Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Gandilo, Natalie"'
Autor:
Datta, Rahul, Chuss, David T., Eimer, Joseph, Essinger-Hileman, Thomas, Gandilo, Natalie N., Helson, Kyle, Kogut, Alan J., Lowe, Luke, Mirel, Paul, Rostem, Karwan, Sagliocca, Marco, Sponseller, Danielle, Switzer, Eric R., Taraschi, Peter A., Wollack, Edward J.
Publikováno v:
Review of Scientific Instruments 92, 035111 (2021)
Measuring the faint polarization signal of the cosmic microwave background (CMB) not only requires high optical throughput and instrument sensitivity but also control over systematic effects. Polarimetric cameras or receivers used in this setting oft
Externí odkaz:
http://arxiv.org/abs/2103.07936
Autor:
Shariff, Jamil A., Ade, Peter A. R., Angilè, Francesco E., Ashton, Peter, Benton, Steven J., Devlin, Mark J., Dober, Bradley, Fissel, Laura M., Fukui, Yasuo, Galitzki, Nicholas, Gandilo, Natalie N., Klein, Jeffrey, Korotkov, Andrei L., Li, Zhi-Yun, Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, Calvin B., Novak, Giles, Pascale, Enzo, Poidevin, Frédérick, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Soler, Juan D., Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek
Linear polarization maps of the Carina Nebula were obtained at 250, 350, and 500 $\mu$m during the 2012 flight of the BLASTPol balloon-borne telescope. These measurements are combined with Planck 850 $\mu$m data in order to produce a submillimeter sp
Externí odkaz:
http://arxiv.org/abs/1809.06375
Autor:
Fissel, Laura M., Ade, Peter A. R., Angilè, Francesco E., Ashton, Peter, Benton, Steven J., Chen, Che-Yu, Cunningham, Maria, Devlin, Mark J., Dober, Bradley, Friesen, Rachel, Fukui, Yasuo, Galitzki, Nicholas, Gandilo, Natalie N., Goodman, Alyssa, Green, Claire-Elise, Jones, Paul, Klein, Jeffrey, King, Patrick, Korotkov, Andrei L., Li, Zhi-Yun, Lowe, Vicki, Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, Calvin B., Newmark, Amanda, Novak, Giles, Pascale, Enzo, Poidevin, Frédérick, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan D., Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek, Zucker, Catherine
We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500-$\mu$m polarization maps made with the BLASTPol balloon-borne polarimeter to the orientation of structures in the integrated line emission maps fro
Externí odkaz:
http://arxiv.org/abs/1804.08979
Autor:
Ashton, Peter C., Ade, Peter A. R., Angilè, Francesco E., Benton, Steven J., Devlin, Mark J., Dober, Bradley, Fissel, Laura M., Fukui, Yasuo, Galitzki, Nicholas, Gandilo, Natalie N., Klein, Jeffrey, Korotkov, Andrei K., Li, Zhi-Yun, Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, Calvin B., Novak, Giles, Pascale, Enzo, Poidevin, Frédéric, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan D., Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek
Polarized emission from aligned dust is a crucial tool for studies of magnetism in the ISM and a troublesome contaminant for studies of CMB polarization. In each case, an understanding of the significance of the polarization signal requires well-cali
Externí odkaz:
http://arxiv.org/abs/1707.02936
Autor:
Gandilo, Natalie N., Ade, Peter A. R., Benford, Dominic, Bennett, Charles L., Chuss, David T., Dotson, Jessie L., Eimer, Joseph R., Fixsen, Dale J., Halpern, Mark, Hilton, Gene, Hinshaw, Gary F., Irwin, Kent, Jhabvala, Christine, Kimball, Mark, Kogut, Alan, Lowe, Luke, McMahon, Jeff J., Miller, Timothy M., Mirel, Paul, Moseley, S. Harvey, Pawlyk, Samuel, Rodriguez, Samelys, Sharp III, Elmer, Shirron, Peter, Staguhn, Johannes G., Sullivan, Dan F., Switzer, Eric R., Taraschi, Peter, Tucker, Carole E., Wollack, Edward J.
