sources at Microsecond Time Scales with CHIME/FRB; Curtin et al., arXiv: 2411.02870 Flaring gamma-ray emission coincident with a hyperactive fast radio burst source; Xing et al., arXiv: 2411.06996 - (but see discussion of ATel 16602 in the April 2024 Newsletter) Polarization properties of 28 repeating fast radio burst sources with CHIME/FRB; Ng et al., arXiv: 2411.09045 Reinvestigation of Fast Radio Bursts Host Galaxy and Event Rate Density; Ma et al., arXiv: 2411.09203 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications; Qiang et al., arXiv: 2411.13973 Unsupervised Machine Learning for Classifying CHIME Fast Radio Bursts and Investigating Empirical Relations; Qiang et al., arXiv: 2411.14040 Unusual intra-burst variations of polarization states in FRB 20210912A and FRB 20230708A : Effects of plasma birefringence?; Bera et al., arXiv: 2411.14784 Structure Functions of Rotation Measures Revealing the Origin of Fast Radio Bursts; Li et al., arXiv: 2411.15546 Long term monitoring of FRB 20121102 with the Nancay Radio Telescope and multi-wavelength campaigns including INTEGRAL; Gouiffes et al., arXiv: 2411.16419 Theory and Modeling The role of magnetic and rotation axis alignment in driving fast radio burst phenomenology; Beniamini & Kumar, arXiv: 2410.19043 "We propose a model that can describe the entire range of FRBs, from non-repeating to highly prolific repeaters." Lensing point-spread function of coherent astrophysical sources and non-trivial wave effects; Shi, arXiv: 2410.20049 A parametric study of population inversions in relativistic plasmas through nonresonant interactions with Alfven waves and their applications to Fast Radio Bursts; Long & Pe'er, arXiv: 2410.21022 Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe; Huang et al., arXiv: 2410.22098 Induced Compton scattering in magnetized electron and positron pair plasma; Nishiura et al., arXiv: 2411.00936 Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization; Ziegler et al., arXiv: 2411.02699 Combining strongly lensed and unlensed fast radio bursts: to be a more precise late-universe probe; Zhang et al., arXiv: 2411.03126 Fast Radio Bursts and Interstellar Objects; Pham et al., arXiv: 2411.09135 Algorithms, Instrumentation, and Data Access frb-voe: A Real-time Virtual Observatory Event Alert Service for Fast Radio Bursts; Abbott et al., arXiv: 2410.22468 Accelerating FRB Search: Dataset and Methods; Guo et al., arXiv: 2411.02859 The Wide Field Monitor (WFM) of the China-Europe eXTP (enhanced X-ray Timing and Polarimetry) mission; Hernanz et al., arXiv: 2411.03050 Self-supervised learning for radio-astronomy source classification: a benchmark; Cecconello et al., arXiv: 2411.14078 A 400Gbit Ethernet core enabling High Data Rate Streaming from FPGAs to Servers and GPUs in Radio Astronomy; Liu et al., arXiv: 2411.15630 Magnetars and other relevant results Fast Transients from Magnetic Disks Around Non-Spinning Collapsar Black Holes; Bopp & Gottlieb; arXiv: 2410.22401 INTEGRAL search for magnetar giant flares from the Virgo Cluster and in nearby galaxies with high star formation rate; Pacholski et al., arXiv: 2411.03235 Origin of the twice 90 degree rotations of the polarization angle in GRB 170114A and GRB 160821A; Wang et al., arXiv: 2411.09070 A 44-minute periodic radio transient in a supernova remnant; Li et al., arXiv: 2411.15739 Searching radio signals from two magnetars and a high-magnetic field pulsar and the serendipitous discovery of a new radio pulsar PSR J1935+2200; Xie et al., arXiv: 2411.15960 The FAST Galactic Plane Pulsar Snapshot survey: VI. The discovery of 473 new pulsars; Han et al., arXiv: 2411.15961 - (includes 2 new FRBs) Detection of X-ray Emission from a Bright Long-Period Radio Transient; Wang et al., arXiv: 2411.16606 - (note this is an independent discovery of the same source presented in the Li et al. listing above) Recent job listings Job advertisements that may be relevant to the readers of this Newsletter: Postdoctoral research position to work on FRBs with Joeri van Leeuwen at ASTRON. Deadline December 2 2024. Two Postdoctoral research positions to work on time-domain radio astronomy with the pulsar/FRB group at Guangzhou University. Deadline December 31 2024. Do you have an item for future newsletters? Please send these via email to the editors (Shami and Kenzie) to be included in an upcoming issue. FRB Newsletter: 2019—2024, produced by Shami Chatterjee and Kenzie Nimmo. We acknowledge support from the Cornell library, the National Science Foundation (NSF), and the MIT Kavli Institute. You are receiving this email because you subscribed to this newsletter. You can unsubscribe here. If you were forwarded this email and would like to subscribe you can subscribe here. We welcome your tips and suggestions by email. Archive of past newsletters with citable DOIs can be found here.