Search Results - "Reionization"

Probing the epoch of reionization by Griffiths, Alex

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Epoch of reionization window. I. Mathematical formalism by Liu, A., Parsons, A., Trott, Cathryn

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The bispectrum and 21-cm foregrounds during the Epoch of Reionization by Watkinson, C.A., Trott, Cathryn, Hothi, I.

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The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array by Koopmans, L., Pritchard, J., Mellema, G., Abdalla, F., Aguirre, J., Ahn, K., Barkana, R., van Bemmel, I., Bernardi, G., Bonaldi, A., Briggs, F., de Bruyn, A., Chang, T., Chapman, E., Chen, X., Ciardi, B., Datta, K., Dayal, P., Ferrara, A., Fialkov, A., Fiore, F., Ichiki, K., Iliev, I., Inoue, S., Jelic, V., Jones, M., Lazio, J., Mack, K., Maio, U., Majumdar, S., Mesinger, A., Morales, M., Parsons, A., Pen, U., Santos, M., Schneider, R., Semelin, B., de Souza, R., Subrahmanyan, R., Takeuchi, T., Trott, Cathryn, Vedantham, H., Wagg, J., Webster, R., Wyithe, S.

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The effect of interplanetary scintillation on epoch of reionization power spectra by Trott, Cathryn, Tingay, Steven

“…These radio sources are a potential foreground contaminant signal for redshifted HI emission from the Epoch of Reionization (EoR) because they yield time-dependent flux density variations in bright extragalactic point sources. …”
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Lyman α emitters gone missing: evidence for late reionization? by Choudhury, Tirthankar Roy, Puchwein, Ewald, Haehnelt, Martin G., Bolton, James S.

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Planck intermediate results. XLVII. Planck constraints on reionization history by Adam, R., Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A.J., Barreiro, R.B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bucher, M., Burigana, C., Calabrese, E., Cardoso, J.-F., Carron, J., Chiang, H.C., Colombo, L.P.L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J.M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Elsner, F., Enßlin, T.A., Eriksen, H.K., Falgarone, E., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A.A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R.T., Gerbino, M., Ghosh, T., González-Nuevo, J., Górski, K.M., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Helou, G., Henrot-Versillé, S., Herranz, D., Hivon, E., Huang, Z., Ilić, S., Jaffe, A.H., Jones, W.C., Keihänen, E., Keskitalo, R., Kisner, T.S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J.-M., Langer, M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Le Jeune, M., Levrier, F., Lewis, A., Liguori, M., Lilje, P.B., López-Caniego, M., Ma, Y.-Z., Macías-Pérez, J.F., Maggio, G., Mangilli, A., Maris, M., Martin, P.G., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J.D., Meinhold, P.R., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschênes, M.-A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Moss, Adam, Naselsky, P., Natoli, P., Oxborrow, C.A., Pagano, L., Paoletti, D., Partridge, B., Patanchon, G., Patrizii, L., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Plaszczynski, S., Polastri, L., Polenta, G., Puget, J.-L., Rachen, J.P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rossetti, M., Roudier, G., Rubiño-Martín, J.A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirri, G., Sunyaev, R., Suur-Uski, A.-S., Tauber, J.A., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B.D., Wehus, I.K., White, M., Zacchei, A., Zonca, A.

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An Improved Statistical Point-source Foreground Model for the Epoch of Reionization by Murray, Steven, Trott, Cathryn, Jordan, C.

“…We present a sophisticated statistical point-source foreground model for low-frequency radio Epoch of Reionization (EoR) experiments using the 21 cm neutral hydrogen emission line. …”
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Reionization and high-redshift galaxies: the view from quasar absorption lines by Becker, George D., Bolton, James S., Lidz, Adam

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Investigating the contribution of extended radio sources to the Epoch of Reionization power spectrum by Cook, J.H., Trott, Cathryn, Line, Jack

Subjects: “…cosmology: dark ages, reionization, first stars…”
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Subtraction of Bright Point Sources from Synthesis Images of the Epoch of Reionization by Pindor, B., Wyithe, J., Mitchell, D., Ord, Stephen, Wayth, Randall, Greenhill, L.

