alphaFeedback
astro-ph.IMastro-ph.COastro-ph.HEastro-ph.GAphysics.space-phastro-ph.EPhep-exastro-ph.SRhep-phphysics.geo-ph

On Valency

published · living versions
W_hfxes35b·v1 · currentpublished
LOFAR: The LOw-Frequency ARray
with M. P. van Haarlem, M. W. Wise, A. W. Gunst, G. Heald +195
1 version

Preprints & journals

79 papers in the corpus · 2004–2026
Assessing ionospheric effects on image quality in the LOFAR Decametre Sky Survey2609.17382v1 · Cristina-Maria Cordun, Harish K. Vedantham, Maaijke Mevius2026 · 0 citationsProceedings of SPIE, Vol. 14153, 3101297 (2026)
Exploring the Galactic plasma with pulsars in the SKA Era2607.06096v2 · Caterina Tiburzi, M. T. Lam, D. J. Reardon et al.2026 · 0 citationsarXiv
The LOFAR Two-metre Sky Survey: VII. Third Data Release2602.15949v1 · T. W. Shimwell, M. J. Hardcastle, C. Tasse et al.2026 · 20 citationsarXiv
Exploring Galactic plasma with pulsars in the SKA era2512.16158v1 · C. Tiburzi, M. T. Lam, D. J. Reardon et al.2025 · 1 citationarXiv
An improved algorithm for separating clock delays from ionospheric effects in radio astronomy2510.01371v1 · C.M. Cordun, M.A. Brentjens, H.K. Vedantham et al.2025 · 1 citationA&A 2025 701
Mitigating incoherent excess variance in high-redshift 21 cm observations with multi-output cross-Gaussian process regression2508.08235v2 · S. Munshi, L. V. E. Koopmans, F. G. Mertens et al.2025 · 0 citationsA&A 704, A205 (2025)
Improved upper limits on the 21-cm signal power spectrum at z=17.0z=17.0 and z=20.3z=20.3 from an optimal field observed with NenuFAR2507.10533v2 · S. Munshi, F. G. Mertens, J. K. Chege et al.2025 · 13 citationsMon Not R Astron Soc (2025) 2785-2807
First upper limits on the 21-cm signal power spectrum of neutral hydrogen at z=9.16z=9.16 from the LOFAR 3C196 field2504.18534v1 · E. Ceccotti, A. R. Offringa, F. G. Mertens et al.2025 · 9 citationsMon Not R Astron Soc (2025) 1255-1283
The impact of diffuse Galactic emission on direction-independent gain calibration in high-redshift 21 cm observations2504.03554v2 · C. Hofer, L.V.E. Koopmans, S.A. Brackenhoff et al.2025 · 3 citationsA&A 704, A117 (2025)
Robust direction-dependent gain-calibration of beam-modelling errors far from the target field2504.02483v2 · S.A. Brackenhoff, A.R. Offringa, M. Mevius et al.2025 · 6 citationsMon Not R Astron Soc (2025) 3993-4010
Near-field imaging of local interference in radio interferometric data: Impact on the redshifted 21 cm power spectrum2503.21728v2 · S. Munshi, F. G. Mertens, L. V. E. Koopmans et al.2025 · 9 citationsA&A 697, A203 (2025)
Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment2503.11740v1 · A. Bonaldi, P. Hartley, R. Braun et al.2025 · 10 citationsarXiv
Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.12503.05576v2 · F. G. Mertens, M. Mevius, L. V. E. Koopmans et al.2025 · 38 citationsA&A 698, A186 (2025)
Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum2502.18459v1 · E. Ceccotti, A. R. Offringa, L. V. E. Koopmans et al.2025 · 9 citationsA&A 696, A56 (2025)
Ionospheric contributions to the excess power in high-redshift 21-cm power-spectrum observations with LOFAR2407.20220v1 · S.A. Brackenhoff, M. Mevius, L.V.E. Koopmans et al.2024 · 10 citationsarXiv
The impact of lossy data compression on the power spectrum of the high redshift 21-cm signal with LOFAR2407.11557v1 · J. K. Chege, L.V.E. Koopmans, A. R. Offringa et al.2024 · 4 citationsA&A 692, A211 (2024)
Beyond the horizon: Quantifying the full sky foreground wedge in the cylindrical power spectrum2407.10686v2 · S. Munshi, F. G. Mertens, L. V. E. Koopmans et al.2024 · 16 citationsA&A 693, A276 (2025)
LOFAR observations of asymmetric quasi-periodic scintillations in the mid-latitude ionosphere2401.16932v1 · Gareth Dorrian, David Themens, Toralf Renkwitz et al.2024 · 0 citationsarXiv
A candidate coherent radio flash following a neutron star merger2312.04237v3 · A. Rowlinson, I. de Ruiter, R.L.C. Starling et al.2023 · 14 citationsarXiv