The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne telescope designed to measure the polarization of the Cosmic Microwave Background on large angular scales. PIPER will map 85% of the sky at 200, 270, 350, and 600 GHz over a se
Externí odkaz:
http://arxiv.org/abs/1607.06172
Autor:
Santos, Fabio P., Ade, Peter A. R., Angile, Francesco E., Ashton, Peter, Benton, Steven J., Devlin, Mark J., Dober, Bradley, Fissel, Laura M., Fukui, Yasuo, Galitzki, Nicholas, Gandilo, Natalie N., Klein, Jeffrey, Korotkov, Andrei L., Li, Zhi-Yun, Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, Calvin B., Novak, Giles, Pascale, Enzo, Poidevin, Frederick, Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan Diego, Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek
We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at submillimeter (sub-mm) wavelengths for the Vela C molecular cloud. The near-IR data consist of mo
Externí odkaz:
http://arxiv.org/abs/1605.08522
Autor:
Gandilo, Natalie N., Ade, Peter A. R., Angilè, Francesco E., Ashton, Peter, Benton, Steven J., Devlin, Mark J., Dober, Bradley, Fissel, Laura M., Fukui, Yasuo, Galitzki, Nicholas, Klein, Jeffrey, Korotkov, Andrei L., Li, Zhi-Yun, Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, Calvin B., Novak, Giles, Pascale, Enzo, Poidevin, Frédérick, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan Diego, Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek
Publikováno v:
The Astrophysical Journal, Volume 824, Number 2, p.84 (2016)
Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500um during the 2012 flight of the balloon-borne telescope BLASTPol. These measurements are used in conjunction with 850um data from Planck to study the submillimeter spe
Externí odkaz:
http://arxiv.org/abs/1512.06745
Autor:
Bryan, Sean, Ade, Peter, Amiri, Mandana, Benton, Steven, Bihary, Richard, Bock, James, Bond, J. Richard, Chiang, H. Cynthia, Contaldi, Carlo, Crill, Brendan, Dore, Olivier, Elder, Benjamin, Filippini, Jeffrey, Fraisse, Aurelien, Gambrel, Anne, Gandilo, Natalie, Gudmundsson, Jon, Hasselfield, Matthew, Halpern, Mark, Hilton, Gene, Holmes, Warren, Hristov, Viktor, Irwin, Kent, Jones, William, Kermish, Zigmund, Lawrie, Craig, MacTavish, Carrie, Mason, Peter, Megerian, Krikor, Moncelsi, Lorenzo, Montroy, Thomas, Morford, Tracy, Nagy, Johanna, Netterfield, C. Barth, Padilla, Ivan, Rahlin, Alexandra S., Reintsema, Carl, Riley, Daniel C., Ruhl, John, Runyan, Marcus, Saliwanchik, Benjamin, Shariff, Jamil, Soler, Juan, Trangsrud, Amy, Tucker, Carole, Tucker, Rebecca, Turner, Anthony, Wen, Shyang, Wiebe, Donald, Young, Edward
Publikováno v:
Review of Scientific Instruments, 87, 014501 (2016)
We describe the cryogenic half-wave plate rotation mechanisms built for and used in Spider, a polarization-sensitive balloon-borne telescope array that observed the Cosmic Microwave Background at 95 GHz and 150 GHz during a stratospheric balloon flig
Externí odkaz:
http://arxiv.org/abs/1510.01771
Autor:
Fissel, Laura M., Ade, Peter A. R., Angilè, Francesco E., Ashton, Peter, Benton, Steven, Devlin, Mark J., Dober, Bradley, Fukui, Yasuo, Galitzki, Nicholas, Gandilo, Natalie N., Klein, J. R., Li, Zhi-Yun, Korotkov, Andrei L., Martin, Peter G., Matthews, Tristan G., Moncelsi, Lorenzo, Nakamura, Fumitaka, Netterfield, C. Barth, Novak, Giles, Pascale, Enzo, Poidevin, Frédérick, Santos, Fabio P., Savini, Giorgio, Scott, Douglas, Shariff, Jamil A., Soler, Juan D., Thomas, Nicholas E., Tucker, Carole E., Tucker, Gregory S., Ward-Thompson, Derek
We present results for Vela C obtained during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol). We mapped polarized intensity across almost the entire extent of this giant molecular cloud, in band
Externí odkaz:
http://arxiv.org/abs/1509.05298
Autor:
Shariff, Jamil A., Ade, Peter A. R., Amiri, Mandana, Benton, Steven J., Bock, Jamie J., Bond, J. Richard, Bryan, Sean A., Chiang, H. Cynthia, Contaldi, Carlo R., Crill, Brendan P., Doré, Olivier P., Farhang, Marzieh, Filippini, Jeffrey P., Fissel, Laura M., Fraisse, Aurelien A., Gambrel, Anne E., Gandilo, Natalie N., Golwala, Sunil R., Gudmundsson, Jon E., Halpern, Mark, Hasselfield, Matthew, Hilton, Gene C., Holmes, Warren A., Hristov, Viktor V., Irwin, Kent D., Jones, William C., Kermish, Zigmund D., Kuo, Chao-Lin, MacTavish, Carolyn J., Mason, Peter V., Megerian, Krikor G., Moncelsi, Lorenzo, Morford, Tracy A., Nagy, Johanna M., Netterfield, C. Barth, O'Brient, Roger, Rahlin, Alexandra S., Reintsema, Carl D., Ruhl, John E., Runyan, Marcus C., Soler, Juan D., Trangsrud, Amy, Tucker, Carole E., Tucker, Rebecca S., Turner, Anthony D., Weber, Alexis C., Wiebe, Donald V., Young, Edward Y.
We present the technology and control methods developed for the pointing system of the SPIDER experiment. SPIDER is a balloon-borne polarimeter designed to detect the imprint of primordial gravitational waves in the polarization of the Cosmic Microwa
Externí odkaz:
http://arxiv.org/abs/1407.1880