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207 results on '"Ade, P.A.R."'

2. The South Pole Telescope

Author

Ruhl, J.E., Ade, P.A.R., Carlstrom, J.E., Cho, H.M., Crawford, T., Dobbs, M., Greer, C.H., Halverson, N.W., Holzapfel, W.L., Lanting, T.M., Lee, A.T., Leitch, E.M., Leong, J., Lu, W., Lueker, M., Mehl, J., Meyer, S.S., Mohr, J.J., Padin, S., Plagge, T., Pryke, C., Runyan, M.C., Schwan, D., Sharp, M.K., Spieler, H., Staniszewski, Z., and Stark, A.A.

Subjects
Physics of elementary particles and fields, Radio telescopes Millimeter- and Submillimeter-wave Techniques Bolometric detectors Focal plane arrays
Abstract

A new 10 meter diameter telescope is being constructed for deployment at the NSF South Pole research station. The telescope is designed for conducting large-area millimeter and sub-millimeter wave surveys of faint, low contrast emission, as required to map primary and secondary anisotropies in the cosmic microwave background. To achieve the required sensitivity and resolution, the telescope design employs an off-axis primary with a 10 m diameter clear aperture. The full aperture and the associated optics will have a combined surface accuracy of better than 20 microns rms to allow precision operation in the submillimeter atmospheric windows. The telescope will be surrounded with a large reflecting ground screen to reduce sensitivity to thermal emission from the ground and local interference. The optics of the telescope will support a square degree field of view at 2mm wavelength and will feed a new 1000-element micro-lithographed planar bolometric array with superconducting transition-edge sensors and frequency-multiplexed readouts. The first key project will be to conduct a survey over 4000 degrees for galaxy clusters using the Sunyaev-Zel dovich Effect. This survey should find many thousands of clusters with a mass selection criteria that is remarkably uniform with redshift. Armed with redshifts obtained from optical and infrared follow-up observations, it is expected that the survey will enable significant constraints to be placed on the equation of state of the dark energy.

Published
2004

3. Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology

Author

de Bernardis, P., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Coble, K., Contaldi, C.R., Crill, B.P., De Troia, G., Farese, P., Ganga, K., Giacometti, M., Hivon, E., Hristov, V.V., Iacoangeli, A., Jaffe, A.H., Jones, W.C., Lange, A.E., Martinis, L., Masi, S., Mason, P., Mauskopf, P.D., Melchiorri, A., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Pongetti, F., Prunet, S., Romeo, G., Ruhl, J.E., and Scaramuzzi, F.

Subjects
General and miscellaneous//mathematics, computing, and information science
Published
2001

4. A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation

Author

de Bernardis, P., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Coble, K., Crill, B.P., De Gasperis, G., Farese, P.C., Ferreira, P.G., Ganga, K., Giacometti, M., Hivon, E., Hristov, V.V., Iacoangeli, A., Jaffe, A.H., Lange, A.E., Martinis, L., Masi, S., Mason, P., Mauskopf, P.D., Melchiorri, A., Miglio, L., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Prunet, S., Rao, S., Romeo, G., Ruhl, J.E., Scaramuzzi, F., Sforna, D., and Vittorio, N.

Subjects
General and miscellaneous//mathematics, computing, and information science
Published
2000

5. The thermal design, characterization, and performance of the Spider long-duration balloon cryostat

Author

Ade, P.A.R., Amiri, M., Benton, S.J., Bock, J.J., Bond, J.R., Bryan, S.A., Chiang, H.C., Contaldi, C.R., Crill, B.P., Dore, O., Filippini, J.P., Fraisse, A.A., Gambrel, A., Gandilo, N.N., Hasselfield, M., Halpern, M., Hilton, G., Holmes, W., Hristov, V.V., Irwin, K.D., Jones, W.C., Kermish, Z., MacTavish, C.J., Mason, P.V., Megerian, K., Moncelsi, L., Montroy, T.E., Morford, T.A., Nagy, J.M., Netterfield, C.B., Rahlin, A.S., Reintsema, C.D., Ruhl, J.E., Runyan, M.C., Shariff, J.A., Soler, J.D., Trangsrud, A., Tucker, C., Tucker, R.S., Turner, A.D., Wiebe, D.V., Young, E., and Gudmundsson, J.E.

Published
2015
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6. 2022 upgrade and improved low frequency camera sensitivity for CMB observation at the South Pole

Author

Soliman, Ahmed, primary, Ade, P.A.R., additional, Ahmed, Z., additional, Amiri, M., additional, Barkats, D., additional, Basu Thakur, R., additional, Bischoff, C.A., additional, Beck, D., additional, Bock, J.J., additional, Buza, V., additional, Cheshire, J., additional, Connors, J., additional, Cornelison, J., additional, Crumrine, M., additional, Cukierman, A.J., additional, Denison, E.V., additional, Dierichx, M.I., additional, Duband, L., additional, Eiben, M., additional, Fatigoni, S., additional, Filippini, J.P., additional, Giannakopoulos, C., additional, Goeckner-Wald, N., additional, Goldfinger, D.C., additional, Grayson, J., additional, Grimes, P.K., additional, Hall, G., additional, Halal, G., additional, Halpern, M., additional, Hand, E., additional, Harrison, S.A., additional, Henderson, S., additional, Hildebrandt, S.R., additional, Hilton, G.C., additional, Hubmayr, J., additional, Hui, H., additional, Irwin, K.D., additional, Kang, J., additional, Karkare, K.S., additional, Kefeli, S., additional, Kovac, J.M., additional, Kuo, C.L., additional, Lau, K., additional, Leitch, E.M., additional, Lennox, A., additional, Liu, T., additional, Megerian, K.G., additional, Minutolo, L., additional, Moncelsi, L., additional, Nakato, Y., additional, Namikawa, T., additional, Nguyen, H.T., additional, O'Brient, R., additional, Palladino, S., additional, Petroff, M.A., additional, Precup, N., additional, Prouve, T., additional, Pryke, C., additional, Racine, B., additional, Reintsema, C.D., additional, Salatino, M., additional, Schillaci, A., additional, Schmitt, B.L., additional, Singari, B., additional, Germaine, T. St., additional, Steinback, B., additional, Sudiwala, R.V., additional, Thompson, K.L., additional, Tsai, C., additional, Tucker, C., additional, Turner, A.D., additional, Umilta, C., additional, Verges, C., additional, Vieregg, A.G., additional, Wandui, A., additional, Weber, A.C., additional, Wiebe, D.V., additional, Willmert, J., additional, Wu, W.L.K., additional, Yang, H., additional, Yoon, K.W., additional, Young, E., additional, Yu, C., additional, Zeng, L., additional, Zhang, C., additional, and Zhang, S., additional

Published
2022
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7. The large scale polarization explorer (LSPE) for CMB measurements: performance forecast

Author

Addamo, G., additional, Ade, P.A.R., additional, Baccigalupi, C., additional, Baldini, A.M., additional, Battaglia, P.M., additional, Battistelli, E.S., additional, Baù, A., additional, de Bernardis, P., additional, Bersanelli, M., additional, Biasotti, M., additional, Boscaleri, A., additional, Caccianiga, B., additional, Caprioli, S., additional, Cavaliere, F., additional, Cei, F., additional, Cleary, K.A., additional, Columbro, F., additional, Coppi, G., additional, Coppolecchia, A., additional, Cuttaia, F., additional, D'Alessandro, G., additional, De Gasperis, G., additional, De Petris, M., additional, Fafone, V., additional, Farsian, F., additional, Ferrari Barusso, L., additional, Fontanelli, F., additional, Franceschet, C., additional, Gaier, T.C., additional, Galli, L., additional, Gatti, F., additional, Genova-Santos, R., additional, Gerbino, M., additional, Gervasi, M., additional, Ghigna, T., additional, Grosso, D., additional, Gruppuso, A., additional, Gualtieri, R., additional, Incardona, F., additional, Jones, M.E., additional, Kangaslahti, P., additional, Krachmalnicoff, N., additional, Lamagna, L., additional, Lattanzi, M., additional, López-Caraballo, C.H., additional, Lumia, M., additional, Mainini, R., additional, Maino, D., additional, Mandelli, S., additional, Maris, M., additional, Masi, S., additional, Matarrese, S., additional, May, A., additional, Mele, L., additional, Mena, P., additional, Mennella, A., additional, Molina, R., additional, Molinari, D., additional, Morgante, G., additional, Natale, U., additional, Nati, F., additional, Natoli, P., additional, Pagano, L., additional, Paiella, A., additional, Panico, F., additional, Paonessa, F., additional, Paradiso, S., additional, Passerini, A., additional, Perez-de-Taoro, M., additional, Peverini, O.A., additional, Pezzotta, F., additional, Piacentini, F., additional, Piccirillo, L., additional, Pisano, G., additional, Polenta, G., additional, Poletti, D., additional, Presta, G., additional, Realini, S., additional, Reyes, N., additional, Rocchi, A., additional, Rubino-Martin, J.A., additional, Sandri, M., additional, Sartor, S., additional, Schillaci, A., additional, Signorelli, G., additional, Siri, B., additional, Soria, M., additional, Spinella, F., additional, Tapia, V., additional, Tartari, A., additional, Taylor, A.C., additional, Terenzi, L., additional, Tomasi, M., additional, Tommasi, E., additional, Tucker, C., additional, Vaccaro, D., additional, Vigano, D.M., additional, Villa, F., additional, Virone, G., additional, Vittorio, N., additional, Volpe, A., additional, Watkins, R.E.J., additional, Zacchei, A., additional, and Zannoni, M., additional

Published
2021
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8. Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data