“…Simulations show that this technique can improve the dynamic range of epoch-of-reionization maps by 2–3 orders of magnitude.…”
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Epoch of reionization window. II. Statistical methods for foreground wedge reduction by Liu, A., Parsons, A., Trott, Cathryn

“…For there to be a successful measurement of the 21 cm epoch of reionization (EoR) power spectrum, it is crucial that strong foreground contaminants be robustly suppressed. …”
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Study of redshifted H I from the epoch of reionization with drift scan by Paul, S., Sethi, S., Subrahmanyan, R., Udaya Shankar, N., Dwarakanath, K., Deshpande, A., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Corey, B., Emrich, David, Gaensler, B., Goeke, R., Greenhill, L., Hazelton, B., Hewitt, J., Johnston-Hollitt, M., Kaplan, D., Kasper, J., Kratzenberg, E., Lonsdale, C., Lynch, Mervyn, McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Oberoi, D., Ord, Stephen, Prabu, T., Rogers, A., Roshi, A., Srivani, K., Tingay, Steven, Wayth, Randall, Webster, R., Whitney, A., Williams, Andrew, Williams, C.

“…The detection of the Epoch of Reionization (EoR) in the redshifted 21-cm line is a challenging task. …”
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Assessment of Ionospheric Activity Tolerances for Epoch of Reionization Science with the Murchison Widefield Array by Trott, Cathryn, Jordan, Christopher, Murray, Steven, Pindor, B., Mitchell, D., Wayth, Randall, Line, J., McKinley, B., Beardsley, A., Bowman, J., Briggs, F., Hazelton, B., Hewitt, J., Jacobs, D., Morales, M., Pober, J., Sethi, S., Shankar, U., Subrahmanyan, R., Tegmark, M., Tingay, Steven, Webster, R., Wyithe, J.

“…Structure imprinted in foreground extragalactic point sources by ionospheric refraction has the potential to contaminate Epoch of Reionization (EoR) power spectra of the 21 cm emission line of neutral hydrogen. …”
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Robust statistics towards detection of the 21 cm signal from the Epoch of Reionization by Trott, Cathryn, Fu, Shih Ching, Murray, Steven, Jordan, Chris, Line, Jack, Barry, N., Byrne, R., Hazelton, B.J., Hasegawa, K., Joseph, R., Kaneuji, T., Kubota, K., Li, W., Lynch, Christene, McKinley, Ben, Mitchell, D.A., Morales, M.F., Pindor, B., Pober, J.C., Rahimi, M., Takahashi, K., Tingay, Steven, Wayth, Randall, Webster, R.L., Wilensky, M., Wyithe, J.S.B., Yoshiura, S., Zheng, Q., Walker, Mia

“…We explore methods for robust estimation of the 21 cm signal from the Epoch of Reionization (EoR). A Kernel Density Estimator (KDE) is introduced for measuring the spatial temperature fluctuation power spectrum from the EoR. …”
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The Effect of Baseline Layouts on the Epoch of Reionization Foreground Wedge: A Semianalytical Approach by Murray, Steven, Trott, Cathryn

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Exploring the evolution of reionization using a wavelet transform and the light cone effect by Trott, Cathryn

“…© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.The Cosmic Dawn and Epoch of Reionization, during which collapsed structures produce the first ionizing photons and proceed to reionize the intergalactic medium, span a large range in redshift (z ~ 30-6) and time (tage ~ 0.1-1.0 Gyr). …”
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The impact of realistic foreground and instrument models on 21 cm epoch of reionization experiments by Nasirudin, Ainulnabilah, Murray, Steven, Trott, Cathryn, Greig, B., Joseph, Ronniy C., Power, C.

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The Impact of Point-Source Subtraction Residuals on 21 cm Epoch of Reionization Estimation by Trott, Cathryn, Wayth, Randall, Tingay, Steven

“…Precise subtraction of foreground sources is crucial for detecting and estimating 21 cm H I signals from the Epoch of Reionization (EoR). We quantify how imperfect point-source subtraction due to limitations of the measurement data set yields structured residual signal in the data set. …”
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On the detectability of the hydrogen 3-cm fine-structure line from the epoch of reionization by Dijkstra, M., Lidz, A., Pritchard, J., Greenhill, L., Mitchell, D., Ord, S., Wayth, Randall

“…< 13.6 eV, that permeates neutral intergalactic gas during the epoch of reionization (EoR) excites the 2p (directly) and 2s (indirectly) states of atomic hydrogen. …”
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