The Effect of Asymmetric Beams in the Wilkinson Microwave Anisotropy Probe Experiment von Wehus, I. K, Ackerman, L, Eriksen, H. K, Groeneboom, N. E

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Cosmic Microwave Background Likelihood Approximation by a Gaussianized Blackwell-Rao Estimator von Rudjord, Ø, Groeneboom, N. E, Eriksen, H. K, Huey, Greg, Górski, K. M, Jewell, J. B

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Bayesian Analysis of White Noise Levels in the Five-Year WMAP Data von Groeneboom, N. E, Eriksen, H. K, Gorski, K, Huey, G, Jewell, J, Wandelt, B

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Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models von Hou, Zhen, Banday, A. J., Górski, K. M., Groeneboom, N. E., Eriksen, H. K.

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INTRODUCING GAMER: A FAST AND ACCURATE METHOD FOR RAY-TRACING GALAXIES USING PROCEDURAL NOISE von Groeneboom, N E, Dahle, H

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Constraining dark energy anisotropic stress von Mota, David F., Kristiansen, Jostein R., Koivisto, Tomi, Groeneboom, Nicolaas E.

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INTRODUCING GAMER: A FAST AND ACCURATE METHOD FOR RAY-TRACING GALAXIES USING PROCEDURAL NOISE von Groeneboom, N. E., Dahle, H.

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Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models von Hou, Zhen, Banday, A. J., Górski, K. M., Groeneboom, N. E., Eriksen, H. K.

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BAYESIAN ANALYSIS OF WHITE NOISE LEVELS IN THE FIVE-YEAR WMAP DATA von Groeneboom, N. E., Eriksen, H. K., Gorski, K., Huey, G., Jewell, J., Wandelt, B.

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Planck 2013 results. XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources von Aghanim, N, Aussel, H, Banday, AJ, Bartlett, JG, Benabed, K, Bobin, J, Bock, JJ, Bonaldi, A, Bucher, M, Burigana, C, Chamballu, A, Church, S, Colombi, S, Comis, B, Couchot, F, Coulais, A, Crill, BP, Cuttaia, F, De Bernardis, P, De Rosa, A, Delouis, J-M, Desert, F-X, Dickinson, C, Dole, H, Donzelli, S, Ensslin, TA, Ferragamo, A, Flores-Cacho, I, Forni, O, Frailis, M, Franceschi, E, Genova-Santos, RT, Giard, M, Gonzalez-Nuevo, J, Hansen, FK, Hanson, D, Harrison, D, Henrot-Versille, S, Herranz, D, Hildebrandt, SR, Jaffe, TR, Kneissl, R, Knoche, J, Kunz, M, Lahteenmaki, A, Lamarre, J-M, Leahy, JP, Li, C, Liguori, M, Lopez-Caniego, M, Maffei, B, Maino, D, Maris, M, Marshall, DJ, Mazzotta, P, Meinhold, PR, Mendes, L, Migliaccio, M, Miville-Deschenes, M-A, Munshi, D, Murphy, JA, Natoli, P, Nesvadba, NPH, Novikov, D, Olamaie, M, Osborne, S, Oxborrow, CA, Paoletti, D, Patanchon, G, Piat, M, Pierpaoli, E, Popa, L, Poutanen, T, Pratt, GW, Prezeau, G, Puget, J-L, Rachen, JP, Reach, WT, Ricciardi, S, Rossee, C, Rowan-Robinson, M, Rusholme, B, Santos, D, Saunders, RDE, Savini, G, Scott, D, Shimwele, TW, Starck, J-L, Stolyarov, V, Sunyaev, R, Suur-Uski, A-S, Tauber, JA, Terenzi, L, Toffolatti, L, Tristram, M, Tucci, M, Valenziano, L, Vibert, L, Wandelt, BD, Zacchei, A

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Bayesian analysis of white noise levels in the 5-year WMAP data von Groeneboom, N E, Eriksen, H K, Gorski, K, Huey, G, Jewell, J, Wandelt, B