Author

Dutcher, D., Balkenhol, L., Ade, P.A.R., Ahmed, Z., Anderes, E., Anderson, A.J., Archipley, M., Avva, J.S., Aylor, K., Barry, P.S., Thakur, R. Basu, Benabed, K., Bender, A.N., Benson, B.A., Bianchini, F., Bleem, L.E., Bouchet, F.R., Bryant, L., Byrum, K., Carlstrom, J.E., Carter, F.W., Cecil, T.W., Chang, C.L., Chaubal, P., Chen, G., Cho, H.-M., Chou, T.-L., Cliche, J.-F., Crawford, T.M., Cukierman, A., Daley, C., De Haan, T., Denison, E.V., Dibert, K., Ding, J., Dobbs, M.A., Everett, W., Feng, C., Ferguson, K.R., Foster, A., Fu, J., Galli, S., Gambrel, A.E., Gardner, R.W., Goeckner-Wald, N., Gualtieri, R., Guns, S., Gupta, N., Guyser, R., Halverson, N.W., Harke-Hosemann, A.H., Harrington, N.L., Henning, J.W., Hilton, G.C., Hivon, E., Holder, G.P., Holzapfel, W.L., Hood, J.C., Howe, D., Huang, N., Irwin, K.D., Jeong, O.B., Jonas, M., Jones, A., Khaire, T.S., Knox, L., Kofman, A.M., Korman, M., Kubik, D.L., Kuhlmann, S., Kuo, C.-L., Lee, A.T., Leitch, E.M., Lowitz, A.E., Lu, C., Meyer, S.S., Michalik, D., Millea, M., Montgomery, J., Nadolski, A., Natoli, T., Nguyen, H., Noble, G.I., Novosad, V., Omori, Y., Padin, S., Pan, Z., Paschos, P., Pearson, J., Posada, C.M., Prabhu, K., Quan, W., Raghunathan, S., Rahlin, A., Reichardt, C.L., Riebel, D., Riedel, B., Rouble, M., Ruhl, J.E., Sayre, J.T., Schiappucci, E., Shirokoff, E., Smecher, G., Sobrin, J.A., Stark, A.A., Stephen, J., Story, K.T., Suzuki, A., Thompson, K.L., Thorne, B., Tucker, C., Umilta, C., Vale, L.R., Vanderlinde, K., Vieira, J.D., Wang, G., Whitehorn, N., Wu, W.L.K., Yefremenko, V., Yoon, K.W., Young, M.R., Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and SPT-3G

Subjects
dimension: 6, satellite: Planck, Cosmology and Nongalactic Astrophysics (astro-ph.CO), pole, cosmic background radiation: spectrum, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, gravitation: lens, cosmological model: parameter space, correlation, cosmic background radiation: multipole, polarization: power spectrum, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

International audience; We present measurements of the E-mode (EE) polarization power spectrum and temperature-E-mode (TE) cross-power spectrum of the cosmic microwave background using data collected by SPT-3G, the latest instrument installed on the South Pole Telescope. This analysis uses observations of a 1500 deg2 region at 95, 150, and 220 GHz taken over a four-month period in 2018. We report binned values of the EE and TE power spectra over the angular multipole range 300≤ℓ<3000, using the multifrequency data to construct six semi-independent estimates of each power spectrum and their minimum-variance combination. These measurements improve upon the previous results of SPTpol across the multipole ranges 300≤ℓ≤1400 for EE and 300≤ℓ≤1700 for TE, resulting in constraints on cosmological parameters comparable to those from other current leading ground-based experiments. We find that the SPT-3G data set is well fit by a ΛCDM cosmological model with parameter constraints consistent with those from Planck and SPTpol data. From SPT-3G data alone, we find H0=68.8±1.5 km s−1 Mpc−1 and σ8=0.789±0.016, with a gravitational lensing amplitude consistent with the ΛCDM prediction (AL=0.98±0.12). We combine the SPT-3G and the Planck data sets and obtain joint constraints on the ΛCDM model. The volume of the 68% confidence region in six-dimensional ΛCDM parameter space is reduced by a factor of 1.5 compared to Planck-only constraints, with no significant shifts in central values. We note that the results presented here are obtained from data collected during just half of a typical observing season with only part of the focal plane operable, and that the active detector count has since nearly doubled for observations made with SPT-3G after 2018.

Published
2021
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9. The quasi-optical design of the QUaD telescope

Author

O’Sullivan, C., Cahill, G., Murphy, J.A., Gear, W.K., Harris, J., Ade, P.A.R., Church, S.E., Thompson, K.L., Pryke, C., Bock, J., Bowden, M., Brown, M.L., Carlstrom, J.E., Castro, P.G., Culverhouse, T., Friedman, R.B., Ganga, K.M., Haynes, V., Hinderks, J.R., Kovak, J., Lange, A.E., Leitch, E.M., Mallie, O.E., Melhuish, S.J., Orlando, A., Piccirillo, L., Pisano, G., Rajguru, N., Rusholme, B.A., Schwarz, R., Taylor, A.N., Wu, E.Y.S., and Zemcov, M.

Published
2008
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10. New artificial dielectric metamaterial and its application as a terahertz antireflection coating

Author

Zhang, J., Ade, P.A.R., Mauskopf, P., Moncelsi, L., Savini, G., and Whitehouse, N.

Subjects
Dielectrics -- Usage, Dielectrics -- Production processes, Dielectrics -- Materials, Optical coatings -- Materials, Optical coatings -- Properties, Astronomy, Physics
Abstract

We describe a novel artificial dielectric material that has applications at millimeter and submillimeter wavelengths. The material is manufactured from layers of metal mesh patterned onto thin polypropylene sheets, which are then bonded together using a hot pressing process to provide planar rugged discs that can be reliably cycled to cryogenic temperatures. The refractive index of this material can be tuned by adjusting the geometry and spacing of the metal mesh layers. We demonstrate its usage by designing and characterizing a broadband antireflection coating for a Z-cut crystalline quartz plate. The coating was fabricated and applied to the quartz using the hot press technique and characterized using a Fourier transform spectrometer. The performance is shown to be in good agreement with a high frequency structure simulator and transmission line modeling results. OCIS codes: 160.3918, 160.4670.

Published
2009

11. South Pole Telescope optics

Author

Padin, S., Staniszewski, Z., Keisler, R., Joy, M., Stark, A.A., Ade, P.A.R., Aird, K.A., Benson, B.A., Bleem, L.E., Carlstrom, J.E., Chang, C.L., Crawford, T.M., Crites, A.T., Dobbs, M.A., Halverson, N.W., Heimsath, S., Hills, R.E., Holzapfel, W.L., Lawrie, C., Lee, A.T., Leitch, E.M., Leong, J., Lu, W., Lueker, M., McMahon, J.J., Meyer, S.S., Mohr, J.J., Montroy, T.E., Plagge, T., Pryke, C., Ruhl, J.E., Schaffer, K.K., Shirokoff, E., Spieler, H.G., and Vieira, J.D.

Subjects
Optics -- Research, Telescope -- Properties, Telescope -- Design and construction, Astronomy, Physics, South Pole Telescope (Telescope) -- Properties, South Pole Telescope (Telescope) -- Design and construction
Abstract

The South Pole Telescope is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, millimeter-wave, bolometer array receiver. The telescope has an unusual optical system with a cold stop around the secondary. The design emphasizes low scattering and low background loading. All the optical components except the primary are cold, and the entire beam from prime focus to the detectors is surrounded by cold absorber. OCIS codes: 350.1260, 110.6770, 220.4880, 090.2910.

Published
2008

12. Optical design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera

Author

Fowler, J.W., Niemack, M.D., Dicker, S.R., Aboobaker, A.M., Ade, P.A.R., Battistelli, E.S., Devlin, M.J., Fisher, R.P., Halpern, M., Hargrave, P.C., Hincks, A.D., Kaul, M., Klein, J., Lau, J.M., Limon, M., Marriage, T.A., Mauskopf, P.D., Page, L., Staggs, S.T., Swetz, D.S., Switzer, E.R., Thornton, R.J., and Tucker, C.E.

Subjects
Optical detectors -- Usage, Optics, Physical -- Measurement, Telescope -- Design and construction, Astronomy, Physics
Abstract

The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background simultaneously at 145, 215, and 280 GHz with arcminute resolution. Each frequency will have a 32 by 32 element focal plane array of transition edge sensor bolometers. The telescope and the cold reimaging optics are optimized for millimeter-wave observations with these sensitive detectors. The design of each is described. OCIS codes: 040.1240, 080.3620, 350.1260.

Published
2007

13. CMB polarization with B oomerang 2003

Author

Piacentini, F., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Jones, W.C., Lange, A.E., Marini-Bettolo, C., Masi, S., Mauskopf, P.D., MacTavish, C.J., Melchiorri, A., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C.B., Pascale, E., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., and Vittorio, N.

Published
2007
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14. The BRAIN CMB polarization experiment

Author

Polenta, G., Ade, P.A.R., Bartlett, J., Bréelle, E., Conversi, L., de Bernardis, P., Dufour, C., Gervasi, M., Giard, M., Giordano, C., Giraud-Heraud, Y., Maffei, B., Masi, S., Nati, F., Orlando, A., Peterzen, S., Piacentini, F., Piat, M., Piccirillo, L., Pisano, G., Pons, R., Rosset, C., Savini, G., Sironi, G., Tartari, A., Veneziani, M., and Zannoni, M.

Published
2007
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15. Searching for non-Gaussian signals in the BOOMERanG 2003 CMB map: Preliminary results

Author

De Troia, G., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., de Gasperis, G., de Oliveira-Costa, A., Di Stefano, G., Ferreira, P.G., Hivon, E., Jaffe, A., Kisner, T., Kunz, M., Jones, W.C., Lange, A.E., Masi, S., Mauskopf, P.D., MacTavish, C., Melchiorri, A., Montroy, T., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., and Vittorio, N.

Published
2007
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16. The millimeter sky as seen with BOOMERanG

Author

Masi, S., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., De Oliveira-Costa, A., De Troia, G., Di Stefano, G., Ehlers, P., Hivon, E., Hristov, V., Iacoangeli, A., Jaffe, A.H., Jones, W.C., Kisner, T.S., Lange, A.E., MacTavish, C.J., Marini Bettolo, C., Mason, P., Mauskopf, P.D., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Torbet, E., Veneziani, M., and Vittorio, N.

Published
2007
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17. The Quasi-Optical Design of the QUaD Telescope

Author

O’Sullivan, C., Cahill, G., Murphy, J.A., Gear, W.K., Harris, J., Ade, P.A.R., Church, S.E., Thompson, K.L., Pryke, C., Bock, J., Bowden, M., Brown, M.L., Carlstrom, J.E., Castro, P.G., Culverhouse, T., Friedman, R.B., Ganga, K.M., Haynes, V., Hinderks, J.R., Kovak, J., Lange, A.E., Leitch, E.M., Mallie, O.E., Melhuish, S.J., Orlando, A., Piccirillo, L., Pisano, G., Rajguru, N., Rusholme, B.A., Schwarz, R., Taylor, A.N., Wu, E.Y.S., and Zemcov, M.

