Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Marco P. Viero"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 516:L30-L34
We investigate the dust properties and star-formation signature of galaxies in the early Universe by stacking 111 227 objects in the recently released COSMOS catalogue on maps at wavelengths bracketing the peak of warmed dust emission. We find an ele
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
Autor:
Patrick C. Breysse, Dongwoo T. Chung, 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, Andrew I. Harris, Richard Hobbs, Laura Keating, James W. Lamb, Charles R. Lawrence, Jonas G. S. Lunde, Norman Murray, Timothy J. Pearson, Liju Philip, Maren Rasmussen, Anthony C. S. Readhead, Thomas J. Rennie, Nils-Ole Stutzer, Marco P. Viero, Duncan J. Watts, Ingunn Kathrine Wehus, David P. Woody
We introduce COMAP-EoR, the next generation of the Carbon Monoxide Mapping Array Project aimed at extending CO intensity mapping to the Epoch of Reionization. COMAP-EoR supplements the existing 30 GHz COMAP Pathfinder with two additional 30 GHz instr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa2b31ad7198068d3d2e7e8a4baac48d
http://hdl.handle.net/10852/96047
http://hdl.handle.net/10852/96047
Autor:
Kieran A. Cleary, Jowita Borowska, Patrick C. Breysse, Morgan Catha, Dongwoo T. Chung, Sarah E. Church, Clive Dickinson, Hans Kristian Eriksen, Marie Kristine Foss, Joshua Ott Gundersen, Stuart E. Harper, Andrew I. Harris, Richard Hobbs, Håvard T. Ihle, Junhan Kim, Jonathon Kocz, James W. Lamb, Jonas G. S. Lunde, Hamsa Padmanabhan, Timothy J. Pearson, Liju Philip, Travis W. Powell, Maren Rasmussen, Anthony C. S. Readhead, Thomas J. Rennie, Marta B. Silva, Nils-Ole Stutzer, Bade D. Uzgil, Duncan J. Watts, Ingunn Kathrine Wehus, David P. Woody, Lilian Basoalto, J. Richard Bond, Delaney A. Dunne, Todd Gaier, Brandon Hensley, Laura C. Keating, Charles R. Lawrence, Norman Murray, Roberta Paladini, Rodrigo Reeves, Marco P. Viero, Risa H. Wechsler
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a73d113c5f962526ec5e437dfaf599d
http://hdl.handle.net/10852/95714
http://hdl.handle.net/10852/95714
Autor:
Dongwoo T. Chung, Patrick C. Breysse, Håvard T. Ihle, Hamsa Padmanabhan, Marta B. Silva, J. Richard Bond, Jowita Borowska, Kieran A. Cleary, Hans Kristian Eriksen, Marie Kristine Foss, Joshua Ott Gundersen, Laura C. Keating, Jonas Gahr Sturtzel Lunde, Liju Philip, Nils-Ole Stutzer, Marco P. Viero, Duncan J. Watts, Ingunn Kathrine Wehus
Line-intensity mapping observations will find fluctuations of integrated line emission are attenuated by varying degrees at small scales due to the width of the line emission profiles. This attenuation may significantly impact estimates of astrophysi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebc54f5c81e4f9332375c0a369e4bbf8
http://arxiv.org/abs/2104.11171
http://arxiv.org/abs/2104.11171
Autor:
James W. Lamb, Kieran A. Cleary, David P. Woody, Morgan Catha, Dongwoo T. Chung, Joshua Ott Gundersen, Stuart E. Harper, Andrew I. Harris, Richard Hobbs, Håvard T. Ihle, Jonathon Kocz, Timothy J. Pearson, Liju Philip, Travis W. Powell, Lilian Basoalto, J. Richard Bond, Jowita Borowska, Patrick C. Breysse, Sarah E. Church, Clive Dickinson, Delaney A. Dunne, Hans Kristian Eriksen, Marie Kristine Foss, Todd Gaier, Junhan Kim, Charles R. Lawrence, Jonas G. S. Lunde, Hamsa Padmanabhan, Maren Rasmussen, Anthony C. S. Readhead, Rodrigo Reeves, Thomas J. Rennie, Nils-Ole Stutzer, Marco P. Viero, Duncan J. Watts, Ingunn Kathrine Wehus