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Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources von Aghanim, N, Aussel, H, Banday, AJ, Bartlett, JG, Benabed, K, Bernard, J, Bobin, J, Bock, JJ, Bonaldi, A, Bucher, M, Burigana, C, Chamballu, A, Colombi, S, Comis, B, Couchot, F, Coulais, A, Crill, BP, Cuttaia, F, De Bernardis, P, Delouis, J-M, Desert, F-X, Dickinson, C, Dole, H, Flores-Cacho, I, Frailis, M, Franceschi, E, Genova-Santos, RT, Giard, M, Gonzalez-Nuevo, J, Hansen, FK, Hanson, D, Harrison, D, Elenrot-Versille, S, Herranz, D, Hildebrandt, SR, Jaffe, TR, Kneissl, R, Knoche, J, Kunz, M, Laeache, G, Lahteenmaki, A, Lamarre, J-M, Leahy, JP, Li, C, Liguori, M, Lopez-Caniego, M, Maffei, B, Maino, D, Maris, M, Mazzotta, P, Meinhold, PR, Meichiorri, A, Mendes, L, Mennelia, A, Migliaccio, M, Miville-Deschenes, M-A, Munshi, D, Murphy, JA, Natoli, P, Netterfield, CB, Osborne, S, Oxborrow, CA, Pagano, L, Pasian, F, Perotto, L, Perrotta, F, Piacentini, F, Plaszczynski, S, Polenta, O, Ponthieu, N, Poutanen, T, Prezeau, G, Prunet, S, Puget, J-L, Rachen, JP, Rebolo, R, Ricciardi, S, Riller, T, Rowan-Robinson, M, Santos, D, Savini, G, Schammel, MP, Shimwell, TW, Spencer, LD, Stanford, SA, Starck, J-L, Stolyarov, V, Sutton, D, Sygnet, J-F, Tauber, JA, Tavagnacco, D, Tucci, M, Tuovinen, J, Tuerler, M, Umana, G, Van Tent, B, Vielva, P, Vilia, F, Yvon, D, Zacchei, A

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Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models von Hou, Zhen, Banday, A J, Gorski, K M, Groeneboom, N E, Eriksen, H K

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Constraining Dark Energy Anisotropic Stress von Mota, D F, Kristiansen, J R, Koivisto, T, Groeneboom, N E

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CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator von Rudjord, Ø, Groeneboom, N E, Eriksen, H K, Huey, Greg, Górski, K M, Jewell, J B

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Imprints of a hemispherical power asymmetry in the seven-year WMAP data due to non-commutativity of space-time von Groeneboom, N. E, Axelsson, M, Mota, D. F, Koivisto, T

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Imprints of a hemispherical power asymmetry in the seven-year WMAP data due to non-commutativity of space-time von Groeneboom, N E, Axelsson, M, Mota, D F, Koivisto, T

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SDSS J2222+2745: A GRAVITATIONALLY LENSED SEXTUPLE QUASAR WITH A MAXIMUM IMAGE SEPARATION OF 15".1 DISCOVERED IN THE SLOAN GIANT ARCS SURVEY von Dahle, H, Gladders, M D, Sharon, K, Bayliss, M B, Wuyts, E, Abramson, L E, Koester, B P, Groeneboom, N, Brinckmann, T E, Kristensen, M T, LINDHOLMER, M O, Nielsen, A, KROGAGER, J-K, Fynbo, J P U

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SDSS J2222+2745: A GRAVITATIONALLY LENSED SEXTUPLE QUASAR WITH A MAXIMUM IMAGE SEPARATION OF 15.''1 DISCOVERED IN THE SLOAN GIANT ARCS SURVEY von Dahle, H., Groeneboom, N., Gladders, M. D., Abramson, L. E., Sharon, K., Bayliss, M. B., Wuyts, E., Koester, B. P., Brinckmann, T. E., Kristensen, M. T., Lindholmer, M. O., Nielsen, A., Krogager, J.-K., Fynbo, J. P. U.

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SDSS J2222+2745: A GRAVITATIONALLY LENSED SEXTUPLE QUASAR WITH A MAXIMUM IMAGE SEPARATION OF 15.″1 DISCOVERED IN THE SLOAN GIANT ARCS SURVEY von Dahle, H., Gladders, M. D., Sharon, K., Bayliss, M. B., Wuyts, E., Abramson, L. E., Koester, B. P., Groeneboom, N., Brinckmann, T. E., Kristensen, M. T., Lindholmer, M. O., Nielsen, A., Krogager, J.-K., Fynbo, J. P. U.

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