Published
2007
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18. Analysis of Temperature-to-Polarization Leakage in BICEP3 and Keck CMB Data from 2016 to 2018

Author

St Germaine, Tyler, primary, Ade, P.A.R., additional, Ahmed, Zeeshan, additional, Amiri, Mandana, additional, Barkats, Denis, additional, Basu Thakur, Ritoban, additional, Bischoff, Colin A., additional, Bock, James J., additional, Boenish, Hans, additional, Bullock, Eric, additional, Buza, Victor, additional, Cheshire, James R., additional, Connors, Jake, additional, Cornelison, James, additional, Crumrine, Michael, additional, Cukierman, Ari Jozef, additional, Denison, Edward, additional, Dierickx, Marion, additional, Duband, Lionel, additional, Eiben, Miranda, additional, Fatigoni, Sofia, additional, Filippini, Jeff, additional, Fliescher, Stefan, additional, Goeckner-Wald, Neil, additional, Goldfinger, David, additional, Grayson, James A., additional, Grimes, Paul, additional, Hall, Grantland, additional, Halpern, Mark, additional, Harrison, Sam A., additional, Henderson, Shawn, additional, Hildebrandt, Sergi, additional, Hilton, Gene C., additional, Hubmayr, Johannes, additional, Hui, Howard, additional, Irwin, Kent D., additional, Kang, Jae Hwan, additional, Karkare, Kirit S., additional, Karpel, Ethan, additional, Kefeli, Sinan, additional, Kernasovskiy, Sarah A., additional, Kovac, John M., additional, Kuo, Chao-Lin, additional, Lau, King, additional, Leitch, Erik M., additional, Megerian, Koko G., additional, Minutolo, Lorenzo, additional, Moncelsi, Lorenzo, additional, Nakato, Yuka, additional, Namikawa, Toshiya, additional, Nguyen, Hien T., additional, O'brient, Roger, additional, Ogburn, R. Walt, additional, Palladino, Steven, additional, Precup, Nathan, additional, Prouve, Thomas, additional, Pryke, Clement, additional, Racine, Benjamin, additional, Reintsema, Carl, additional, Richter, Steffen, additional, Schillaci, Alessandro, additional, Schmitt, Benjamin, additional, Schwartz, Robert, additional, Sheehy, Chris D., additional, Soliman, Ahmed, additional, Steinbach, Bryan, additional, Sudiwala, Rashmi, additional, Teply, Grant, additional, Thompson, Keith L., additional, Tolan, James E., additional, Tucker, Carole, additional, Turner, Anthony D., additional, Umilta, Caterina, additional, Vieregg, Abigail G., additional, Wandui, Albert, additional, Weber, Alexis C., additional, Wiebe, Don, additional, Willmert, Justin, additional, Wong, Chin Lin, additional, Wu, Wai Ling K., additional, Yang, Hung-I, additional, Yoon, Ki Won, additional, Young, Edward, additional, Yu, Cyndia, additional, Zeng, Lingzhen, additional, Zhang, Cheng, additional, and Zhang, Silvia, additional

Published
2020
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19. Design and pre-flight performance of SPIDER 280 GHz receivers

Author

Shaw, E. C., primary, Ade, P.A.R., additional, Akers, S., additional, Amiri, M., additional, Austermann, Jason E., additional, Beall, James A., additional, Becker, D.T., additional, Benton, S.J., additional, Bergman, A. S., additional, Bock, J.J., additional, Bond, J.R., additional, Bryan, S.A., additional, Chiang, H.C., additional, Contaldi, C.R., additional, Domagalski, R.S., additional, Dore, O., additional, Duff, S. M., additional, Duivenvoorden, A.J., additional, Eriksen, H.K., additional, Farhang, M., additional, Filippini, J. P., additional, Fissel, L.M., additional, Fraisse, A.A., additional, Freese, K., additional, Galloway, M., additional, Gambrel, A. E., additional, Gandilo, N.N., additional, Ganga, K., additional, Grigorian, A., additional, Gualtieri, R, additional, Gudmundsson, J.E., additional, Halpern, M., additional, Hartley, J., additional, Hasselfield, M., additional, Hilton, G., additional, Holmes, W., additional, Hristov, V.V., additional, Huang, Z., additional, Hubmayr, Johannes, additional, Irwin, K.D., additional, Jones, W.C., additional, Kahn, A., additional, Kuo, C.L., additional, Kermish, Z.D., additional, Lennox, A., additional, Leung, J. S.-Y., additional, Megerian, K., additional, Reintsema, C., additional, Li, S., additional, Mason, P.V., additional, Runyan, M. C., additional, Moncelsi, L., additional, Morford, T.A., additional, Nagy, J.M., additional, Nie, R., additional, Mocanu, L. M., additional, Padilla, I.L., additional, Netterfield, C. B., additional, Osherson, B., additional, Rahlin, A.S., additional, Redmond, S., additional, Turner, A. D., additional, Romualdez, L.J., additional, Nolta, M., additional, Ruhl, J.E., additional, Shariff, J.A., additional, Shiu, C., additional, Soler, J.D., additional, Song, X., additional, Trangsrud, A., additional, Thommesen, H., additional, Tucker, C, additional, Tucker, R.S., additional, Ullom, Joel, additional, van der List, J.F., additional, Van Lanen, Jeff, additional, Vissers, M. R., additional, Weber, A. C., additional, Wen, S., additional, Wehus, I.K., additional, Wiebe, D.V., additional, and Young, E.Y., additional

Published
2020
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20. Thermal testing for cryogenic CMB instrument optical design

Author

Zmuidzinas, Jonas, Gao, Jian-Rong, Goldfinger, D. C., Ade, P.A.R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Beck, D., Bischoff, C. A., Bock, J. J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A. J., Denison, E. V., Dierickx, M. I., Duband, L., Eiben, M., Fatigoni, S., Filippini, J. P., Giannakopoulos, C., Goeckner-Wald, N., Grayson, J., Grimes, P. K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S. A., Henderson, S., Hildebrandt, S. R., Hilton, G. C., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Leitch, E. M., Lennox, A., Liu, T., Megerian, K. G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H. T., O'Brient, R., Palladino, S., Petroff, M. A., Prouvé, T., Pryke, C., Racine, B., Reintsema, C. D., Salatino, M., Schillaci, A., Schmitt, B. L., Singari, B., Soliman, A., Smith, A. G., St. Germaine, T., Steinbach, B., Sudiwala, R. V., Thompson, K. L., Tsai, C., Tucker, C., Turner, A. D., Umiltà, C., Verges, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, H., Yoon, K. W., Young, E., Yu, C., Zeng, L., Zhang, C., and Zhang, S.

Published
2022
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22. Observations of the temperature and polarization anisotropies with Boomerang 2003

Author

Jones, W.C., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C.R., Crill, B.P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A.H., Kisner, T.S., Lange, A.E., MacTavish, C.J., Masi, S., Mauskopf, P.D., Melchiorri, A., Montroy, T.E., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J.E., Santini, P., Tegmark, M., Veneziani, M., and Vittorio, N.

Published
2006
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23. APEX-SZ first light and instrument status

Author

Dobbs, M., Halverson, N.W., Ade, P.A.R., Basu, K., Beelen, A., Bertoldi, F., Cohalan, C., Cho, H.M., Güsten, R., Holzapfel, W.L., Kermish, Z., Kneissl, R., Kovács, A., Kreysa, E., Lanting, T.M., Lee, A.T., Lueker, M., Mehl, J., Menten, K.M., Muders, D., Nord, M., Plagge, T., Richards, P.L., Schilke, P., Schwan, D., Spieler, H., Weiss, A., and White, M.

Published
2006
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25. Fabrication of prototype imaging arrays for SCUBA-2

Author

Hilton, G.C., Beall, J.A., Doriese, W.B., Duncan, W.D., Ferreira, L.S., Irwin, K.D., Reintsema, C.D., Ullom, J.N., Vale, L.R., Xu, Y., Zink, B.L., Parkes, W., Bunting, A.S., Dunare, C.C., Gundlach, A.M., Stevenson, J.T.M., Walton, A.J., Schulte, E., Corrales, E., Sienicki, J.P., Bintley, Dan, Ade, P.A.R., Sudiwala, Rashmi V., Woodcraft, Adam L., Halpern, Mark, Holland, W., Audley, M.D., and MacIntosh, M.

Published
2006
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26. THE BOOMERANG/LDB INSTRUMENT

Author

PIACENTINI, F., primary, ADE, P.A.R., additional, BOCK, J.J., additional, BOSCALERI, A., additional, CARDONI, P., additional, COBLE, K., additional, CRILL, B.P., additional, DE BERNARDIS, P., additional, DE TROIA, G., additional, FARESE, P., additional, GIACOMETTI, M., additional, HIVON, E., additional, HRISTOV, V.V., additional, IACOANGELI, A., additional, LANGE, A.E., additional, MARTINIS, L., additional, MASI, S., additional, MASON, P.V., additional, MAUSKOPF, P.D., additional, MIGLIO, L., additional, MONTROY, T., additional, NETTERFIELD, C.B., additional, PASCALE, E., additional, PONGETTI, F., additional, ROMEO, G., additional, RUHL, J.E., additional, SCARAMUZZI, F., additional, and SFORNA, D., additional

Published
2002
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27. GALACTIC DUST CONTAMINATION IN THE BOOMERANG MAPS

Author

MASI, S., primary, ADE, P.A.R., additional, BOCK, J.J, additional, BOSCALERI, A., additional, CRILL, B.R, additional, DE BERNARDIS, P., additional, GIACOMETTI, M., additional, HIVON, E., additional, HRISTOV, V.V., additional, LANGE, A.E., additional, MAUSKOPF, P.D., additional, MONTROY, T., additional, NETTERFIELD, C.B., additional, PASCALE, E., additional, PIACENTINI, F., additional, PRUNET, S., additional, and RUHL, J., additional

Published
2002
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28. Transient response in doped germanium photoconductors under very low background operation

Author

Church, S.E., Price, M.C., Haegel, N.M., Griffin, M.J., and Ade, P.A.R.

