Zobrazeno 1 - 10
of 67
pro vyhledávání: '"V. N., Pandey"'
Autor:
H. Gan, L. V. E. Koopmans, F. G. Mertens, M. Mevius, A. R. Offringa, B. Ciardi, B. K. Gehlot, R. Ghara, A. Ghosh, S. K. Giri, I. T. Iliev, G. Mellema, V. N. Pandey, S. Zaroubi
Publikováno v:
Astronomy & astrophysics, 663:A9. EDP Sciences
The detection of the 21 cm signal of neutral hydrogen from the Epoch of Reionization (EoR) is challenging due to bright foreground sources, radio frequency interference (RFI), the ionosphere, and instrumental effects. Even after correcting for these
Autor:
B. K. Gehlot, L. V. E. Koopmans, A. R. Offringa, H. Gan, R. Ghara, S. K. Giri, M. Kuiack, F. G. Mertens, M. Mevius, R. Mondal, V. N. Pandey, A. Shulevski, R. A. M. J. Wijers, S. Yatawatta
Publikováno v:
Astronomy & Astrophysics, 662:A97. EDP Sciences
Astronomy & Astrophysics, 662:A97
Astronomy and astrophysics, 662:A97. EDP Sciences
Astronomy & Astrophysics, 662:A97
Astronomy and astrophysics, 662:A97. EDP Sciences
Aims: Contamination from bright diffuse Galactic thermal and non-thermal radio emission poses crucial challenges in experiments aiming to measure the 21-cm signal of neutral hydrogen from the Cosmic Dawn and Epoch of Reionization. If not included in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12aaa5ba5ed2e35717a5c31016b90443
https://hdl.handle.net/1887/3561903
https://hdl.handle.net/1887/3561903
Autor:
H. Gan, F. G. Mertens, L. V. E. Koopmans, A. R. Offringa, M. Mevius, V. N. Pandey, S. A. Brackenhoff, E. Ceccotti, B. Ciardi, B. K. Gehlot, R. Ghara, S. K. Giri, I. T. Iliev, S. Munshi
Publikováno v:
Astronomy & astrophysics, 669:A20. EDP Sciences
Context. Detecting the 21 cm signal from the epoch of reionisation (EoR) has been highly challenging due to the strong astrophysical foregrounds, ionospheric effects, radio frequency interference (RFI), and instrumental effects. Better characterisati
Autor:
Mrinalini, Pal, V. S., Pandey, Ajay, Dhawal, Prachi, Upadhyay, Vartika, Ratanajay, Sharma, B. N., Singh, Ishwar, Das, V. N., Pandey
Publikováno v:
Journal of Drug Delivery & Therapeutics; 2022 Supplement, Vol. 12, p208-216, 9p
Autor:
F. Mertens, Abhik Ghosh, Benedetta Ciardi, B. K. Gehlot, Saleem Zaroubi, Sarod Yatawatta, Maaijke Mevius, Garrelt Mellema, H. Gan, A. R. Offringa, Léon V. E. Koopmans, Sambit K. Giri, Ilian T. Iliev, V. N. Pandey, Michiel A. Brentjens, Emma Chapman, Raghunath Ghara
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, ⟨10.1093/mnras/stab3233⟩
Monthly Notices of the Royal Astronomical Society, 509(3), 3693-3702. Oxford University Press
Mon.Not.Roy.Astron.Soc., 2021, ⟨10.1093/mnras/stab3233⟩
Monthly Notices of the Royal Astronomical Society, 509(3), 3693-3702. Oxford University Press
We investigate systematic effects in direction dependent gain calibration in the context of the Low-Frequency Array (LOFAR) 21-cm Epoch of Reionization (EoR) experiment. The LOFAR EoR Key Science Project aims to detect the 21-cm signal of neutral hyd
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::653e98fc07d668bfa5b97710dc64c879
Autor:
Abhik Ghosh, I. T. Iliev, Sambit K. Giri, Sarod Yatawatta, Léon V. E. Koopmans, A. R. Offringa, Vibor Jelić, M. B. Silva, Rajesh Mondal, Maaijke Mevius, Raghunath Ghara, Saleem Zaroubi, Joop Schaye, Garrelt Mellema, Florent Mertens, B. K. Gehlot, Simon Gazagnes, R. Kooistra, V. N. Pandey, K. M. B. Asad, B. Ciardi, Emma Chapman
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 493 (4), pp.4728-4748. ⟨10.1093/mnras/staa487⟩
Mon.Not.Roy.Astron.Soc., 2020, 493 (4), pp.4728-4747. ⟨10.1093/mnras/staa487⟩
Monthly Notices of the Royal Astronomical Society, 493(4), 4728-4747
Monthly Notices of the Royal Astronomical Society, 493(4), 4728-4747. Oxford University Press
Monthly notices of the Royal Astronomical Society
Mon.Not.Roy.Astron.Soc., 2020, 493 (4), pp.4728-4748. ⟨10.1093/mnras/staa487⟩
Mon.Not.Roy.Astron.Soc., 2020, 493 (4), pp.4728-4747. ⟨10.1093/mnras/staa487⟩
