Zobrazeno 1 - 9
of 9
pro vyhledávání: '"D. E. Schenck"'
Autor:
Masashi Hazumi, P. Hyland, Kam Arnold, Y. Akiba, Frederick Matsuda, Paul L. Richards, M. Atlas, Yuji Chinone, A. E. Anthony, Amit P. S. Yadav, P. A. R. Ade, Y. Hori, A Orlando, S. Moyerman, Aaron Lee, Reijo Keskitalo, M. Navaroli, Nathan Stebor, I. Schanning, Bryan Steinbach, N. W. Halverson, Yuki Inoue, Chase Owen Shimmin, Zigmund Kermish, H. Nishino, Tucker Elleflot, M. J. Myers, G. Fabbian, Christian L. Reichardt, Eric V. Linder, Masaya Hasegawa, Kaori Hattori, E. M. Leitch, Helmuth Spieler, Theodore Kisner, Chang Feng, Meir Shimon, J. Howard, Praween Siritanasak, Brian Keating, O. Zahn, J. Peloton, Julian Borrill, D. Boettger, Darcy Barron, Radek Stompor, Marius Lungu, H. Morii, S. Takakura, A. Shimizu, Tomotake Matsumura, Hans P. Paar, William F. Grainger, Gabriel M. Rebeiz, E. Quealy, Graeme Smecher, X. Meng, D. E. Schenck, Scott Chapman, Takayuki Tomaru, A. J. Gilbert, Josquin Errard, D. Poletti, B. Wilson, W. L. Holzapfel, Aritoki Suzuki, Daniel Flanigan, Colin Ross, Nathan J. Miller, M. Le Jeune, M. A. Dobbs, Blake D. Sherwin, G. Jaehnig, Andrew H. Jaffe
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2017, 848, ⟨10.3847/1538-4357/aa8c70⟩
The Astrophysical Journal, vol 848, iss 1
The Astrophysical Journal, 2017, 848, ⟨10.3847/1538-4357/aa8c70⟩
The Astrophysical Journal, vol 848, iss 1
We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34d68f7b211c80f1b4339a9c415c0a14
https://hal.science/hal-03735950
https://hal.science/hal-03735950
Autor:
Nathan Stebor, Tomotake Matsumura, Christian L. Reichardt, Michael J. Myers, S. Takakura, Masaya Hasegawa, Giuseppe Puglisi, Adrian T. Lee, Kaori Hattori, Charles A. Hill, Julian Borrill, Nobuhiko Katayama, K. M. Rotermund, Stephen M. Feeney, Kam Arnold, Davide Poletti, E. M. Leitch, Darcy Barron, Neil Goeckner-Wald, Yuji Chinone, Peter A. R. Ade, Nathan Whitehorn, M. Atlas, Y. Akiba, Greg Jaehnig, Andrew H. Jaffe, Chang Feng, Scott Chapman, Gabriel M. Rebeiz, Brian Keating, A. Gilbert, Colin Ross, M. Navaroli, Aritoki Suzuki, Tucker Elleflot, Graeme Smecher, Hans P. Paar, Ted Kisner, J. Peloton, Oliver Jeong, Amit P. S. Yadav, Giulio Fabbian, J. P. Kaufman, D. E. Schenck, N. W. Halverson, A. Ducout, A. Tikhomirov, Masashi Hazumi, Takayuki Tomaru, Radek Stompor, Praween Siritanasak, Zigmund Kermish, Oliver Zahn, Blake D. Sherwin, D. Boettger, M. Le Jeune, Takahiro Okamura, A. Cukierman, B. Wilson, D. Leon, Nathan J. Miller, Reijo Keskitalo, Bryan Steinbach, M. A. Dobbs, Yuki Inoue, Josquin Errard, W. L. Holzapfel, Y. Hori, Jacques Delabrouille, Paul L. Richards, Frederick Matsuda, H. Nishino, Osamu Tajima, Eric V. Linder, Carlo Baccigalupi
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩
The Astrophysical Journal, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
The Astrophysical Journal, American Astronomical Society, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩
The Astrophysical Journal, 2015, 809, pp.63. ⟨10.1088/0004-637X/809/1/63⟩
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies their effective noise, while its fluctuations introduce spatial and tem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7caf15a1af991702235e3c30b583d198
http://hal.in2p3.fr/in2p3-01184756
http://hal.in2p3.fr/in2p3-01184756
X-ray observations were used to examine the complex temperature structure of Abell 85, a cool-core galaxy cluster. Temperature features can provide evidence of merging events which shock heat the intracluster gas. Temperature maps were made from both
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7c29c7fc3b766245f88c336ee460555
http://arxiv.org/abs/1405.2366
http://arxiv.org/abs/1405.2366
Autor:
Aritoki Suzuki, Frederick Matsuda, Daniel Flanigan, Meir Shimon, Kam Arnold, Nathan J. Miller, Colin Ross, X. Meng, Y. Akiba, S. Takakura, A. E. Anthony, Y. Hori, Josquin Errard, D. Poletti, Julian Borrill, Hans P. Paar, Tomotake Matsumura, Yuki Inoue, Yuji Chinone, Takayuki Tomaru, W. L. Holzapfel, D. E. Schenck, Jonathon Howard, S. Moyerman, Tucker Elleflot, M. A. Dobbs, Nathan Stebor, P. Hyland, A. Tikhomirov, Paul L. Richards, I. Schanning, M. Le Jeune, Eric V. Linder, Masaya Hasegawa, Christian L. Reichardt, Giulio Fabbian, M. Atlas, Andrew H. Jaffe, J. Peloton, H. Morii, Oliver Zahn, A. Shimizu, Kaori Hattori, E. M. Leitch, Helmuth Spieler, Scott Chapman, N. W. Halverson, E. Quealy, Masashi Hazumi, William F. Grainger, M. J. Myers, Graeme Smecher, Chang Feng, Blake D. Sherwin, Darcy Barron, Theodore Kisner, Marius Lungu, Reijo Keskitalo, Bryan Steinbach, G. Jaehnig, Peter A. R. Ade, Praween Siritanasak, Kaja Rotermund, Gabriel M. Rebeiz, Amit P. S. Yadav, M. Navaroli, Colin Borys, Zigmund Kermish, Radek Stompor, Adrian T. Lee, A. J. Gilbert, B. Wilson, Brian Keating, D. Boettger, Chase Owen Shimmin, H. Nishino
Publikováno v:
Physical Review Letters
Physical Review Letters, American Physical Society, 2014, 112, pp.131302. ⟨10.1103/PhysRevLett.112.131302⟩
Physical Review Letters, American Physical Society, 2014, 112, pp.131302
Physical Review Letters, 2014, 112, pp.131302. ⟨10.1103/PhysRevLett.112.131302⟩
Physical Review Letters, American Physical Society, 2014, 112, pp.131302. ⟨10.1103/PhysRevLett.112.131302⟩
Physical Review Letters, American Physical Society, 2014, 112, pp.131302
Physical Review Letters, 2014, 112, pp.131302. ⟨10.1103/PhysRevLett.112.131302⟩
We reconstruct the gravitational lensing convergence signal from Cosmic Microwave Background (CMB) polarization data taken by the POLARBEAR experiment and cross-correlate it with Cosmic Infrared Background (CIB) maps from the Herschel satellite. From
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c802826e8f6a6a79080a42f18eff20b
http://hal.in2p3.fr/in2p3-01083502
http://hal.in2p3.fr/in2p3-01083502
Autor:
Suguru Takada, A. E. Anthony, D. E. Schenck, Takayuki Tomaru, Radek Stompor, G. Jaehnig, Amit P. S. Yadav, Theodore Kisner, Takahiro Okamura, Masashi Hazumi, J. Peloton, Kam Arnold, M. Navaroli, Blake D. Sherwin, J. Borrilll, H. Morii, Yuji Chinone, Paul L. Richards, Christian L. Reichardt, Scott Chapman, Darcy Barron, M. Atlas, Zigmund Kermish, Kaori Hattori, Aritoki Suzuki, A. Cukierman, N. W. Halverson, M. J. Myers, Chang Feng, M. Sholl, Hans P. Paar, Tomotake Matsumura, Andrew H. Jaffe, S. Takakura, A. J. Gilbert, Reijo Keskitalo, M. A. Dobbs, Graeme Smecher, Bryan Steinbach, Colin Ross, Amy N. Bender, Tucker Elleflot, B. Wilson, Eric V. Linder, D. Boettger, Brian Keating, Peter A. R. Ade, Adrian T. Lee, Gabriel M. Rebeiz, Praween Siritanasak, G. Fabbian, Jun-ichi Suzuki, Nathan Stebor, Masaya Hasegawa, E. M. Leitch, Y. Akiba, O. Zahn, Frederick Matsuda, M. Le Jeune, H. Yamaguchi, Y. Hori, Yuki Inoue, N. Katayama, Josquin Errard, D. Poletti, W. L. Holzapfel, H. Nishino, X. Meng
POLARBEAR-2 (PB-2) is a cosmic microwave background (CMB) polarization experiment for B-mode detection. The PB-2 receiver has a large focal plane and aperture that consists of 7588 transition edge sensor (TES) bolometers at 250 mK. The receiver consi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::89c86ce6974ee3accee7ad6354c9d0fb
http://hdl.handle.net/20.500.11767/115010
http://hdl.handle.net/20.500.11767/115010
Autor:
Amit P. S. Yadav, Tomotake Matsumura, M. Navaroli, Reijo Keskitalo, Zigmund Kermish, Bryan Steinbach, Y. Akiba, S. Takakura, A. E. Anthony, A. Cukierman, Peter A. R. Ade, Paul L. Richards, N. W. Halverson, M. J. Myers, Takahiro Okamura, Tucker Elleflot, Jun-ichi Suzuki, Amy N. Bender, Nathan J. Miller, Praween Siritanasak, Gabriel M. Rebeiz, X. Meng, E. M. Leitch, O. Zahn, Eric V. Linder, Neil Goeckner-Wald, Giulio Fabbian, M. Atlas, D. E. Schenck, Andrew H. Jaffe, Brian Keating, Aritoki Suzuki, J. Peloton, Takayuki Tomaru, Adrian T. Lee, Kam Arnold, Frederick Matsuda, M. Le Jeune, Julian Borrill, Christopher Raum, Chang Feng, M. A. Dobbs, Josquin Errard, Yuji Chinone, D. Poletti, N. Katayama, K. M. Rotermund, Radek Stompor, W. L. Holzapfel, Nathan Stebor, Darcy Barron, Theodore Kisner, Graeme Smecher, I. Shirley, A. J. Gilbert, M. Sholl, B. Wilson, Hans P. Paar, Masaya Hasegawa, H. Nishino, G. Jaehnig, D. Boettger, Masashi Hazumi, Blake D. Sherwin, Colin Ross, Christian L. Reichardt, Kaori Hattori, H. Morii, Scott Chapman, Suguru Takada, Y. Hori, Yuki Inoue
Publikováno v:
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2014
SPIE Astronomical Telescopes + Instrumentation 2014, Jun 2014, Montreal, Canada. pp.91531F, ⟨10.1117/12.2057332⟩
SPIE Astronomical Telescopes + Instrumentation 2014
SPIE Astronomical Telescopes + Instrumentation 2014, Jun 2014, Montreal, Canada. pp.91531F, ⟨10.1117/12.2057332⟩
International audience; The Simons Array is an expansion of the POLARBEAR cosmic microwave background (CMB) polarization experiment currently observing from the Atacama Desert in Northern Chile. This expansion will create an array of three 3.5m teles
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d405643c5eb8f9eb15f9c6b26e78f46f
http://hdl.handle.net/10281/323386
http://hdl.handle.net/10281/323386
We present an analysis of the relation between the star formation rate (SFR) and mass of dense gas in Galactic clumps and nearby galaxies. Using the bolometric luminosity as a measure of SFR and the molecular line luminosity of HCO+ (3-2) as a measur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdf99d84d37c710ed96f6b280ddae208
http://arxiv.org/abs/1109.1246
http://arxiv.org/abs/1109.1246
Autor:
Meir Shimon, S. Takakura, Tomotake Matsumura, J. Peloton, Radek Stompor, Tucker Elleflot, Daniel Flanigan, M. Atlas, Masashi Hazumi, Chang Feng, A. E. Anthony, Eric V. Linder, S. Moyerman, Oliver Zahn, Josquin Errard, Blake D. Sherwin, Nathan Stebor, Julian Borrill, Giulio Fabbian, I. Schanning, Hans P. Paar, D. Poletti, Gabriel M. Rebeiz, H. Morii, William F. Grainger, Y. Akiba, W. L. Holzapfel, Masaya Hasegawa, Scott Chapman, Yuji Chinone, M. Le Jeune, N. W. Halverson, Colin Ross, M. J. Myers, Paul L. Richards, Kam Arnold, Andrew H. Jaffe, Aritoki Suzuki, Brian Keating, Amit P. S. Yadav, Nathan J. Miller, G. Jaehnig, M. Navaroli, E. M. Leitch, Zigmund Kermish, A. J. Gilbert, Helmuth Spieler, A. Orlando, B. Wilson, D. Boettger, Praween Siritanasak, Chase Owen Shimmin, H. Nishino, Darcy Barron, Marius Lungu, M. A. Dobbs, Christian L. Reichardt, Kaori Hattori, X. Meng, D. E. Schenck, Takayuki Tomaru, E. Quealy, Graeme Smecher, J. Howard, Reijo Keskitalo, P. Hyland, Bryan Steinbach, Theodore Kisner, Y. Hori, Yuki Inoue, Frederick Matsuda, A. Shimizu, Adrian T. Lee
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2014, 794 (2), pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794 (2), pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794, pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794, pp.171
The Astrophysical Journal, 2014, 794 (2), pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794 (2), pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794, pp.171. ⟨10.1088/0004-637X/794/2/171⟩
The Astrophysical Journal, American Astronomical Society, 2014, 794, pp.171
We report a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile. The faint B-mode polarization signature carries information about the Universe's entire history of gra
Publikováno v:
The Astrophysical Journal. 793:80
The galaxy cluster Abell 3667 is an ideal laboratory to study the plasma processes in the intracluster medium (ICM). High resolution Chandra X-ray observations show a cold front in Abell 3667. At radio wavelengths, Abell 3667 reveals a double radio-r