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Related papers: RFI Flagging Implications for Short-Duration Trans…

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We present a project to implement a national common strategy for the mitigation of the steadily deteriorating Radio Frequency Interference (RFI) situation at the Italian radio telescopes. The project involves the Medicina, Noto, and…

The data taken by the advanced LIGO and Virgo gravitational-wave detectors contains short duration noise transients that limit the significance of astrophysical detections and reduce the duty cycle of the instruments. As the advanced…

Instrumentation and Methods for Astrophysics · Physics 2017-01-25 Jade Powell , Alejandro Torres-Forné , Ryan Lynch , Daniele Trifirò , Elena Cuoco , Marco Cavaglià , Ik Siong Heng , José A. Font

Extensive radio frequency interference (RFI) monitoring is essential in the site selection process before constructing radio astronomy observatories, followed by mitigation strategies to minimize its adverse effects. Malaysia has an…

We introduce a new pipeline for analyzing and mitigating radio frequency interference (RFI), which we call Sky-Subtracted Incoherent Noise Spectra (SSINS). SSINS is designed to identify and remove faint RFI below the single baseline thermal…

Instrumentation and Methods for Astrophysics · Physics 2019-10-10 Michael J. Wilensky , Miguel F. Morales , Bryna J. Hazelton , Nichole Barry , Ruby Byrne , Sumit Roy

In Earth remote sensing, spatial-frequency domain visibility samples are inversely transformed into spatial-domain brightness temperature (BT) images through the signal processing pipeline of synthetic aperture interferometric radiometers…

Signal Processing · Electrical Eng. & Systems 2026-04-03 Yuankai Luo , Han Zhou , Jinlong Hao , Dong Zhu , Fei Hu

With the ongoing growth in radio communications, there is an increased contamination of radio astronomical source data, which hinders the study of celestial radio sources. In many cases, fast mitigation of strong radio frequency…

Signal Processing · Electrical Eng. & Systems 2024-03-08 Zaid Bin Tariq , Teviet Creighton , Louis P. Dartez , Naofal Al-Dhahir , Murat Torlak

Phased Array Feed (PAF) receivers are at the forefront of modern day radio astronomy. PAFs are currently being developed for spectral line and radio continuum surveys and to search for pulsars and fast radio bursts. Here, we present results…

High Energy Astrophysical Phenomena · Physics 2019-08-21 K. M. Rajwade , D. Agarwal , D. R. Lorimer , N. M. Pingel , D. J. Pisano , M. Ruzindana , B. Jeffs , K. F. Warnick , D. A. Roshi , M. A. McLaughlin

We report on the methodology and first results from the Deep Lens Survey transient search. We utilize image subtraction on survey data to yield all sources of optical variability down to 24th magnitude. Images are analyzed immediately after…

We discuss a possible generation of radio bursts preceding final stages of binary neutron star mergings which can be accompanied by short gamma-ray bursts. Detection of such bursts appear to be advantageous in the low-frequency radio band…

High Energy Astrophysical Phenomena · Physics 2010-04-29 M. S. Pshirkov , K. A. Postnov

A few members of the recently discovered class of long-period transients have been identified as binaries with white-dwarf primaries. In most cases, however, electromagnetic data are inconclusive, and isolated magnetars or compact binaries…

High Energy Astrophysical Phenomena · Physics 2025-09-09 Arthur G. Suvorov , Clara Dehman , José A. Pons

Astrophysical transients have been observed for millennia and have shaped our most basic assumptions about the Universe. In the last century, systematic searches have grown from detecting handfuls of transients per year to over 7000 in 2018…

The ongoing optical time-domain astronomy surveys are routinely reporting fifty transient candidates per night. Here, I investigate the demographics of astronomical transients and supernova classifications reported to the Transient Name…

Instrumentation and Methods for Astrophysics · Physics 2020-04-14 S. R. Kulkarni

The Square Kilometre Array (SKA) is expected to start science operations in 2030 and by that time there could be up to 10$^5$ artificial satellites in Earth's orbit, comprising an increase of an order of magnitude compared to 2024. Most of…

Instrumentation and Methods for Astrophysics · Physics 2026-04-27 Nicolas Cerardi , Emma Tolley , Federico di Vruno

We introduce SigNova, a new semi-supervised framework for detecting anomalies in streamed data. While our initial examples focus on detecting radio-frequency interference (RFI) in digitized signals within the field of radio astronomy, it is…

Instrumentation and Methods for Astrophysics · Physics 2024-03-13 Paola Arrubarrena , Maud Lemercier , Bojan Nikolic , Terry Lyons , Thomas Cass

Increasing levels of Radio Frequency Interference (RFI) are a problem for research in radio astronomy. Various techniques to suppress RFI and extract astronomical signals from data affected by interference are being tried out. However,…

Astrophysics · Physics 2007-05-23 K. Jeeva Priya , D. Anish Roshi

Passive space-borne radiometers operating in the 1400-1427 MHz protected frequency band face radio frequency interference (RFI) from terrestrial sources. With the growth of wireless devices and the appearance of new technologies, the…

