Zobrazeno 1 - 10
of 252
pro vyhledávání: '"Bade D"'
Autor:
Chung, Dongwoo T., Breysse, Patrick C., Cleary, Kieran A., Ihle, Håvard T., Padmanabhan, Hamsa, Silva, Marta B., Bond, J. Richard, Borowska, Jowita, Catha, Morgan, Church, Sarah E., Dunne, Delaney A., Eriksen, Hans Kristian, Foss, Marie Kristine, Gaier, Todd, Gundersen, Joshua Ott, Harper, Stuart E., Harris, Andrew I., Hensley, Brandon, Hobbs, Richard, Keating, Laura C., Kim, Junhan, Lamb, James W., Lawrence, Charles R., Lunde, Jonas Gahr Sturtzel, Murray, Norman, Pearson, Timothy J., Philip, Liju, Rasmussen, Maren, Readhead, Anthony C. S., Rennie, Thomas J., Stutzer, Nils-Ole, Uzgil, Bade D., Viero, Marco P., Watts, Duncan J., Wechsler, Risa H., Wehus, Ingunn Kathrine, Woody, David P.
Publikováno v:
ApJ, 933, 186 (2022)
We present the current state of models for the $z\sim3$ carbon monoxide (CO) line-intensity signal targeted by the CO Mapping Array Project (COMAP) Pathfinder in the context of its early science results. Our fiducial model, relating dark matter halo
Externí odkaz:
http://arxiv.org/abs/2111.05931
Autor:
Ihle, Håvard T., Borowska, Jowita, Cleary, Kieran A., Eriksen, Hans Kristian, Foss, Marie K., Harper, Stuart E., Kim, Junhan, Lunde, Jonas G. S., Philip, Liju, Rasmussen, Maren, Stutzer, Nils-Ole, Uzgil, Bade D., Watts, Duncan J., Wehus, Ingunn Kathrine, Bond, J. Richard, Breysse, Patrick C., Catha, Morgan, Church, Sarah E., Chung, Dongwoo T., Dickinson, Clive, Dunne, Delaney A., Gaier, Todd, Gundersen, Joshua Ott, Harris, Andrew I., Hobbs, Richard, Lamb, James W., Lawrence, Charles R., Murray, Norman, Readhead, Anthony C. S., Padmanabhan, Hamsa, Pearson, Timothy J., Rennie, Thomas J., Woody, David P.
We present the power spectrum methodology used for the first-season COMAP analysis, and assess the quality of the current data set. The main results are derived through the Feed-feed Pseudo-Cross-Spectrum (FPXS) method, which is a robust estimator wi
Externí odkaz:
http://arxiv.org/abs/2111.05930
Autor:
Foss, Marie K., Ihle, Håvard T., Borowska, Jowita, Cleary, Kieran A., Eriksen, Hans Kristian, Harper, Stuart E., Kim, Junhan, Lamb, James W., Lunde, Jonas G. S., Philip, Liju, Rasmussen, Maren, Stutzer, Nils-Ole, Uzgil, Bade D., Watts, Duncan J., Wehus, Ingunn K., Woody, David P., Bond, J. Richard, Breysse, Patrick C., Catha, Morgan, Church, Sarah E., Chung, Dongwoo T., Dickinson, Clive, Dunne, Delaney A., Gaier, Todd, Gundersen, Joshua Ott, Harris, Andrew I., Hobbs, Richard, Lawrence, Charles R., Murray, Norman, Readhead, Anthony C. S., Padmanabhan, Hamsa, Pearson, Timothy J., Rennie, Thomas J.