Subjects
Photoconductivity -- Research, Photodetectors -- Research, Transients (Electricity) -- Research, Germanium -- Electric properties, Astronomy, Physics
Abstract

Doped germanium photoconductors are the most sensitive detectors for astronomy in the wavelength range 40-240 [[micro]meter]. Under the extremely low background conditions encountered in cooled satellite instruments, these devices exhibit a number of transient effects, such as slow relaxation after a step change in illumination or bias, and spontaneous spiking at high signal levels. Such behavior can degrade the excellent instantaneous sensitivity of these detectors and create calibration uncertainties. These effects have been observed in the Ge:Be photoconductors and the stressed and unstressed Ge:Ga photoconductors in the Long Wavelength Spectrometer, one of the instruments on the Infrared Space Observatory. A systematic investigation of the transient response of the Long Wavelength Spectrometer detectors to a step change in illumination as a function of operating temperature, bias electric field, and illumination step size has been carried out to determine operating conditions that minimize the effects of this behavior. The transient effects appear to be due primarily to carrier sweep out, but they are not fully explained by existing models for transient response.

Published
1996

29. SCUBA-2: A large-format TES array for submillimetre astronomy

Author

Audley, M.D, Holland, W.S, Duncan, W.D, Atkinson, D, Cliffe, M, Ellis, M, Gao, X, Gostick, D.C, Hodson, T, Kelly, D, MacIntosh, M.J, McGregor, H, Peacocke, T, Robson, I, Smith, I, Irwin, K.D, Hilton, G.C, Ullom, J.N, Walton, A, Dunare, C, Parkes, W, Ade, P.A.R, Bintley, D, Gannaway, F, Griffin, M, Pisano, G, Sudiwala, R.V, Walker, I, Woodcraft, A, Fich, M, Halpern, M, Mitchell, G, Naylor, D, and Bastien, P

Published
2004
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32. Design and performance of cryogenic, scanning Fabry-Perot interferometers for the long-wavelength spectrometer on the Infrared Space Observatory

Author

Davis, G.R., Furniss, I., Towlson, W.A., Ade, P.A.R., Emery, R.J., Glencross, W.M., Naylor, D. A., Patrick, T.J., Sidey, R.C., and Swinyard, B.M.

Subjects
Infrared astronomy -- Research, Infrared spectroscopy -- Research, Low temperatures -- Research, Capacitance meters -- Research, Interferometers -- Research, Astronomy, Physics
Abstract

The design of cryogenic, scanning Fabry-Perot interferometers for the Long-Wavelength Spectrometer on the ESA Infrared Space Observatory is presented. The interferometers were designed to provide a spectral resolving power of [10.sup.4] over the wavelength range 45-180 [[micro]meter], with the highest possible transmission efficiency consistent with this requirement. Metal meshes, custom designed with the aid of a theoretical model of metallic reflection, were used as the reflecting elements. The scanning mechanism featured a spring-suspended plate, which was servocontrolled by moving coil actuators and monitored by capacitance micrometers. The spectroscopic performance of the interferometers was measured in the laboratory and is compared with the model developed for the interferometer design. Although the measured resolving powers were somewhat lower than expected because of the laboratory measurement conditions, the transmission efficiencies were in approximate agreement with the design specification. Key words: Infrared Space Observatory, Long-Wavelength Spectrometer, Fabry-Perot, infrared, spectroscopy, cryogenic, mesh, capacitance micrometer.

Published
1995

33. Measuring CMB polarization with B oomerang

Author

Montroy, T, Ade, P.A.R, Balbi, A, Bock, J.J, Bond, J.R, Borrill, J, Boscaleri, A, Cabella, P, Contaldi, C.R, Crill, B.P, de Bernardis, P, De Gasperis, G, de Oliveira-Costa, A, De Troia, G, di Stefano, G, Ganga, K, Hivon, E, Hristov, V.V, Iacoangeli, A, Jaffe, A.H, Kisner, T.S, Jones, W.C, Lange, A.E, Masi, S, Mauskopf, P.D, MacTavish, C, Melchiorri, A, Nati, F, Natoli, P, Netterfield, C.B, Pascale, E, Piacentini, F, Pogosyan, D, Polenta, G, Prunet, S, Ricciardi, S, Romeo, G, Ruhl, J.E, Torbet, E, Tegmark, M, and Vittorio, N

Published
2003
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36. BOOMERANG returns

Author

Mauskopf, P.D., Ade, P.A.R., Balbi, A., Cabella, P., De Gasperis, G., Natoli, P., Vittorio, N., Bock, J.J., Hristov, V.V., Jones, W.C., Lange, A.E., Bond, J.R., Contaldi, C.R., J. Borrill, J., Boscaleri, A., Crill, B.P., de Bernardis, P., De Troia, G., Iacoangeli, A., Masi, S., Melchiorri, A., Nati, F., Piacentini, F., Polenta, G., Ricciardi, S., de Oliveira-Costa, A., Tegmark, M., di Stefano, G., Romeo, G., Ganga, K., Hivon, E., Jaffe, A.H., Ruhl, J.E., Kisner, T.S., Montroy, T., Torbet, E., Mactavish, C., Netterfield, C.B., Pascale, E., Pogosyan, D., and Prunet, S.

Published
2003
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37. Constraints on Primordial Gravitational Waves Using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season

Author

Ade, P.A.R, Ahmed, Z., Aikin, R.W., Alexander, K.D., Barkats, D., Benton, S.J., Bischoff, C.A., Bock, J.J., Bowens-Rubin, R., Brevik, J.A., Buder, I., Bullock, E., Buza, V., Connors, J., Cornelison, J., Crill, B.P., Crumrine, M., Dierickx, M., Duband, L., Dvorkin, C., Filippini, J.P., Fliescher, S., Grayson, J., Hall, G., Halpern, M., Harrison, S., Hildebrandt, S.R., Hilton, G.C., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Karpel, E., Kaufman, J.P., Keating, B.G., Kefeli, S., Kernasovskiy, S.A., Kovac, J.M., Kuo, C.L., Larsen, N.A., Lau, K., Leitch, E.M., Lueker, M., Megerian, K.G., Moncelsi, L., Namikawa, T., Netterfield, C.B., Nguyen, H.T., O'Brient, R., Ogburn, R.W., Palladino, S., Pryke, C., Racine, B., Richter, S., Schillaci, A., Schwarz, R., Sheehy, C.D., Soliman, A., St.Germaine, T., Staniszewski, Z.K., Steinbach, B., Sudiwala, R.V., Teply, G.P., Thompson, K.L., Tolan, J.E., Tucker, C., Turner, A.D., Umiltà, C., Vieregg, A.G., Wandui, A., Weber, A.C., Wiebe, D.V., Willmert, J., Wong, C.L., Wu, W.L.K., Yang, H., Yoon, K.W., and Zhang, C.

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We present results from an analysis of all data taken by the bicep2/Keck CMB polarization experiments up to and including the 2015 observing season. This includes the first Keck Array observations at 220 GHz and additional observations at 95 and 150 GHz. The Q and U maps reach depths of 5.2, 2.9, and 26 μK_{CMB} arcmin at 95, 150, and 220 GHz, respectively, over an effective area of ≈400 square degrees. The 220 GHz maps achieve a signal to noise on polarized dust emission approximately equal to that of Planck at 353 GHz. We take auto and cross spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz. We evaluate the joint likelihood of the spectra versus a multicomponent model of lensed-ΛCDM+r+dust+synchrotron+noise. The foreground model has seven parameters, and we impose priors on some of these using external information from Planck and WMAP derived from larger regions of sky. The model is shown to be an adequate description of the data at the current noise levels. The likelihood analysis yields the constraint r_{0.05}0.07 at 95% confidence, which tightens to r_{0.05}0.06 in conjunction with Planck temperature measurements and other data. The lensing signal is detected at 8.8σ significance. Running a maximum likelihood search on simulations we obtain unbiased results and find that σ(r)=0.020. These are the strongest constraints to date on primordial gravitational waves.

Published
2018

39. Exploring Cosmic Origins with CORE: Cluster Science

Author

Melin, J.-B., Bonaldi, A., Remazeilles, M., Hagstotz, S., Diego, J.M., Hernandez-Monteagudo, C., Genova-Santos, R.T., Luzzi, G., Martins, C.J.A.P., Grandis, S., Mohr, J.J., Bartlett, J.G., Delabrouille, J., Ferraro, S., Tramonte, D., Rubino-Martin, J.A., Macias-Perez, J.F., Achúcarro, A., Ade, P.A.R., Allison, R., Ashdown, M., Ballardini, M., Banday, A.J., Banerji, R., Bartolo, N., Basak, S., Baselmans, J., Basu, K., Battye, R.A., Baumann, D., Bersanelli, M., Bonato, M., Borrill, J., Bouchet, F.R., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Cai, Z.Y., Calvo, M., Carvalho, C.S., Castellano, M.G., Challinor, A., Chluba, J., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, Giuseppe, De Bernardis, P., de Gasperis, G., De Petris, M., de Zotti, G., Di Valentino, E., Errard, J., Forastieri, F., Galli, S., Gerbino, M., Gonzalez-Nuevo, J., Greenslade, J., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T.S., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Le Brun, A.M.C., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Lopez-Caniego, M., Maffei, B., Martinez-Gonzalez, E., Masi, S., McCarthy, D., Melchiorri, A., Molinari, D., Monfardini, A., Natoli, P., Negrello, M., Notari, A., Paiella, A., Paoletti, D., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Roman, M., Salvati, L., Tartari, A., Tomasi, M., Trappe, Neil, Triqueneaux, S., Trombetti, T., Tucker, C., Valiviita, J., van de Weygaert, R., Van Tent, B., Vennin, V., Vielva, P., Vittorio, N., Weller, J., Young, K., and Zannoni, M.