Machine Learning · Computer Science 2023-04-27 Ali Owfi , Fatemeh Afghah

Searches for gravitational waves (GWs) traditionally focus on persistent sources (e.g., pulsars or the stochastic background) or on transients sources (e.g., compact binary inspirals or core-collapse supernovae), which last for timescales…

There are several unexplored regions of the short-duration radio transient phase space. One such unexplored region is the luminosity gap between giant pulses (from pulsars) and cosmologically located fast radio bursts (FRBs). The Survey for…

High Energy Astrophysical Phenomena · Physics 2020-02-05 Christopher D. Bochenek , Daniel L. McKenna , Konstantin V. Belov , Jonathon Kocz , Shri R. Kulkarni , James Lamb , Vikram Ravi , David Woody

This paper presents an analysis of the transient behavior of the Advanced LIGO suspensions used to seismically isolate the optics. We have characterized the transients in the longitudinal motion of the quadruple suspensions during Advanced…

Instrumentation and Methods for Astrophysics · Physics 2018-01-17 M. Walker , T. D. Abbott , S. M. Aston , G. González , D. M. Macleod , J. McIver , B. P. Abbott , R. Abbott , C. Adams , R. X. Adhikari , S. B. Anderson , A. Ananyeva , S. Appert , K. Arai , S. W. Ballmer , D. Barker , B. Barr , L. Barsotti , J. Bartlett , I. Bartos , J. C. Batch , A. S. Bell , J. Betzwieser , G. Billingsley , J. Birch , S. Biscans , C. Biwer , C. D. Blair , R. Bork , A. F. Brooks , G. Ciani , F. Clara , S. T. Countryman , M. J. Cowart , D. C. Coyne , A. Cumming , L. Cunningham , K. Danzmann , C. F. Da Silva Costa , E. J. Daw , D. DeBra , R. T. DeRosa , R. DeSalvo , K. L. Dooley , S. Doravari , J. C. Driggers , S. E. Dwyer , A. Effler , T. Etzel , M. Evans , T. M. Evans , M. Factourovich , H. Fair , A. Fernández Galiana , R. P. Fisher , P. Fritschel , V. V. Frolov , P. Fulda , M. Fyffe , J. A. Giaime , K. D. Giardina , E. Goetz , R. Goetz , S. Gras , C. Gray , H. Grote , K. E. Gushwa , E. K. Gustafson , R. Gustafson , E. D. Hall , G. Hammond , J. Hanks , J. Hanson , T. Hardwick , G. M. Harry , M. C. Heintze , A. W. Heptonstall , J. Hough , K. Izumi , R. Jones , S. Kandhasamy , S. Karki , M. Kasprzack , S. Kaufer , K. Kawabe , N. Kijbunchoo , E. J. King , P. J. King , J. S. Kissel , W. Z. Korth , G. Kuehn , M. Landry , B. Lantz , N. A. Lockerbie , M. Lormand , A. P. Lundgren , M. MacInnis , S. Márka , Z. Márka , A. S. Markosyan , E. Maros , I. W. Martin , D. V. Martynov , K. Mason , T. J. Massinger , F. Matichard , N. Mavalvala , R. McCarthy , D. E. McClelland , S. McCormick , G. McIntyre , G. Mendell , E. L. Merilh , P. M. Meyers , J. Miller , R. Mittleman , G. Moreno , G. Mueller , A. Mullavey , J. Munch , L. K. Nuttall , J. Oberling , M. Oliver , P. Oppermann , Richard J. Oram , B. O'Reilly , D. J. Ottaway , H. Overmier , J. R. Palamos , H. R. Paris , W. Parker , A. Pele , S. Penn , M. Phelps , V. Pierro , I. Pinto , M. Principe , L. G. Prokhorov , O. Puncken , V. Quetschke , E. A. Quintero , F. J. Raab , H. Radkins , P. Raffai , S. Reid , D. H. Reitze , N. A. Robertson , J. G. Rollins , V. J. Roma , J. H. Romie , S. Rowan , K. Ryan , T. Sadecki , E. J. Sanchez , V. Sandberg , R. L. Savage , R. M. S. Schofield , D. Sellers , D. A. Shaddock , T. J. Share , B. Shapiro , P. Shawhan , D. H. Shoemaker , D. Sigg , B. J. J. Slagmolen , B. Smith , J. R. Smith , B. Sorazu , A. Staley , K. A. Strain , D. B. Tanner , R. Taylor , M. Thomas , P. Thomas , K. A. Thorne , E. Thrane , C. I. Torrie , G. Traylor , D. Tuyenbayev , G. Vajente , G. Valdes , A. A. van Veggel , A. Vecchio , P. J. Veitch , K. Venkateswara , T. Vo , C. Vorvick , R. L. Ward , J. Warner , B. Weaver , R. Weiss , P. Weßels , B. Willke , C. C. Wipf , J. Worden , G. Wu , H. Yamamoto , C. C. Yancey , Hang Yu , Haocun Yu , L. Zhang , M. E. Zucker , J. Zweizig