We describe the first season COMAP analysis pipeline that converts raw detector readouts to calibrated sky maps. This pipeline implements four main steps: gain calibration, filtering, data selection, and map-making. Absolute gain calibration relies o
Externí odkaz:
http://arxiv.org/abs/2111.05929
Autor:
Cleary, Kieran A., Borowska, Jowita, Breysse, Patrick C., Catha, Morgan, Chung, Dongwoo T., Church, Sarah E., Dickinson, Clive, Eriksen, Hans Kristian, Foss, Marie Kristine, Gundersen, Joshua Ott, Harper, Stuart E., Harris, Andrew I., Hobbs, Richard, Håvard, Ihle, T., Kim, Junhan, Kocz, Jonathon, Lamb, James W., Lunde, Jonas G. S., Padmanabhan, Hamsa, Pearson, Timothy J., Philip, Liju, Powell, Travis W., Rasmussen, Maren, Readhead, Anthony C. S., Rennie, Thomas J., Silva, Marta B., Stutzer, Nils-Ole, Uzgil, Bade D., Watts, Duncan J., Wehus, Ingunn Kathrine, Woody, David P., Basoalto, Lilian, Bond, J. Richard, Dunne, Delaney A., Gaier, Todd, Hensley, Brandon, Keating, Laura C., Lawrence, Charles R., Murray, Norman, Reeves, Rodrigo, Viero, Marco P., Wechsler, Risa
The CO Mapping Array Project (COMAP) aims to use line intensity mapping of carbon monoxide (CO) to trace the distribution and global properties of galaxies over cosmic time, back to the Epoch of Reionization (EoR). To validate the technologies and te
Externí odkaz:
http://arxiv.org/abs/2111.05927
Autor:
Uzgil, Bade D., Oesch, Pascal A., Walter, Fabian, Aravena, Manuel, Boogaard, Leindert, Carilli, Chris, Decarli, Roberto, Díaz-Santos, Tanio, Fudamoto, Yoshi, Inami, Hanae, Bouwens, Rychard, Cortes, Paulo C., Cox, Pierre, Daddi, Emmanuele, González-López, Jorge, Labbe, Ivo, Popping, Gergö, Riechers, Dominik, Stefanon, Mauro, Van der Werf, Paul, Weiss, Axel
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212-272 GHz) covers potential [CII] emission in galaxies at $6\leq z \leq8$ throughout a 2.9 arcmin$^2$ area. By selecting on known Lyman-$\alpha$ emitters (LAEs) and
Externí odkaz:
http://arxiv.org/abs/2102.10706
Autor:
Sun, Guochao, Chang, Tzu-Ching, Uzgil, Bade D., Bock, Jamie, Bradford, Charles M., Butler, Victoria, Caze-Cortes, Tessalie, Cheng, Yun-Ting, Cooray, Asantha, Crites, Abigail T., Hailey-Dunsheath, Steve, Emerson, Nick, Frez, Clifford, Hoscheit, Benjamin L., Hunacek, Jonathon R., Keenan, Ryan P., Li, Chao-Te, Madonia, Paolo, Marrone, Daniel P., Moncelsi, Lorenzo, Shiu, Corwin, Trumper, Isaac, Turner, Anthony, Weber, Alexis, Wei, Ta-Shun, Zemcov, Michael
Line intensity mapping (LIM) provides a unique and powerful means to probe cosmic structures by measuring the aggregate line emission from all galaxies across redshift. The method is complementary to conventional galaxy redshift surveys that are obje
Externí odkaz:
http://arxiv.org/abs/2012.09160
Autor:
Uzgil, Bade D., Bradford, C. Matt, Hailey-Dunsheath, Steve, Maloney, Philip R., Aguirre, James E.
We present Herschel observations of far-infrared (FIR) fine-structure (FS) lines [CII]158$\mu$m, [OI]63$\mu$m, [OIII]52$\mu$m, and [SiII]35$\mu$m in the z=2.56 Cloverleaf quasar, and combine them with published data in an analysis of the dense inters
Externí odkaz:
http://arxiv.org/abs/1610.00347
Publikováno v:
ApJ, 793, 116 (2014)
Infrared fine-structure emission lines from trace metals are powerful diagnostics of the interstellar medium in galaxies. We explore the possibility of studying the redshifted far-IR fine-structure line emission using the three-dimensional (3-D) powe
Externí odkaz:
http://arxiv.org/abs/1407.4860
Akademický článek
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Autor:
Dongwoo T. Chung, Patrick C. Breysse, Kieran A. Cleary, Håvard T. Ihle, Hamsa Padmanabhan, Marta B. Silva, J. Richard Bond, Jowita Borowska, Morgan Catha, Sarah E. Church, Delaney A. Dunne, Hans Kristian Eriksen, Marie Kristine Foss, Todd Gaier, Joshua Ott Gundersen, Stuart E. Harper, Andrew I. Harris, Brandon Hensley, Richard Hobbs, Laura C. Keating, Junhan Kim, James W. Lamb, Charles R. Lawrence, Jonas Gahr Sturtzel Lunde, Norman Murray, Timothy J. Pearson, Liju Philip, Maren Rasmussen, Anthony C. S. Readhead, Thomas J. Rennie, Nils-Ole Stutzer, Bade D. Uzgil, Marco P. Viero, Duncan J. Watts, Risa H. Wechsler, Ingunn Kathrine Wehus, David P. Woody
Publikováno v:
The Astrophysical Journal
We present the current state of models for the $z\sim3$ carbon monoxide (CO) line-intensity signal targeted by the CO Mapping Array Project (COMAP) Pathfinder in the context of its early science results. Our fiducial model, relating dark matter halo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::923e87f1ac9532eb8372c8adfb6a526b
https://resolver.caltech.edu/CaltechAUTHORS:20220722-769356000
https://resolver.caltech.edu/CaltechAUTHORS:20220722-769356000