Monthly Notices of the Royal Astronomical Society, 493(4), 4728-4747
Monthly Notices of the Royal Astronomical Society, 493(4), 4728-4747. Oxford University Press
Monthly notices of the Royal Astronomical Society
We derive constraints on the thermal and ionization states of the intergalactic medium (IGM) at redshift $\approx$ 9.1 using new upper limits on the 21-cm power spectrum measured by the LOFAR radio-telescope and a prior on the ionized fraction at tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80e309f24f995bd4e5fea1f3e6d349b5
https://doi.org/10.1093/mnras/staa487
https://doi.org/10.1093/mnras/staa487
Autor:
F. de Gasperin, J. Vink, J. P. McKean, A. Asgekar, I. Avruch, M. J. Bentum, R. Blaauw, A. Bonafede, J. W. Broderick, M. Brüggen, F. Breitling, W. N. Brouw, H. R. Butcher, B. Ciardi, V. Cuciti, M. de Vos, S. Duscha, J. Eislöffel, D. Engels, R. A. Fallows, T. M. O. Franzen, M. A. Garrett, A. W. Gunst, J. Hörandel, G. Heald, M. Hoeft, M. Iacobelli, L. V. E. Koopmans, A. Krankowski, P. Maat, G. Mann, M. Mevius, G. Miley, R. Morganti, A. Nelles, M. J. Norden, A. R. Offringa, E. Orrú, H. Paas, V. N. Pandey, M. Pandey-Pommier, R. Pekal, R. Pizzo, W. Reich, A. Rowlinson, H. J. A. Rottgering, D. J. Schwarz, A. Shulevski, O. Smirnov, C. Sobey, M. Soida, M. Steinmetz, M. Tagger, M. C. Toribio, A. van Ardenne, A. J. van der Horst, M. P. van Haarlem, R. J. van Weeren, C. Vocks, O. Wucknitz, P. Zarka, P. Zucca
Publikováno v:
Astronomy & Astrophysics
Astronomy & astrophysics, 635. EDP Sciences
Astronomy and Astrophysics
Astronomy and Astrophysics, EDP Sciences, 2020, 635, pp.A150. ⟨10.1051/0004-6361/201936844⟩
Astronomy and astrophysics 635, A150 (2020). doi:10.1051/0004-6361/201936844
Astronomy & Astrophysics, 635, pp. 1-7
Astronomy & Astrophysics, 635, A150
Astronomy & Astrophysics, 635:A150. EDP Sciences
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A150. ⟨10.1051/0004-6361/201936844⟩
Astronomy & Astrophysics, 635, 1-7
Astronomy & astrophysics, 635. EDP Sciences
Astronomy and Astrophysics
Astronomy and Astrophysics, EDP Sciences, 2020, 635, pp.A150. ⟨10.1051/0004-6361/201936844⟩
Astronomy and astrophysics 635, A150 (2020). doi:10.1051/0004-6361/201936844
Astronomy & Astrophysics, 635, pp. 1-7
Astronomy & Astrophysics, 635, A150
Astronomy & Astrophysics, 635:A150. EDP Sciences
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A150. ⟨10.1051/0004-6361/201936844⟩
Astronomy & Astrophysics, 635, 1-7
The four persistent radio sources in the northern sky with the highest flux density at metre wavelengths are Cassiopeia A, Cygnus A, Taurus A, and Virgo A; collectively they are called the A-team. Their flux densities at ultra-low frequencies (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::612dc95fc83c60d515ae5d62db17b118
https://pub.uni-bielefeld.de/record/2942903
https://pub.uni-bielefeld.de/record/2942903
Autor:
Maaijke Mevius, Michiel A. Brentjens, Sarod Yatawatta, B. K. Gehlot, V. N. Pandey, M. Hatef, Léon V. E. Koopmans, A. R. Offringa, A. G. de Bruyn, Saleem Zaroubi, Vibor Jelić, K. M. B. Asad
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 478(2), 1484-1501. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 478(2), 1484-1501. Oxford University Press
Contamination due to foregrounds (Galactic and Extra-galactic), calibration errors and ionospheric effects pose major challenges in detection of the cosmic 21 cm signal in various Epoch of Reionization (EoR) experiments. We present the results of a p
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 476(3), 3051-3062. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 476(3), 3051-3062. Oxford University Press
Leakage of polarized Galactic diffuse emission into total intensity can potentially mimic the 21-cm signal coming from the epoch of reionization (EoR), as both of them might have fluctuating spectral structure. Although we are sensitive to the EoR si