Line intensity mapping (LIM) is a new technique for tracing the global properties of galaxies over cosmic time. Detection of the very faint signals from redshifted carbon monoxide (CO), a tracer of star formation, pushes the limits of what is feasibl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::477d57997feafcdec241b455816bcfd0
We combine recent simulation work on the SFR--[C II] correlation at high redshift with empirical modeling of the galaxy--halo connection (via UniverseMachine) to forecast [C II] auto power spectra from $z\sim4$ to $z\sim8$. We compare these to sensit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1a80420725193f38007d8f2b9489ae6
http://arxiv.org/abs/1812.08135
http://arxiv.org/abs/1812.08135
Autor:
Joseph J. Mohr, Elizabeth George, C. L. Chang, Marius Millea, Daniel M. Luong-Van, Bradford Benson, Antony A. Stark, R. Williamson, C. Pryke, N. L. Harrington, Stephen Padin, Adrian T. Lee, Jeff McMahon, J. D. Hrubes, Lindsey Bleem, J. E. Ruhl, Michael Zemcov, W. B. Everett, M. A. Dobbs, Joaquin Vieira, H-M. Cho, Zhen Hou, John E. Carlstrom, T. de Haan, S. S. Meyer, W. L. Holzapfel, A. T. Crites, Erik Shirokoff, N. W. Halverson, G. P. Holder, Keith Vanderlinde, Lorenzo Moncelsi, K. T. Story, K. K. Schaffer, T. M. Crawford, Marco P. Viero, Z. K. Staniszewski, Christian L. Reichardt, James J. Bock, Lloyd Knox, L. M. Mocanu, Daniel P. Marrone, Paolo Serra
Publikováno v:
Astrophys.J.
Astrophys.J., 2019, 881 (2), pp.96. ⟨10.3847/1538-4357/ab2da0⟩
Astrophys.J., 2019, 881 (2), pp.96. ⟨10.3847/1538-4357/ab2da0⟩
We present measurements of the power spectra of cosmic infrared background (CIB) and cosmic microwave background (CMB) fluctuations in six frequency bands. Maps at the lower three frequency bands, 95, 150, and 220 GHz (3330, 2000, 1360 $\mu$m) are fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bb8b6e5dd05c5a8a8abb1b651ff7e2f
https://hal.archives-ouvertes.fr/hal-01914656
https://hal.archives-ouvertes.fr/hal-01914656
Autor:
Jonathon Hunacek, Guochao Sun, Bade Uzgil, Marta B. Silva, Asantha Cooray, Marco P. Viero, Tzu-Ching Chang, C. Matt Bradford, A. T. Crites, Lorenzo Moncelsi, Yun-Ting Cheng, Steve Hailey-Dunsheath, James J. Bock, Michael Zemcov
Publikováno v:
Astrophysical Journal, 856(2):107. IOP PUBLISHING LTD
The Astrophysical Journal
The Astrophysical Journal
Intensity mapping provides a unique means to probe the epoch of reionization (EoR), when the neutral intergalactic medium was ionized by the energetic photons emitted from the first galaxies. The [CII] 158$��$m fine-structure line is typically on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c372ead450d60c5a2657ca9b03327de7
https://resolver.caltech.edu/CaltechAUTHORS:20170531-140121068
https://resolver.caltech.edu/CaltechAUTHORS:20170531-140121068
Autor:
Joshua O. Gundersen, Marcelo A. Alvarez, Marco P. Viero, J. Richard Bond, Hamsa Padmanabhan, Patrick C. Breysse, Marie Kristine Foss, Stuart Harper, H. K. Eriksen, I. K. Wehus, Norman Murray, Kieran Cleary, Håvard T. Ihle, Dongwoo Chung, George Stein
We develop a framework for joint constraints on the CO luminosity function based on power spectra (PS) and voxel intensity distributions (VID), and apply this to simulations of COMAP, a CO intensity mapping experiment. This Bayesian framework is base
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ebe77f0ed9475664dd58b322e133276