Mertens, F, G
6075  Ergebnisse:
Personensuche X
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1

Ionospheric contributions to the excess power in high-redsh..:

Brackenhoff, S A ; Mevius, M ; Koopmans, L V E...
Monthly Notices of the Royal Astronomical Society.  533 (2024)  1 - p. 632-656 , 2024
 
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2

A novel radio imaging method for physical spectral index mo..:

Ceccotti, E ; Offringa, A R ; Koopmans, L V E...
Monthly Notices of the Royal Astronomical Society.  525 (2023)  3 - p. 3946-3962 , 2023
 
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3

Large-scale 21 cm signal predictions at cosmic dawn with ca..:

Gillet, N J F ; Aubert, D ; Mertens, F G.
Monthly Notices of the Royal Astronomical Society.  507 (2021)  3 - p. 3179-3186 , 2021
 
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4

Improved upper limits on the 21 cm signal power spectrum of..:

Silva, M B ; Schaye, J ; Mondal, R...
Monthly Notices of the Royal Astronomical Society.  493 (2020)  2 - p. 1662-1685 , 2020
 
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5

Comparing foreground removal techniques for recovery of the..:

Hothi, Ian ; Chapman, Emma ; Pritchard, Jonathan R...
Monthly Notices of the Royal Astronomical Society.  500 (2020)  2 - p. 2264-2277 , 2020
 
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6

Constraining the intergalactic medium at z ≈ 9.1 using LOFA..:

Yatawatta, S ; Pandey, V N ; Offringa, A R...
Monthly Notices of the Royal Astronomical Society.  493 (2020)  4 - p. 4728-4747 , 2020
 
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7

The AARTFAAC Cosmic Explorer: observations of the 21-cm pow..:

Gehlot, B K ; Mertens, F G ; Koopmans, L V E...
Monthly Notices of the Royal Astronomical Society.  499 (2020)  3 - p. 4158-4173 , 2020
 
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8

Tight constraints on the excess radio background at z = 9.1..:

Mondal, R ; Fialkov, A ; Fling, C...
Monthly Notices of the Royal Astronomical Society.  498 (2020)  3 - p. 4178-4191 , 2020
 
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9

The first power spectrum limit on the 21-cm signal of neutr..:

Gehlot, B K ; Mertens, F G ; Koopmans, L V E...
Monthly Notices of the Royal Astronomical Society.  488 (2019)  3 - p. 4271-4287 , 2019
 
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11

Deconvolving the wedge: maximum-likelihood power spectra vi..:

Ghosh, A ; Mertens, F G ; Koopmans, L V E
Monthly Notices of the Royal Astronomical Society.  474 (2017)  4 - p. 4552-4563 , 2017
 
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