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics
Abstract

We examine the cosmological constraints that can be achieved with a galaxy cluster survey with the future CORE space mission. Using realistic simulations of the millimeter sky, produced with the latest version of the Planck Sky Model, we characterize the CORE cluster catalogues as a function of the main mission performance parameters. We pay particular attention to telescope size, key to improved angular resolution, and discuss the comparison and the complementarity of CORE with ambitious future ground-based CMB experiments that could be deployed in the next decade. A possible CORE mission concept with a 150 cm diameter primary mirror can detect of the order of 50,000 clusters through the thermal Sunyaev-Zeldovich effect (SZE). The total yield increases (decreases) by 25% when increasing (decreasing) the mirror diameter by 30 cm. The 150 cm telescope configuration will detect the most massive clusters (> 1014 M) at redshift z > 1.5 over the whole sky, although the exact number above this redshift is tied to the uncertain evolution of the cluster SZE flux-mass relation; assuming self-similar evolution, CORE will detect ∼ 500 clusters at redshift z > 1.5. This changes to 800 (200) when increasing (decreasing) the mirror size by 30 cm. CORE will be able to measure individual cluster halo masses through lensing of the cosmic microwave background anisotropies with a 1-σ sensitivity of 4 × 1014M, for a 120 cm aperture telescope, and 1014M for a 180 cm one. From the ground, we estimate that, for example, a survey with about 150,000 detectors at the focus of 350 cm telescopes observing 65% of the sky from Atacama would be shallower than CORE and detect about 11,000 clusters, while a survey from the South Pole with the same number of detectors observing 25% of sky with a 10 m telescope is expected to be deeper and to detect about 70,000 clusters. When combined with such a South Pole survey, CORE would reach a limiting mass of M500 ∼ 2 − 3 × 1013Mand detect 220,000 clusters (5 sigma detection limit). Cosmological constraints from CORE cluster counts alone are competitive with other scheduled large scale structure surveys in the 2020’s for measuring the dark energy equation-of-state parameters w0 and wa (σw0 = 0.28, σwa = 0.31). In combination with primary CMB constraints, CORE cluster counts can further reduce these error bars on w0 and wa to 0.05 and 0.13 respectively, and constrain the sum of the neutrino masses, Σmν, to 39 meV (1 sigma). The wide frequency coverage of CORE, 60 - 600 GHz, will enable measurement of the relativistic thermal SZE by stacking clusters. Contamination by dust emission from the clusters, however, makes constraining the temperature of the intracluster medium difficult. The kinetic SZE pairwise momentum will be extracted with S/N = 70 in the foreground-cleaned CMB map. Measurements of TCMB(z) using CORE clusters will establish competitive constraints on the evolution of the CMB temperature: (1+z) 1−β , with an uncertainty of σβ . 2.7×10−3 at low redshift (z . 1). The wide frequency coverage also enables clean extraction of a map of the diffuse SZE signal over the sky, substantially reducing contamination by foregrounds compared to the Planck SZE map extraction. Our analysis of the one-dimensional distribution of Compton-y values in the simulated map finds an order of magnitude improvement in constraints on σ8 over the Planck result, demonstrating the potential of this cosmological probe with CORE.

Published
2018

40. Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance

Author

Masi, S., primary, de Bernardis, P., additional, Paiella, A., additional, Piacentini, F., additional, Lamagna, L., additional, Coppolecchia, A., additional, Ade, P.A.R., additional, Battistelli, E.S., additional, Castellano, M.G., additional, Colantoni, I., additional, Columbro, F., additional, D'Alessandro, G., additional, Petris, M. De, additional, Gordon, S., additional, Magneville, C., additional, Mauskopf, P., additional, Pettinari, G., additional, Pisano, G., additional, Polenta, G., additional, Presta, G., additional, Tommasi, E., additional, Tucker, C., additional, Vdovin, V., additional, Volpe, A., additional, and Yvon, D., additional

Published
2019
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41. Erratum: Kinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization

Author

Paiella, A, primary, Coppolecchia, A, additional, Lamagna, L, additional, Ade, P.A.R, additional, Battistelli, E.S, additional, Castellano, M.G, additional, Colantoni, I, additional, Columbro, F, additional, D'Alessandro, G, additional, Bernardis, P. de, additional, Gordon, S, additional, Masi, S, additional, Mauskopf, P, additional, Pettinari, G, additional, Piacentini, F, additional, Pisano, G, additional, Presta, G, additional, and Tucker, C, additional

Published
2019
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42. Kinetic inductance detectors for the OLIMPO experiment: design and pre-flight characterization

Author

Paiella, A., primary, Coppolecchia, A., additional, Lamagna, L., additional, Ade, P.A.R., additional, Battistelli, E.S., additional, Castellano, M. G., additional, Colantoni, I., additional, Columbro, F., additional, D'Alessandro, G., additional, de Bernardis, P., additional, Gordon, S., additional, Masi, S., additional, Mauskopf, P., additional, Pettinari, G., additional, Piacentini, F., additional, Pisano, G., additional, Presta, G., additional, and Tucker, C., additional

Published
2019
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43. The new images of the microwave sky: a concordance cosmology ?

Author

de Bernardis, P., Ade, P.A.R., Bock, J.J., Bond, J.R., Borrill, J., Boscaleri, A., Coble, K., Contaldi, C.R., Crill, B.P., De Gasperis, G., De Troia, G., Farese, P., Ganga, K., Giacometti, M., Hivon, E., Hristov, V.V., Iacoangeli, A., Jaffe, A.H., Jones, W.C., Lange, A.E., Martinis, L., Mason, P., Mauskopf, P.D., Melchiorri, A., Montroy, T., Natoli, P., Netterfield, C.B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Pongetti, F., Prunet, S., Romeo, G., Ruhl, J.E., Scaramuzzi, F., and Vittorio, N.

Published
2002
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44. Planck 2015 results. V. LFI calibration

Author

Ade, P.A.R., Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartolo, N., Battaglia, P., Battaner, E., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.-F., Catalano, A., Chamballu, A., Christensen, P.R., Colombi, S., Colombo, L.P.L., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Eriksen, H.K., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Giard, M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D.L., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Juvela, M., Keskitalo, R., Kisner, T.S., Knoche, J., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leahy, J.P., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P.B., Lubin, P.M., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Masi, S., Matarrese, S., McGehee, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Montier, L., Morgante, G., Mortlock, D., Moss, Adam, Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Novikov, D., Novikov, I., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, T.J., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Pierpaoli, E., Pietrobon, D., Pointecouteau, E., Polenta, G., Pratt, G.W., Prunet, S., Puget, J.-L., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Romelli, E., Rosset, C., Rossetti, M., Roudier, G., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Stolyarov, V., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vassallo, T., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Watson, R., Wehus, I.K., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.

Subjects
data analysis, Astrophysics::Instrumentation and Methods for Astrophysics, instrumentation: polarimeters, Astrophysics::Cosmology and Extragalactic Astrophysics, cosmic background radiation, methods
Abstract

We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering four years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the cosmic microwave background dipole, but we now use the orbital component, rather than adopting the Wilkinson Microwave Anisotropy Probe (WMAP) solar dipole. This allows our 2015 LFI analysis to provide an independent Solar dipole estimate, which is in excellent agreement with that of HFI and within 1? (0.3% in amplitude) of the WMAP value. This 0.3% shift in the peak-to-peak dipole temperature from WMAP and a general overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45% (30?GHz), 0.64% (44?GHz), and 0.82% (70?GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is now at the level of 0.20% for the 70?GHz map, 0.26% for the 44?GHz map, and 0.35% for the 30?GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.

