Zobrazeno 1 - 10
of 12 076
pro vyhledávání: '"HARPER, S."'
Autor:
Chung, D. T., Breysse, P. C., Cleary, K. A., Dunne, D. A., Lunde, J. G. S., Padmanabhan, H., Stutzer, N. -O., Tolgay, D., Bond, J. R., Church, S. E., Eriksen, H. K., Gaier, T., Gundersen, J. O., Harper, S. E., Harris, A. I., Hobbs, R., Ihle, H. T., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Wehus, I. K., Woody, D. P.
The Carbon monOxide Mapping Array Project (COMAP) Pathfinder survey continues to demonstrate the feasibility of line-intensity mapping using high-redshift carbon monoxide (CO) line emission traced at cosmological scales. The latest COMAP Pathfinder p
Externí odkaz:
http://arxiv.org/abs/2406.07512
Autor:
Stutzer, N. -O., Lunde, J. G. S., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Ihle, H. T., Padmanabhan, H., Tolgay, D., Wehus, I. K., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Harper, S. E., Hobbs, R., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Woody, D. P.
We present updated constraints on the cosmological 3D power spectrum of carbon monoxide CO(1-0) emission in the redshift range $2.4$-$3.4$. The constraints are derived from the two first seasons of Carbon monOxide Mapping Array Project (COMAP) Pathfi
Externí odkaz:
http://arxiv.org/abs/2406.07511
Autor:
Lunde, J. G. S., Stutzer, N. -O., Breysse, P. C., Chung, D. T., Cleary, K. A., Dunne, D. A., Eriksen, H. K., Harper, S. E., Ihle, H. T., Lamb, J. W., Pearson, T. J., Philip, L., Wehus, I. K., Woody, D. P., Bond, J. R., Church, S. E., Gaier, T., Gundersen, J. O., Harris, A. I., Hobbs, R., Kim, J., Lawrence, C. R., Murray, N., Padmanabhan, H., Readhead, A. C. S., Rennie, T. J., Tolgay, D.
The CO Mapping Array Project (COMAP) Pathfinder is performing line intensity mapping of CO emission to trace the distribution of unresolved galaxies at redshift $z \sim 3$. We present an improved version of the COMAP data processing pipeline and appl
Externí odkaz:
http://arxiv.org/abs/2406.07510
Autor:
Ghigna, T., Adler, A., Aizawa, K., Akamatsu, H., Akizawa, R., Allys, E., Anand, A., Aumont, J., Austermann, J., Azzoni, S., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Basyrov, A., Beckman, S., Bersanelli, M., Bortolami, M., Bouchet, F., Brinckmann, T., Campeti, P., Carinos, E., Carones, A., Casas, F. J., Cheung, K., Chinone, Y., Clermont, L., Columbro, F., Coppolecchia, A., Curtis, D., de Bernardis, P., de Haan, T., de la Hoz, E., De Petris, M., Della Torre, S., Monache, G. Delle, Di Giorgi, E., Dickinson, C., Diego-Palazuelos, P., García, J. J. Díaz, Dobbs, M., Dotani, T., D'Alessandro, G., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Farias, N., Ferreira, E., Franceschet, C., Fuskeland, U., Galloni, G., Galloway, M., Ganga, K., Gerbino, M., Gervasi, M., Génova-Santos, R. T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., González, R. González, Grandsire, L., Gruppuso, A., Halverson, N. W., Hargrave, P., Harper, S. E., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Herranz, D., Hivon, E., Hlozek, R. A., Hoang, T. D., Hubmayr, J., Ichiki, K., Ikuma, K., Ishino, H., Jaehnig, G., Jost, B., Kohri, K., Konishi, K., Lamagna, L., Lattanzi, M., Leloup, C., Levrier, F., Lonappan, A. I., Luzzi, G., Macias-Perez, J., Maffei, B., Marchitelli, E., Martínez-González, E., Masi, S., Matarrese, S., Matsumura, T., Micheli, S., Migliaccio, M., Monelli, M., Montier, L., Morgante, G., Mousset, L., Nagano, Y., Nagata, R., Natoli, P., Novelli, A., Noviello, F., Obata, I., Occhiuzzi, A., Odagiri, K., Omae, R., Pagano, L., Paiella, A., Paoletti, D., Pascual-Cisneros, G., Patanchon, G., Pavlidou, V., Piacentini, F., Piat, M., Piccirilli, G., Pinchera, M., Pisano, G., Porcelli, L., Raffuzzi, N., Raum, C., Remazeilles, M., Ritacco, A., Rubino-Martin, J., Ruiz-Granda, M., Sakurai, Y., Savini, G., Scott, D., Sekimoto, Y., Shiraishi, M., Signorelli, G., Stever, S. L., Sullivan, R. M., Suzuki, A., Takaku, R., Takakura, H., Takakura, S., Tartari, Y. Takase. A., Tassis, K., Thompson, K. L., Tomasi, M., Tristram, M., Tucker, C., Vacher, L., van Tent, B., Vielva, P., Watanuki, K., Wehus, I. K., Westbrook, B., Weymann-Despres, G., Winter, B., Wollack, E. J., Zacchei, A., Zannoni, M., Zhou, Y., Collaboration, the LiteBIRD
LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangi
Externí odkaz:
http://arxiv.org/abs/2406.02724
Autor:
Fernández-Torreiro, M., Rubiño-Martín, J. A., López-Caraballo, C. H., Génova-Santos, R. T., Peel, M. W., Guidi, F., Harper, S. E., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Herranz, D., Hoyland, R., Lasenby, A., Martínez-Gonzalez, E., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
Anomalous Microwave Emission (AME) is an important emission component between 10 and 60 GHz that is not yet fully understood. It seems to be ubiquituous in our Galaxy and is observed at a broad range of angular scales. Here we use the new QUIJOTE-MFI
Externí odkaz:
http://arxiv.org/abs/2305.06762
Autor:
Rubino-Martin, J. A., Guidi, F., Genova-Santos, R. T., Harper, S. E., Herranz, D., Hoyland, R. J., Lasenby, A. N., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Vansyngel, F., Vielva, P., Watson, R. A., Artal, E., Ashdown, M., Barreiro, R. B., Bilbao-Ahedo, J. D., Casas, F. J., Casaponsa, B., Cepeda-Arroita, R., de la Hoz, E., Dickinson, C., Fernandez-Cobos, R., Fernandez-Torreiro, M., Gonzalez-Gonzalez, R., Hernandez-Monteagudo, C., Lopez-Caniego, M., Lopez-Caraballo, C., Martinez-Gonzalez, E., Peel, M. W., Pelaez-Santos, A. E., Perrott, Y., Piccirillo, L., Razavi-Ghods, N., Scott, P., Titterington, D., Tramonte, D., Vignaga, R.
We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17 and 19GHz, and covering approximately 29000 deg$^2$, including most of the Northern sky region. These maps result from 9000 h of observations taken b
Externí odkaz:
http://arxiv.org/abs/2301.05113
Autor:
Singal, J., Fornengo, N., Regis, M., Bernardi, G., Bordenave, D., Branchini, E., Cappelluti, N., Caputo, A., Carucci, I. P., Chluba, J., Cuoco, A., DiLullo, C., Fialkov, A., Hale, C., Harper, S. E., Heston, S., Holder, G., Kogut, A., Krause, M. G. H., Leahy, J. P., Mittal, S., Monsalve, R. A., Piccirilli, G., Pinetti, E., Recchia, S., Taoso, M., Todarello, E.
Publikováno v:
2003, PASP, 135, 136001
We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the diffuse radio zero level continue to suggest that it is several times h
Externí odkaz:
http://arxiv.org/abs/2211.16547
Autor:
Ambrosino, E., Auweele, K.V., Been, J., Beijers, R., Bertens, L., Bloemenkamp, K., Boderie, N., Burdorf, L., Ochoa, L.B., de Jonge, A., de Weerth, C., Franx, A., Harper, S., Kazemier, B.M., Klein, P.P., Kretz, D., Labrecque, J., Mol, B.W., Muris, J., Nieuwenhuijze, M., Obermann, S., Oudijk, M., Peters, L., Ramerman, L., Ravelli, A., Schonewille-Rosman, A., Struijs, J., Torij, H., Van Beukering, M., van den Akker, T., van den Heuvel, M., van Dillen, J., van Lenthe, F., Van Ourti, T., Verhoeff, A., Vermeulen, M., Visser, N., Willers, S., Schoenmakers, S., Zainularab, Z., Gravesteijn, B.Y., Boderie, N.W., Bertens, L.C.M., Burgos Ochoa, L., Klein, P.P.F., Kwint-Reijnders, I., Labrecque, J.A., Obermann-Borst, S.A., Ravelli, A.C.J., Rosman, A., Been, J.V., de Groot, C.J.
Publikováno v:
In Public Health October 2024 235:15-25
Autor:
Harper, S. E., Dickinson, C., Barr, A., Cepeda-Arroita, R., Grumitt, R. D. P., Heilgendorff, H. M., Jew, L., Jonas, J. L., Jones, M. E., Leahy, J. P., Leech, J., Pearson, T. J., Peel, M. W., Readhead, A. C. S., Taylor, A. C.
The C-Band All-Sky Survey (C-BASS) has observed the Galaxy at 4.76GHz with an angular resolution of $0.73^\circ$ full-width half-maximum, and detected Galactic synchrotron emission with high signal-to-noise ratio over the entire northern sky ($\delta
Externí odkaz:
http://arxiv.org/abs/2202.10411
Autor:
Guidi, F., Rubiño-Martín, J. A., Pelaez-Santos, A. E., Génova-Santos, R. T., Ashdown, M., Barreiro, R. B., Bilbao-Ahedo, J. D., Harper, S. E., Watson, R. A.
Map-making is an important step for the data analysis of Cosmic Microwave Background (CMB) experiments. It consists of converting the data, which are typically a long, complex and noisy collection of measurements, into a map, which is an image of the
Externí odkaz:
http://arxiv.org/abs/2108.09063