First upper limits on the 21 cm signal power spectrum from cosmic dawn from one night of observations with NenuFAR2311.05364v2 · S. Munshi, F. G. Mertens, L. V. E. Koopmans et al.2023 · 65 citationsA&A 681, A62 (2024)
LOFAR Deep Fields: Probing faint Galactic polarised emission in ELAIS-N12303.13152v1 · Iva Snidari'c, Vibor Jeli'c, Maaijke Mevius et al.2023 · 9 citationsA&A 674, A119 (2023)
The Scintillating Tail of Comet C/2020 F3 (Neowise)2210.02139v1 · R.A. Fallows, B. Forte, M. Mevius et al.2022 · 1 citationA&A 667, A57 (2022)
Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21-cm signal power spectrum2209.07854v2 · H. Gan, F. G. Mertens, L. V. E. Koopmans et al.2022 · 24 citationsA&A 669, A20 (2023)
The LOFAR Two-metre Sky Survey -- V. Second data release2202.11733v1 · T. W. Shimwell, M. J. Hardcastle, C. Tasse et al.2022 · 493 citationsarXiv
Degree-Scale Galactic Radio Emission at 122 MHz around the North Celestial Pole with LOFAR-AARTFAAC2112.00721v3 · B. K. Gehlot, L. V. E. Koopmans, A. R. Offringa et al.2021 · 12 citationsA&A 662, A97 (2022)
The AARTFAAC Cosmic Explorer: observations of the 21-cm power spectrum in the EDGES absorption trough2010.02269v1 · B. K. Gehlot, F. G. Mertens, L. V. E. Koopmans et al.2020 · 43 citationsarXiv
A LOFAR Observation of Ionospheric Scintillation from Two Simultaneous Travelling Ionospheric Disturbances2003.04013v1 · Richard A. Fallows, Biagio Forte, Ivan Astin et al.2020 · 37 citationsarXiv
Cassiopeia A, Cygnus A, Taurus A, and Virgo A at ultra-low radio frequencies2002.10431v1 · F. de Gasperin, J. Vink, J.P. McKean et al.2020 · 47 citationsarXiv
The LOFAR Two-metre Sky Survey - II. First data release1811.07926v1 · T. W. Shimwell, C. Tasse, M. J. Hardcastle et al.2018 · 601 citationsarXiv
Systematic effects in LOFAR data: A unified calibration strategy1811.07954v1 · F. de Gasperin, T. J. Dijkema, A. Drabent et al.2018 · 216 citationsarXiv
The effect of the ionosphere on ultra-low frequency radio-interferometric observations1804.07947v1 · F. de Gasperin, M. Mevius, D.A. Rafferty et al.2018 · 74 citationsA&A 615, A179 (2018)
Wide-field LOFAR-LBA power-spectra analyses: Impact of calibration, polarization leakage and ionosphere1709.07727v2 · B. K. Gehlot, L. V. E. Koopmans, A. G. de Bruyn et al.2017 · 34 citationsarXiv
Overview of lunar detection of ultra-high energy particles and new plans for the SKA1704.05336v1 · Clancy W. James, Jaime Alvarez-Muniz, Justin D. Bray et al.2017 · 12 citationsEPJ Web Conf., Volume 135, 04001 (2017)
Upper limits on the 21-cm Epoch of Reionization power spectrum from one night with LOFAR1702.08679v1 · A.H. Patil, S. Yatawatta, L.V.E. Koopmans et al.2017 · 289 citationsarXiv
The lunar Askaryan technique with the Square Kilometre Array1608.02408v1 · Clancy W. James, Jaime Alvarez-Muniz, Justin D. Bray et al.2016 · 3 citationsPOS(ICRC2015)291
Corrigendum: A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations.27437581 · Buitink, S, Corstanje, A, Falcke, H et al.2017 · 3 citationsNature. 2016;537(7621):572
Probing Ionospheric Structures using the LOFAR radio telescope1606.04683v1 · M. Mevius, S. van der Tol, V. N. Pandey et al.2016 · 133 citationsRadio Sci. 51 (2016) 927-941
Systematic biases in low frequency radio interferometric data due to calibration: the LOFAR EoR case1605.07619v1 · Ajinkya H. Patil, Sarod Yatawatta, Saleem Zaroubi et al.2016 · 114 citationsarXiv
A large light-mass component of cosmic rays at 10(17)-10(17.5) electronvolts from radio observations.26935696 · Buitink, S, Corstanje, A, Falcke, H et al.2016 · 157 citationsNature. 2016;531(7592):70-3
LOFAR facet calibration1601.05422v1 · R. J. van Weeren, W. L. Williams, M. J. Hardcastle et al.2016 · 278 citationsarXiv
Career total: at least 246 works. 79 are in this corpus.Showing the 50 most recent.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.