Published
2016

45. Planck 2015 results XXVII. The second Planck catalogue of Sunyaev-Zeldovich sources

Author

Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Barrena, R., Bartlett, J.G., Bartolo, N., Battaner, E., Battye, R., Benabed, K., Benoit, A., Benoit-Lévy, A., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bikmaev, I., Böhringer, H., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Bucher, M., Burenin, R., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.-F., Carvalho, P., Catalano, A., Challinor, A., Chamballu, A., Chary, R.-R., Chiang, H.C., Chon, G., Christensen, P.R., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Dahle, H., Danese, L., Davies, R.D., Davis, R.J., De Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Desert, F.-X., Dickinson, C., Diego, J.M., Dolag, K., Dole, H., Donzelli, S., Dore, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Eisenhardt, P., Elsner, F., Enßlin, T.A., Eriksen, H.K., Falgarone, E., Fergusson, J., Feroz, F., Ferragamo, A., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Genova-Santos, R.T., Giard, M., Giraud-Héraud, Y., Gjerløw, E., Gonzalez-Nuevo, J., Gorski, K.M., Grainge, K.J.B., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Hanson, D., Harrison, D., Hempel, A., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jin, T., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Khamitov, I., Kisner, T.S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maggio, G., Maino, D., Mak, D.S.Y., Mandolesi, N., Mangilli, A., Martin, P.G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., McGehee, P., Mei, S., Melchiorri, A., Melin, J.-B., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J.Anthony, Naselsky, P., Nastasi, A., Nati, F., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Olamaie, M., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Patanchon, G., Pearson, T.J., Perdereau, O., Perotto, L., Perrott, Y.C., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G.W., Prezeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rozo, E., Rubino-Martin, J.A., Rumsey, C., Rusholme, B., Rykoff, E.S., Sandri, M., Santos, D., Saunders, R.D.E., Savelainen, M., Savini, G., Schammel, M.P., Scott, D., Seiffert, M.D., Shellard, E.P.S., Shimwell, T.W., Spencer, L., Stanford, S.A., Stern, A., Stolyarov, V., Stompor, R., Streblyanska, A., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tramonte, D., Tristram, M., Tucci, M., Tuovinen, J., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Wehus, I., White, S.D.M., Wright, E.L., Yvon, D., Zacchei, A., Zonca, A., Science and Technology Facilities Council (STFC), Imperial College Trust, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Barrena, R., Bartlett, J. G., Bartolo, N., Battaner, E., Battye, R., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bikmaev, I., Böhringer, H., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bucher, M., Burenin, R., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. F., Carvalho, P., Catalano, A., Challinor, A., Chamballu, A., Chary, R. R., Chiang, H. C., Chon, G., Christensen, P. R., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Dahle, H., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Désert, F. X., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, Simona, Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Eisenhardt, P. R. M., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Fergusson, J., Feroz, F., Ferragamo, A., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Génova Santos, R. T., Giard, M., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Grainge, K. J. B., Gratton, S., Gregorio, Anna, Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Hanson, D., Harrison, D. L., Hempel, A., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jin, T., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Khamitov, I., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki Suonio, H., Lagache, G., Lamarre, J. M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P. B., Linden Vørnle, M., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maggio, G., Maino, D., Mak, D. S. Y., Mandolesi, N., Mangilli, A., Martin, P. G., Martínez González, E., Masi, S., Matarrese, S., Mazzotta, P., Mcgehee, P., Mei, S., Melchiorri, A., Melin, J. B., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Miville Deschênes, M. A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nastasi, A., Nati, F., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Olamaie, M., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Patanchon, G., Pearson, T. J., Perdereau, O., Perotto, L., Perrott, Y. C., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rozo, E., Rubinõ Martín, J. A., Rumsey, C., Rusholme, B., Rykoff, E. S., Sandri, M., Santos, D., Saunders, R. D. E., Savelainen, M., Savini, G., Schammel, M. P., Scott, D., Seiffert, M. D., Shellard, E. P. S., Shimwell, T. W., Spencer, L. D., Stanford, S. A., Stern, D., Stolyarov, V., Stompor, R., Streblyanska, A., Sudiwala, R., Sunyaev, R., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tramonte, D., Tristram, M., Tucci, M., Tuovinen, J., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., White, S. D. M., Wright, E. L., Yvon, D., Zacchei, A., Zonca, A., Ade, P, Aghanim, N, Arnaud, M, Ashdown, M, Aumont, J, Baccigalupi, C, Banday, A, Barreiro, R, Barrena, R, Bartlett, J, Bartolo, N, Battaner, E, Battye, R, Benabed, K, Benoît, A, Benoit Lévy, A, Bernard, J, Bersanelli, M, Bielewicz, P, Bikmaev, I, Böhringer, H, Bonaldi, A, Bonavera, L, Bond, J, Borrill, J, Bouchet, F, Bucher, M, Burenin, R, Burigana, C, Butler, R, Calabrese, E, Cardoso, J, Carvalho, P, Catalano, A, Challinor, A, Chamballu, A, Chary, R, Chiang, H, Chon, G, Christensen, P, Clements, D, Colombi, S, Colombo, L, Combet, C, Comis, B, Couchot, F, Coulais, A, Crill, B, Curto, A, Cuttaia, F, Dahle, H, Danese, L, Davies, R, Davis, R, DE BERNARDIS, P, De Rosa, A, De Zotti, G, Delabrouille, J, Désert, F, Dickinson, C, Diego, J, Dolag, K, Dole, H, Donzelli, S, Doré, O, Douspis, M, Ducout, A, Dupac, X, Efstathiou, G, Eisenhardt, P, Elsner, F, Enßlin, T, Eriksen, H, Falgarone, E, Fergusson, J, Feroz, F, Ferragamo, A, Finelli, F, Forni, O, Frailis, M, Fraisse, A, Franceschi, E, Frejsel, A, Galeotta, S, Galli, S, Ganga, K, Génova Santos, R, Giard, M, Giraud Héraud, Y, Gjerløw, E, González Nuevo, J, Górski, K, Grainge, K, Gratton, S, Gregorio, A, Gruppuso, A, Gudmundsson, J, Hansen, F, Hanson, D, Harrison, D, Hempel, A, Henrot Versillé, S, Hernández Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Hobson, M, Holmes, W, Hornstrup, A, Hovest, W, Huffenberger, K, Hurier, G, Jaffe, A, Jaffe, T, Jin, T, Jones, W, Juvela, M, Keihänen, E, Keskitalo, R, Khamitov, I, Kisner, T, Kneissl, R, Knoche, J, Kunz, M, Kurki Suonio, H, Lagache, G, Lamarre, J, Lasenby, A, Lattanzi, M, Lawrence, C, Leonardi, R, Lesgourgues, J, Levrier, F, Liguori, M, Lilje, P, Linden Vørnle, M, López Caniego, M, Lubin, P, Maciás Pérez, J, Maggio, G, Maino, D, Mak, D, Mandolesi, N, Mangilli, A, Martin, P, Martínez González, E, Masi, S, Matarrese, S, Mazzotta, P, Mcgehee, P, Mei, S, Melchiorri, A, Melin, J, Mendes, L, Mennella, A, Migliaccio, M, Mitra, S, Miville Deschênes, M, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Murphy, J, Naselsky, P, Nastasi, A, Nati, F, Natoli, P, Netterfield, C, Nørgaard Nielsen, H, Noviello, F, Novikov, D, Novikov, I, Olamaie, M, Oxborrow, C, Paci, F, Pagano, L, Pajot, F, Paoletti, D, Pasian, F, Patanchon, G, Pearson, T, Perdereau, O, Perotto, L, Perrott, Y, Perrotta, F, Pettorino, V, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Pratt, G, Prézeau, G, Prunet, S, Puget, J, Rachen, J, Reach, W, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Renzi, A, Ristorcelli, I, Rocha, G, Rosset, C, Rossetti, M, Roudier, G, Rozo, E, Rubinõ Martín, J, Rumsey, C, Rusholme, B, Rykoff, E, Sandri, M, Santos, D, Saunders, R, Savelainen, M, Savini, G, Schammel, M, Scott, D, Seiffert, M, Shellard, E, Shimwell, T, Spencer, L, Stanford, S, Stern, D, Stolyarov, V, Stompor, R, Streblyanska, A, Sudiwala, R, Sunyaev, R, Sutton, D, Suur Uski, A, Sygnet, J, Tauber, J, Terenzi, L, Toffolatti, L, Tomasi, M, Tramonte, D, Tristram, M, Tucci, M, Tuovinen, J, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Wade, L, Wandelt, B, Wehus, I, White, S, Wright, E, Yvon, D, Zacchei, A, Zonca, A, Ministerio de Economía y Competitividad (España), European Space Agency, Centre National de la Recherche Scientifique (France), Istituto Nazionale di Astrofisica, National Aeronautics and Space Administration (US), Science and Technology Facilities Council (UK), Academy of Finland, Center for Science (Finland), Agenzia Spaziale Italiana, Department of Energy (US), UK Space Agency, Fundação para a Ciência e a Tecnologia (Portugal), Science Foundation Ireland, DTU Space (Denmark), Swiss Space Office, Max Planck Society, German Centre for Air and Space Travel, European Commission, Consejo Superior de Investigaciones Científicas (España), Junta de Andalucía, European Research Council, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Planck, Hélium : du fondamental aux applications (HELFA), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Library science, FOS: Physical sciences, observation [Cosmology], Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Astronomy & Astrophysics, clusters: general [Galaxies], Cosmology: observation, 01 natural sciences, NO, Physics::Geophysics, Methods statistical, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Statistical analysis, observations [Cosmology], GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, cosmology: observations, galaxies: clusters: general, catalogs, Astrophysics - Cosmology and Nongalactic Astrophysics, Physics, Diffuse radiation, observations, galaxies: clusters: general, catalogs [cosmology], 010308 nuclear & particles physics, 4. Education, Cosmology: observations, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Astronomy and Astrophysic, Catalogues, 0201 Astronomical And Space Sciences, Space and Planetary Science, Energy density, astro-ph.CO, Catalog, Galaxies: clusters: general, Catalogs
Abstract

Acknowledgements. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/planck-collaboration. We thank Ian McCarthy for providing images and profiles of simulated clusters from cosmo-OWLS. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and the SIMBAD database, operated at CDS, Strasbourg, France This research made use of data retrieved from SDSS-III. Funding for SDSSIII has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science; the SDSS-III web site is http://www.sdss3.org/. This research has made use of data processed by the Centre d’Analyse de Données Étendues (http://cade.irap.omp.eu/) and has made use of the HEALPix pixelization software (http://healpix.sourceforge.net; Górski et al. 2005). Some of this work was performed using the Darwin Supercomputer of the University of Cambridge High Performance Computing Service (http: //www.hpc.cam.ac.uk/), provided by Dell Inc. using Strategic Research Infrastructure Funding from the Higher Education Funding Council for England and funding from the Science and Technology Facilities Council., We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest systematic all-sky surveyof galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data sets, and is the first SZ-selected cluster survey containing >103 confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the estimates of the SZ strength parameter Y5R500are robust to pressure-profile variation and beam systematics, but accurate conversion to Y500 requires the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical, and X-ray data sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under-luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples., European Space Agency, Centre National D'etudes Spatiales, CNRS/INSU-IN2P3-INP (France), Italian Space Agency (ASI), Italian National Research Council, Istituto Nazionale Astrofisica (INAF), National Aeronautics & Space Administration (NASA), Max Planck Society, CSA (Canada), DTU Space (Denmark), SER/SSO (Switzerland), RCN (Norway), Science Foundation Ireland, Portuguese Foundation for Science and Technology, ERC (EU), European Union (EU), Higher Education Funding Council for England, Alfred P. Sloan Foundation, National Science Foundation (NSF), United States Department of Energy (DOE), Science & Technology Facilities Council (STFC) ST/F01239X/1 ST/L000393/1 ST/K001051/1 ST/K004131/1 ST/L000768/1 ST/N001206/1 ST/M001172/1 ST/H001239/1

Published
2016

46. Planck 2015 results. IV. Low Frequency Instrument beams and window functions

Author

Ade, P.A.R., Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartolo, N., Battaner, E., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.-F., Catalano, A., Chamballu, A., Christensen, P.R., Colombi, S., Colombo, L.P.L., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Eriksen, H.K., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Giard, M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D.L., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Juvela, M., Keskitalo, R., Kiiveri, K., Kisner, T.S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P.B., Lindholm, V., Lubin, P.M., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Masi, S., Matarrese, S., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Montier, L., Morgante, G., Mortlock, D., Moss, Adam, Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Novikov, D., Novikov, I., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Pierpaoli, E., Pietrobon, D., Pointecouteau, E., Polenta, G., Pratt, G.W., Prunet, S., Puget, J.-L., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Stolyarov, V., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vassallo, T., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Watson, R., Wehus, I.K., Yvon, D., Zacchei, A., and Zonca, A.

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Physics::Accelerator Physics, telescopes, cosmic background radiation, methods: data analysis
Abstract

This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. The in-flight assessment of the LFI main beams relies on measurements performed during observations of Jupiter. By stacking data from seven Jupiter transits, the main beam profiles are measured down to –25 dB at 30 and 44 GHz, and down to –30 dB at 70 GHz. It has been confirmed that the agreement between the simulated beams and the measured beams is better than 1% at each LFI frequency band (within the 20 dB contour from the peak, the rms values are 0.1% at 30 and 70 GHz; 0.2% at 44 GHz). Simulated polarized beams are used for the computation of the effective beam window functions. The error budget for the window functions is estimated from both main beam and sidelobe contributions, and accounts for the radiometer band shapes. The total uncertainties in the effective beam window functions are 0.7% and 1% at 30 and 44 GHz, respectively (at ℓ ≈ 600); and 0.5% at 70 GHz (at ℓ ≈ 1000).

