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Testing Quadru- and Octopolar Asymmetry in Planck Data

Jønvik, Sara Clausen (Master thesis / Masteroppgave, 2017)

We perform an investigation of quadru- and octopolar asymmetry in the CMB data by expanding the on the study of alignment and angular clustering of the dipole components of the CMB power distribution across multipoles l = ...

Consistency relations for large-scale structures: Applications for the integrated Sachs-Wolfe effect and the kinematic Sunyaev-Zeldovich effect

Rizzo, Luca Alberto; Mota, David; Valageas, Patrick (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)

Consistency relations of large-scale structures provide exact nonperturbative results for cross-correlations of cosmic fields in the squeezed limit. They only depend on the equivalence principle and the assumption of ...

Constraints to Dark Energy Using PADE Parameterizations

Rezaei, M.; Malekjani, M.; Basilakos, S.; Mehrabi, A.; Mota, David (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)

Time delays and microlensing of gravitationally lensed quasars.

Dyrland, Karianne (Master thesis / Masteroppgave, 2019)

Thermal Dust Emission in the Microwave Frequency Range

Herman, Daniel Christopher (Master thesis / Masteroppgave, 2019)

Small-scale Intensity Mapping: Extended Halos as a Probe of the Ionizing Escape Fraction and Faint Galaxy Populations during Reionization

Mas Ribas, Lluis; Hennawi, J. F.; Dijkstra, Mark; Davies, Frederick B.; Stern, Jonathan; Rix, Hans-Walter (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)

Does a generalized Chaplygin gas correctly describe the cosmological dark sector?

vom Marttens, Rodrigo F.; Casarini, Luciano; Zimdahl, Winfried; Hipólito-Ricaldi, William S.; Mota, David (Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2017)

vom Marttens, R. F., et al. "Does a generalized Chaplygin gas correctly describe the cosmological dark sector?." Physics of the Dark Universe 15 (2017): 114-124. © 2017. This manuscript version is made available under the ...

Applications of Grid-Based Likelihood Methods to CMB Analysis

Mikkelsen, Kristin (Doctoral thesis / Doktoravhandling, 2014)

First analysis of solar structures in 1.21 mm full-disc ALMA image of the Sun

Brajša, R.; Sudar, D.; Benz, A. O.; Skokić, I.; Bárta, M.; De Pontieu, Bart Walter; Kim, S.; Kobelski, A.; Kuhar, M.; Shimojo, M.; Wedemeyer, Sven; White, S.; Yagoubov, P.; Yan, Y. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)

Context: Various solar features can be seen in emission or absorption on maps of the Sun in the millimetre and submillimetre wavelength range. The recently installed Atacama Large Millimetre/submillimetre Array (ALMA) is ...

Planck 2013 results. II. Low Frequency Instrument data processing

Aghanim, N; Armitage-Caplan, C; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; Baccigalupi, C; Banday, A. J.; Barreiro, RB; Battaner, E; Benabed, K; Benoit, A; Benoit-Levy, A; Bernard, JP; Bersanelli, M; Bielewicz, P; Bobin, J; Bock, JJ; Bonaldi, A; Bonavera, L; Bond, JR; Borrill, J; Bouchet, FR; Bridges, M; Bucher, M; Burigana, C; Butler, RC; Cappellini, B; Cardoso, JF; Catalano, A; Chamballu, A; Chen, X; Chiang, LY; Christensen, PR; Church, S; Colombi, S; Colombo, LPL; Crill, BP; Cruz, M; Curto, A; Cuttaia, F; Danese, L; Davies, RD; Davis, RJ; De Bernardis, P; De Rosa, A; De Zotti, G; Delabrouille, J; Dickinson, C; Diego, JM; Dole, H; Donzelli, S; Dore, O; Douspis, M; Dupac, X; Efstathiou, G; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Falvella, MC; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Gaier, TC; Galeotta, S; Ganga, K; Giard, M; Giardino, G; Giraud-Heraud, Y; Gjerløw, Eirik; Gonzalez-Nuevo, J; Gorski, KM; Gratton, S; Gregorio, A; Gruppuso, A; Hansen, Frode Kristian; Hanson, D; Harrison, D; Henrot-Versille, S; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Holmes, WA; Hornstrup, A; Hovest, W; Huffenberger, KM; Jaffe, AH; Jaffe, TR; Jewell, J; Jones, WC; Juvela, M; Kangaslahti, P; Keihänen, E; Keskitalo, R; Kiiveri, K; Kisner, TS; Knoche, J; Knox, L; Kunz, M; Kurki-Suonio, H; Lagache, G; Lähteenmäki, A; Lamarre, JM; Lasenby, A; Lattanzi, M; Laureijs, RJ; Lawrence, CR; Leach, S; Leahy, JP; Leonardi, R; Lesgourgues, J; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lindholm, V; Lopez-Caniego, M; Lubin, PM; MacIas-Perez, JF; Maggio, G; Maino, D; Mandolesi, N; Maris, M; Marshall, DJ; Martin, PG; Martinez-Gonzalez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Mazzotta, P; Meinhold, PR; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Moneti, A; Montier, L; Morgante, G; Morisset, N; Mortlock, D; Moss, A; Munshi, D; Naselsky, P; Natoli, P; Netterfield, CB; Nørgaard-Nielsen, HU; Novikov, D; Novikov, I; O'Dwyer, IJ; Osborne, S; Paci, F; Pagano, L; Paladini, R; Paoletti, D; Partridge, B; Pasian, F; Patanchon, G; Peel, M; Perdereau, O; Perotto, L; Perrotta, F; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Platania, P; Pointecouteau, E; Polenta, G; Ponthieu, N; Popa, L; Poutanen, T; Pratt, GW; Prezeau, G; Prunet, S; Puget, JL; Rachen, JP; Reach, WT; Rebolo, R; Reinecke, M; Remazeilles, M; Ricciardi, S; Riller, T; Robbers, G; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubino-Martin, JA; Rusholme, B; Salerno, E; Sandri, M; Santos, D; Scott, D; Seiffert, MD; Shellard, EPS; Spencer, LD; Starck, JL; Stolyarov, V; Stompor, R; Sureau, F; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Turler, M; Umana, G; Valenziano, L; Väliviita, Jussi-Pekka; Van Tent, B; Varis, J; Vielva, P; Villa, F; Vittorio, N; Wade, LA; Wandelt, BD; Watson, R; Wehus, IK; White, SDM; Wilkinson, A; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)

We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. ...

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