Evidence for inverse Compton scattering in high-redshift Lyman-break galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press 543:1 (2025) 507-517

Authors:

IH Whittam, MJ Jarvis, Eric J Murphy, NJ Adams, RAA Bowler, A Matthews, RG Varadaraj, CL Hale, I Heywood, K Knowles, L Marchetti, N Seymour, F Tabatabaei, AR Taylor, M Vaccari, A Verma

Abstract:

Radio continuum emission provides a unique opportunity to study star formation unbiased by dust obscuration. However, if radio observations are to be used to accurately trace star formation to high redshifts, it is crucial that the physical processes that affect the radio emission from star-forming galaxies are well understood. While inverse Compton (IC) losses from the cosmic microwave background (CMB) are negligible in the local universe, the rapid increase in the strength of the CMB energy density with redshift [] means that this effect becomes increasingly important at . Using a sample of high-redshift () Lyman-break galaxies selected in the rest-frame ultraviolet (UV), we have stacked radio observations from the MIGHTEE survey to estimate their 1.4-GHz flux densities. We find that for a given rest-frame UV magnitude, the 1.4-GHz flux density and luminosity decrease with redshift. We compare these results to the theoretical predicted effect of energy losses due to IC scattering off the CMB, and find that the observed decrease is consistent with this explanation. We discuss other possible causes for the observed decrease in radio flux density with redshift at a given UV magnitude, such as a top-heavy initial mass function at high redshift or an evolution of the dust properties, but suggest that IC scattering is the most compelling explanation.

Hi gas in the rejuvenated radio galaxy PKS 2014–55

Monthly Notices of the Royal Astronomical Society Oxford University Press 543:1 (2025) 285-291

Authors:

Leon K Mtshweni, Kshitij Thorat, Roger P Deane, Bradley S Frank, Filippo M Maccagni, Gyula I Józsa, William D Cotton, Gourab Giri, Sarah V White, Marcellin Atemkeng, Hertzog L Bester, Bernie L Fanaroff, Ian Heywood, Graham Lawrie, Thato E Manamela, Isaac Magolego, Tom Mauch, Nadeem Oozeer, Oleg Smirnov, Masacheba S Kupa

Abstract:

We present new high-spectral-resolution MeerKAT observations of absorption against the central region of the restarted, giant, X-shaped radio galaxy PKS2014–55, which exhibits morphological evidence of three distinct cycles of activity. We report a wide component (FWHM 38 7 km ) redshifted to 96 50 km , a deep-narrow detection (FWHM 19 6 km ) which is redshifted to 160 40 km, and a shallow component (FWHM 22 6 km) redshifted to 240 40 km . One of the three components exceeds the typical rotational velocity of 100 km , suggesting complex kinematics of the inflowing gas. These observations support the correlation between the occurrence of absorption and the rejuvenation of radio activity.

Erratum: “A Novel Technosignature Search in the Breakthrough Listen Green Bank Telescope Archive” (2025, AJ, 169, 222)

The Astronomical Journal American Astronomical Society 170:3 (2025) 194

Authors:

Caleb Painter, Steve Croft, Matthew Lebofsky, Alex Andersson, Carmen Choza, Vishal Gajjar, Danny Price, Andrew PV Siemion

Silent Speech Recognition with Wearable Magnetometers

bioRxiv preprint 2025.08:04.668236 (2025)

Authors:

Debadatta Dash, Evan Kittle, Isabel Gerrard, Richard Csaky, Gabriel Gonzalez, David Taylor, Juan Pablo Llinas, Dominic Labanowski, Nishita Deka, Richy Yun

Abstract:

Next-generation human-computer interaction (HCI) is moving towards more seamless, intuitive,
and personal modes of communication, redefining how we interact with technology and one another.
Within this landscape, silent speech recognition (SSR) offers a powerful new interaction paradigm,
enabling hands-free, private interaction while supporting individuals with speech impairments and
enabling communication in noisy or sensitive environments. Recent advances in miniaturized sensors and artificial intelligence (AI) have accelerated the development of more sophisticated wearable
SSR systems, driven by growing demand for effortless and accessible communication. Although
electrophysiological (ExG) modalities, particularly electromyography (EMG), have dominated early
efforts in developing wearable SSR, critical challenges remain. Limited generalizability across
users, sensor-skin interface issues, and difficulties with the comfort of use are all current roadblocks
to reliable, high-fidelity signals in a wearable form factor. We propose that magnetometers offer
a promising alternative to ExG and have the potential to unlock more robust, generalizable, and
user-friendly SSR systems. We demonstrate that magnetometers embedded in a headphone form
factor achieve a per-user SSR accuracy of 86%, significantly outperforming previously reported
state-of-the-art wearable headphones combining ExG and inertial measurement units (IMUs). In
addition, we show that wearable magnetometry enables generalization across individuals for SSR.
Extending beyond headphones, we also introduce a necklace form factor with magnetometers that
is capable of decoding both silent and overt speech in ambient conditions, further showcasing the
versatility of magnetometers across different wearable designs in real-world conditions.

Commensal Transient Searches with MeerKAT in Gamma-Ray Burst and Supernova Fields

The Astrophysical Journal American Astronomical Society 988:2 (2025) 227

Authors:

SI Chastain, AJ van der Horst, A Horesh, A Rowlinson, A Andersson, R Diretse, M Vaccari, RP Fender, PA Woudt

Abstract:

The sensitivity and field of view of the MeerKAT radio telescope provide excellent opportunities for commensal transient searches. We carry out a commensal transient search in supernova and short gamma-ray burst fields using methodologies established by S. I. Chastain et al. We search for transients in MeerKAT L-band images with integration times of 30 minutes, finding 13 variable sources. We compare these sources to the VLASS and RACS survey data, and examine possible explanations for the variability. Additionally, for one of these sources we examine archival Chandra ACIS data. We find that 12 of these sources are consistent with variability due to interstellar scintillation. The remaining source could possibly have some intrinsic variability. We also split the MeerKAT L band into upper and lower halves, and search for transients in images with an integration time of 8 s. We find a source with a duration of 8–16 s that is highly polarized at the lowest frequencies. This source is spatially coincident with a star detected by the Transiting Exoplanet Survey Satellite. We conclude that this source may be consistent with a stellar flare. Finally, we calculate accurate upper and lower limits on the transient rate using transient simulations.