Published
2016

47. BICEP array cryostat and mount design

Author

Crumrine, Michael, primary, Ade, P.A.R., primary, Ahmed, Zeeshan, primary, Aikin, Randol, primary, Alexander, Kate D., primary, Barkats, Denis, primary, Benton, Steve J., primary, Bischoff, Colin, primary, Bock, James J., primary, Bowens-Rubin, Rachel, primary, Brevik, Justus A., primary, Buder, Immanuel, primary, Bullock, Eric, primary, Buza, Victor, primary, Connors, Jake, primary, Cornelison, James, primary, Crill, Bendan, primary, Dierickx, Marion, primary, Duband, Lionel, primary, Dvorkin, Cora, primary, Filippini, Jeff P., primary, Fliescher, Stefan, primary, Grayson, James A., primary, Hall, Grantland, primary, Halpern, Mark, primary, Harrison, Sam A., primary, Hildebrandt, Sergi, primary, Hilton, Gene C., primary, Hui, Howard, primary, Irwin, Kent D., primary, Kang, Jae Hwan, primary, Karkare, Kirit S., primary, Karpel, Ethan, primary, Kaufman, Jonathan, primary, Keating, Brian, primary, Kefeli, Sinan, primary, Kernasovskiy, Sarah A., primary, Kovac, J. M., primary, Kuo, Chao-lin, primary, Larson, Nicole, primary, Lau, King, primary, Leitch, Erik M., primary, Lueker, Martin, primary, Wiebe, Don, primary, Megerian, Koko. G., primary, Moncelsi, Lorenzo, primary, Namikawa, Toshiya, primary, Netterfield, C. B., primary, Nguyen, H. T., primary, O'brient, Roger, primary, Ogburn IV, R. Walt, primary, Palladino, Steven, primary, Pryke, Clement, primary, Racine, Benjamin, primary, Richter, Steffen, primary, Schillaci, Alessandro, primary, Schwarz, Robert, primary, Sheehy, Chris D., primary, Soliman, Ahmed, primary, St Germaine, Tyler, primary, Staniszewski, Zachary K., primary, Steinbach, Bryan, primary, Sudiwala, Rashmi, primary, Teply, Grant P., primary, Thompson, Keith L., primary, Tolan, James E., primary, Tucker, Carole, primary, Turner, Anthony D., primary, Umiltà, Caterina, primary, Vieregg, Abigail G., primary, Wandui, Albert, primary, Weber, Alexis C., primary, Willmer, Justin, primary, Wong, Chin Lin, primary, Wu, Wai Ling K., primary, Yang, Hung-I, primary, Yoon, Ki Won, primary, and Zhang, Cheng, primary

Published
2018
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48. Exploring cosmic origins with CORE: The instrument

Author

de Bernardis, P., primary, Ade, P.A.R., additional, Baselmans, J.J.A., additional, Battistelli, E.S., additional, Benoit, A., additional, Bersanelli, M., additional, Bideaud, A., additional, Calvo, M., additional, Casas, F.J., additional, Castellano, M.G., additional, Catalano, A., additional, Charles, I., additional, Colantoni, I., additional, Columbro, F., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, Petris, M. De, additional, Delabrouille, J., additional, Doyle, S., additional, Franceschet, C., additional, Gomez, A., additional, Goupy, J., additional, Hanany, S., additional, Hills, M., additional, Lamagna, L., additional, Macias-Perez, J., additional, Maffei, B., additional, Martin, S., additional, Martinez-Gonzalez, E., additional, Masi, S., additional, McCarthy, D., additional, Mennella, A., additional, Monfardini, A., additional, Noviello, F., additional, Paiella, A., additional, Piacentini, F., additional, Piat, M., additional, Pisano, G., additional, Signorelli, G., additional, Tan, C.Y., additional, Tartari, A., additional, Trappe, N., additional, Triqueneaux, S., additional, Tucker, C., additional, Vermeulen, G., additional, Young, K., additional, Zannoni, M., additional, Achúcarro, A., additional, Allison, R., additional, Artall, E., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.Y., additional, Carvalho, C.S., additional, Challinor, A., additional, Chluba, J., additional, Clesse, S., additional, Gasperis, G. De, additional, Zotti, G. De, additional, Valentino, E. Di, additional, Diego, J.M., additional, Errard, J., additional, Feeney, S., additional, Fernandez-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Génova-Santos, R., additional, Gerbino, M., additional, González-Nuevo, J., additional, Hagstotz, S., additional, Greenslade, J., additional, Handley, W., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lasenby, A., additional, Lattanzi, M., additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Luzzi, G., additional, Martins, C.J.A.P., additional, Matarrese, S., additional, Melchiorri, A., additional, Melin, J.B., additional, Molinari, D., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Paoletti, D., additional, Patanchon, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rubiño-Martín, J.A., additional, Salvati, L., additional, Tomasi, M., additional, Tramonte, D., additional, Trombetti, T., additional, Väliviita, J., additional, de Weyjgaert, R. Van, additional, Tent, B. van, additional, Vennin, V., additional, Vielva, P., additional, and Vittorio, N., additional

Published
2018
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49. Mapping the CMB sky: THE BOOMERanG experiment

Author

de Bernardis, P., Ade, P.A.R., Artusa, R., Bock, J.J., Boscaleri, A., Crill, B.P., De Troia, G., Farese, P.C., Giacometti, M., Hristov, V.V., Iacoangeli, A., Lange, A.E., Lee, A.T., Masi, S., Martinis, L., Mason, P.V., Mauskopf, P.D., Melchiorri, F., Miglio, L., Montroy, T., Netterfield, C.B., Pascale, E., Piacentini, F., Richards, P.L., Ruhl, J.E., and Scaramuzzi, F.

Published
1999
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50. Planck intermediate results. VIII. Filaments between interacting clusters

Author

Bartlett, J.G., Cardoso, J.-F., Castex, G., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Le Jeune, M., Patanchon, G., Piat, M., Remazeilles, M., Roman, M., Rosset, C., Smoot, G.F., Poutanen, T., Bikmaev, I., Natoli, P., Polenta, G., Mandolesi, N., Ashdown, M., Hobson, M., Lasenby, A., Bhatia, R., Kneissl, R., Bond, J.R., Miville-Deschênes, M.-A., Banday, A.J., Bernard, J.-P., Flores-Cacho, I., Forni, O., Giard, M., Jaffe, T.R., Montier, L., Pointecouteau, E., Ristorcelli, I., Doré, O., Hildebrandt, S.R., Mei, S., Rocha, G., Dahle, H., Lilje, P.B., Da Silva, A., Hernández-Monteagudo, C., Borrill, J., Rebolo, R., Melin, J.-B., Piffaretti, R., Yvon, D., Linden-Vørnle, Michael, Nørgaard-Nielsen, Hans Ulrik, Frommert, M., Kunz, M., Atrio-Barandela, F., Toffolatti, L., Rachen, J.P., Scott, D., Colombo, L.P.L., Pierpaoli, E., Juvela, M., Kurki-Suonio, H., Suur-Uski, A.-S., Jones, W.C., Knox, L., Lubin, P.M., Zonca, A., Wandelt, B.D., Cayón, L., Matarrese, S., De Bernardis, P., Masi, S., Melchiorri, A., Nati, F., Piacentini, F., Bersanelli, M., Maino, D., Mennella, A., Rossetti, M., Gregorio, A., Burigana, C., Balbi, A., Bourdin, H., De Gasperis, G., Mazzotta, P., Vittorio, N., Cabella, P., Christensen, P.R., Naselsky, P., Hempel, A., Rubiño-Martín, J.A., Dupac, X., Jagemann, T., Leonardi, R., Mendes, L., Tauber, J.A., De Zotti, G., Colafrancesco, S., Frailis, M., Galeotta, S., Maris, M., Pasian, F., Zacchei, A., Massardi, M., Cuttaia, F., Finelli, F., Franceschi, E., Gruppuso, A., Morgante, G., Paoletti, D., Ricciardi, S., Sandri, M., Terenzi, L., Valenziano, L., Villa, F., Donzelli, S., Tomasi, M., Désert, F.-X., Ponthieu, N., Mitra, S., Chamballu, A., Clements, D.L., Jaffe, A.H., Novikov, D., Chary, R.-R., Rusholme, B., Benoît, A., Dole, H., Aghanim, N., Aumont, J., Douspis, M., Lagache, G., Pajot, F., Puget, J.-L., Welikala, N., Benabed, K., Bouchet, F.R., Hivon, E., Moneti, A., Prunet, S., Sygnet, J.-F., Popa, L., Marleau, F., Chiang, L.-Y., Efstathiou, G., Harrison, D., Sutton, D., Eriksen, H.K., Hansen, F.K., Génova-Santos, R.T., Barreiro, R.B., Diego, J.M., González-Nuevo, J., Herranz, D., López-Caniego, M., Martínez-González, E., Vielva, P., Crill, B.P., Górski, K.M., Holmes, W.A., Lawrence, C.R., Wade, L.A., Bonaldi, A., Davis, R.J., Maffei, B., Noviello, F., Henrot-Versillé, S., Luzzi, G., Perdereau, O., Plaszczynski, S., Tristram, M., Catalano, A., Coulais, A., Lamarre, J.-M., Arnaud, M., Démoclès, J., Marshall, D.J., Pratt, G.W., Starck, J.-L., Comis, B., Hurier, G., MacÍas-Pérez, J.F., Perotto, L., Renault, C., Van Tent, B., Kisner, T.S., Dolag, K., Dörl, U., Enßlin, T.A., Gilfanov, M., Hovest, W., Knoche, J., Matthai, F., Reinecke, M., Riller, T., Sunyaev, R., White, S.D.M., Böhringer, H., Chon, G., Murphy, J.A., Novikov, I., Savini, G., Baccigalupi, C., Danese, L., Perrotta, F., Ade, P.A.R., Munshi, D., Sudiwala, R., Burenin, R., Osborne, S., Khamitov, I., Schaefer, B.M., Battaner, E., Department of Physics, Helsinki Institute of Physics, lanck Collaboration: P. A. R., Ade, N., Aghanim, M., Arnaud, M., Ashdown, F., Atrio Barandela, J., Aumont, C., Baccigalupi, Balbi, . A., A. J., Banday, R. B., Barreiro, J. G., Bartlett, E., Battaner, K., Benabed, A., Benoˆıt, J. P., Bernard, M., Bersanelli, R., Bhatia, I., Bikmaev, H., Bo ̈hringer, A., Bonaldi, J. R., Bond, J., Borrill, F. R., Bouchet, H., Bourdin, R., Burenin, Burigana, . C., P., Cabella, J. F., Cardoso, G., Castex, A., Catalano, L., Cayo ́n, A., Chamballu, R. R., Chary, L. Y., Chiang, G., Chon, P. R., Christensen, D. L., Clement, S., Colafrancesco, L. P. L., Colombo, B., Comi, A., Coulai, B. P., Crill, Cuttaia, . F., A., Da Silva, H., Dahle, L., Danese, R. J., Davi, P., de Bernardi, G., de Gasperi, G., de Zotti, J., Delabrouille, De ́mocle`s, . J., F. X., De ́sert, J. M., Diego, K., Dolag, H., Dole, S., Donzelli, O., Dore ́, U., Do ̈rl, M., Douspi, X., Dupac, Efstathiou, . G., T. A., Enßlin, H. K., Eriksen, F., Finelli, I., Flores Cacho, O., Forni, M., Fraili, E., Franceschi, M., Frommert, Galeotta, . S., K., Ganga, R. T., Ge ́nova Santo, M., Giard, M., Gilfanov, Y., Giraud He ́raud, J., Gonza ́lez Nuevo, K. M., Go ́rski, Gregorio, Anna, A., Gruppuso, F. K., Hansen, D., Harrison, A., Hempel, S., Henrot Versille ́, C., Herna ́ndez Monteagudo, Herranz, . D., S. R., Hildebrandt, E., Hivon, M., Hobson, W. A., Holme, W., Hovest, G., Hurier⋆⋆, T. R., Jaffe, A. H., Jaffe, Jagemann, . T., W. C., Jone, M., Juvela, I., Khamitov, T. S., Kisner, R., Kneissl, J., Knoche, L., Knox, M., Kunz, Kurki Suonio, . H., G., Lagache, J. M., Lamarre, A., Lasenby, C. R., Lawrence, M., Le Jeune, R., Leonardi, P. B., Lilje, Linden Vørnle, . M., M., Lo ́pez Caniego, P. M., Lubin, G., Luzzi, J. F., Mac ́ıas Pe ́rez, B., Maffei, D., Maino, N., Mandolesi, Maris, . M., F., Marleau, D. J., Marshall, E., Mart ́ınez Gonza ́lez, S., Masi, M., Massardi, S., Matarrese, F., Matthai, P., Mazzotta, Mei, . S., A., Melchiorri, J. B., Melin, L., Mende, A., Mennella, S., Mitra, M. A., Miville Descheˆne, A., Moneti, Montier, . L., G., Morgante, D., Munshi, J. A., Murphy, P., Naselsky, F., Nati, P., Natoli, H. U., Nørgaard Nielsen, F., Noviello, D., Novikov, I., Novikov, S., Osborne, F., Pajot, D., Paoletti, F., Pasian, G., Patanchon, O., Perdereau, L., Perotto, F., Perrotta, Piacentini, . F., M., Piat, E., Pierpaoli, R., Piffaretti, S., Plaszczynski, E., Pointecouteau, G., Polenta, N., Ponthieu, L., Popa, Poutanen, . T., G. W., Pratt, S., Prunet, J. L., Puget, J. P., Rachen, R., Rebolo, M., Reinecke, M., Remazeille, C., Renault, S., Ricciardi, T., Riller, I., Ristorcelli, G., Rocha, M., Roman, C., Rosset, M., Rossetti, J. A., Rubin ̃o Mart ́ın, B., Rusholme, M., Sandri, G., Savini, B. M., Schaefer, D., Scott, G. F., Smoot, J. L., Starck, R., Sudiwala, R., Sunyaev, D., Sutton, A. S., Suur Uski, J. F., Sygnet, J. A., Tauber, L., Terenzi, L., Toffolatti, M., Tomasi, M., Tristram, L., Valenziano, B., Van Tent, P., Vielva, F., Villa, N., Vittorio, L. A., Wade, B. D., Wandelt, N., Welikala, S. D. M., White, D., Yvon, A., Zacchei, A., Zonca, Universidad de Cantabria, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), PLANCK, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), HELFA - Hélium : du fondamental aux applications, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Collaboration, P, Ade, P, Aghanim, N, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Balbi, A, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Bernard, J, Bersanelli, M, Bhatia, R, Bikmaev, I, Bohringer, H, Bonaldi, A, Bond, J, Borrill, J, Bouchet, F, Bourdin, H, Burenin, R, Burigana, C, Cabella, P, Cardoso, J, Castex, G, Catalano, A, Cayon, L, Chamballu, A, Chary, R, Chiang, L, Chon, G, Christensen, P, Clements, D, Colafrancesco, S, Colombo, L, Comis, B, Coulais, A, Crill, B, Cuttaia, F, Da Silva, A, Dahle, H, Danese, L, Davis, R, De Bernardis, P, De Gasperis, G, De Zotti, G, Delabrouille, J, Democles, J, Desert, F, Diego, J, Dolag, K, Dole, H, Donzelli, S, Dore, O, Dorl, U, Douspis, M, Dupac, X, Efstathiou, G, Ensslin, T, Eriksen, H, Finelli, F, Flores-Cacho, I, Forni, O, Frailis, M, Franceschi, E, Frommert, M, Galeotta, S, Ganga, K, Genova-Santos, R, Giard, M, Gilfanov, M, Giraud-Heraud, Y, Gonzalez-Nuevo, J, Gorski, K, Gregorio, A, Gruppuso, A, Hansen, F, Harrison, D, Hempel, A, Henrot-Versille, S, Hernandez-Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Hobson, M, Holmes, W, Hovest, W, Hurier, G, Jaffe, T, Jaffe, A, Jagemann, T, Jones, W, Juvela, M, Khamitov, I, Kisner, T, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamarre, J, Lasenby, A, Lawrence, C, Le Jeune, M, Leonardi, R, Lilje, P, Linden-Vørnle, M, Linden-Vornle, M, Lopez-Caniego, M, Lubin, P, Luzzi, G, Macias-Perez, J, Maffei, B, Maino, D, Mandolesi, N, Maris, M, Marleau, F, Marshall, D, Martinez-Gonzalez, E, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Mei, S, Melchiorri, A, Melin, J, Mendes, L, Mennella, A, Mitra, S, Miville-Deschenes, M, Moneti, A, Montier, L, Morgante, G, Munshi, D, Murphy, J, Naselsky, P, Nati, F, Natoli, P, Nørgaard-Nielsen, H, Norgaard-Nielsen, H, Noviello, F, Novikov, D, Novikov, I, Osborne, S, Pajot, F, Paoletti, D, Pasian, F, Patanchon, G, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piffaretti, R, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G, Prunet, S, Puget, J, Rachen, J, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Riller, T, Ristorcelli, I, Rocha, G, Roman, M, Rosset, C, Rossetti, M, Rubino-Martin, J, Rusholme, B, Sandri, M, Savini, G, Schaefer, B, Scott, D, Smoot, G, Starck, J, Sudiwala, R, Sunyaev, R, Sutton, D, Suur-Uski, A, Sygnet, J, Tauber, J, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Valenziano, L, Van Tent, B, Vielva, P, Villa, F, Vittorio, N, Wade, L, Wandelt, B, Welikala, N, White, S, Yvon, D, Zacchei, A, Zonca, A, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)

Subjects
clusters:general [galaxies], Cosmology and Nongalactic Astrophysics (astro-ph.CO), Large-scale structure of Universe, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Astrophysics::High Energy Astrophysical Phenomena, education, galaxies:clusters:general, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, clusters: general [Galaxies], Hadrons, 7. Clean energy, 01 natural sciences, Virial theorem, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, ROSAT, Thermal, Cluster (physics), Planck, Planck ESA mission, 010303 astronomy & astrophysics, Galaxy cluster, Astrophysics::Galaxy Astrophysics, Galaxies: clusters: general, Physics, X rays, 010308 nuclear & particles physics, Astronomy and Astrophysics, 115 Astronomy, Space science, Galaxies, Galaxy, Baryon, galaxies: clusters: general, galaxies: clusters: general / large-scale structure of universe, large-scale structure of universe, Space and Planetary Science, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

[Context]: About half of the baryons of the Universe are expected to be in the form of filaments of hot and low-density intergalactic medium. Most of these baryons remain undetected even by the most advanced X-ray observatories, which are limited in sensitivity to the diffuse low-density medium. [Aims]: The Planck satellite has provided hundreds of detections of the hot gas in clusters of galaxies via the thermal Sunyaev-Zel'dovich (tSZ) effect and is an ideal instrument for studying extended low-density media through the tSZ effect. In this paper we use the Planck data to search for signatures of a fraction of these missing baryons between pairs of galaxy clusters. [Methods]: Cluster pairs are good candidates for searching for the hotter and denser phase of the intergalactic medium (which is more easily observed through the SZ effect). Using an X-ray catalogue of clusters and the Planck data, we selected physical pairs of clusters as candidates. Using the Planck data, we constructed a local map of the tSZ effect centred on each pair of galaxy clusters. ROSAT data were used to construct X-ray maps of these pairs. After modelling and subtracting the tSZ effect and X-ray emission for each cluster in the pair, we studied the residuals on both the SZ and X-ray maps. [Results]: For the merging cluster pair A399-A401 we observe a significant tSZ effect signal in the intercluster region beyond the virial radii of the clusters. A joint X-ray SZ analysis allows us to constrain the temperature and density of this intercluster medium. We obtain a temperature of kT = 7.1 ± 0.9 keV (consistent with previous estimates) and a baryon density of (3.7 ± 0.2) × 10-4 cm -3. Conclusions. The Planck satellite mission has provided the first SZ detection of the hot and diffuse intercluster gas. © 2013 ESO., The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU).

Published
2016

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