Zobrazeno 1 - 10
of 910
pro vyhledávání: '"Jansen, R. P."'
Autor:
Polletta, M., Frye, B. L., Garuda, N., Willner, S. P., Berta, S., Kneissl, R., Dole, H., Jansen, R. A., Lehnert, M. D., Cohen, S. H., Summers, J., Windhorst, R. A., D'Silva, J. C. J., Koekemoer, A. M., Coe, D., Conselice, C. J., Driver, S. P., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Ryan, Jr., R. E., Willmer, C. N. A., Yan, H., Arumugam, V., Cheng, C., Gim, H. B., Hathi, N. P., Holwerda, B., Kamieneski, P., Keel, W. C., Li, J., Pascale, M., Rottgering, H., Smith, B. M., Yun, M. S.
Dusty star-forming galaxies (DSFGs) contribute significantly to the stellar buildup at cosmic noon. Major mergers and gas accretion are often invoked to explain DSFGs' prodigious star-formation rates (SFRs) and large stellar masses. We conducted a sp
Externí odkaz:
http://arxiv.org/abs/2405.07986
Autor:
Jansen, R., Yuasa, S.
Publikováno v:
npj Quantum Information 10, 21 (2024)
Employing spins in quantum dots for fault-tolerant quantum computing in large-scale qubit arrays with on-chip control electronics requires high-fidelity qubit operation at elevated temperature. This poses a challenge for single spin initialization an
Externí odkaz:
http://arxiv.org/abs/2403.19986
Autor:
Pierel, J. D. R., Frye, B. L., Pascale, M., Caminha, G. B., Chen, W., Dhawan, S., Gilman, D., Grayling, M., Huber, S., Kelly, P., Thorp, S., Arendse, N., Birrer, S., Bronikowski, M., Canameras, R., Coe, D., Cohen, S. H., Conselice, C. J., Driver, S. P., Dsilva, J. C. J., Engesser, M., Foo, N., Gall, C., Garuda, N., Grillo, C., Grogin, N. A., Henderson, J., Hjorth, J., Jansen, R. A., Johansson, J., Kamieneski, P. S., Koekemoer, A. M., Larison, C., Marshall, M. A., Moustakas, L. A., Nonino, M., Ortiz Iii, R., Petrushevska, T., Pirzkal, N., Robotham, A., Ryan, Jr., R. E., Schuldt, S., Strolger, L. G., Summers, J., Suyu, S. H., Treu, T., Willmer, C. N. A., Windhorst, R. A., Yan, H., Zitrin, A., Acebron, A., Chakrabarti, S., Coulter, D. A., Fox, O. D., Huang, X., Jha, S. W., Li, G., Mazzali, P. A., Meena, A. K., Perez-Fournon, I., Poidevin, F., Rest, A., Riess, A. G.
Supernova (SN) H0pe is a gravitationally lensed, triply-imaged, Type Ia SN (SN Ia) discovered in James Webb Space Telescope imaging of the PLCK G165.7+67.0 cluster of galaxies. Well-observed multiply-imaged SNe provide a rare opportunity to constrain
Externí odkaz:
http://arxiv.org/abs/2403.18954
Autor:
Willner, S. P., Gim, H. B., Polletta, M. del Carmen, Cohen, S. H., Willmer, C. N. A., Zhao, X., D'Silva, J. C. J., Jansen, R. A., Koekemoer, A. M., Summers, J., Windhorst, R. A., Coe, D., Conselice, C. J., Driver, S. P., Frye, B., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Tompkins, S., Yan, H., Hammel, H. B., Milam, S. N., Adams, N. J., Beacom, J. F., Bhatawdekar, R., Cheng, C., Civano, F., Cotton, W., Hyun, M., Kikuta, S., Nyland, K. E., Peters, W. M., Petric, A., Röttgering, H. J. A., Shimwell, T., Yun, M. S.
The Time Domain Field (TDF) near the North Ecliptic Pole in JWST's continuous-viewing zone will become a premier "blank field" for extragalactic science. JWST/NIRCam data in a 16 arcmin$^2$ portion of the TDF identify 4.4 $\mu$m counterparts for 62 o
Externí odkaz:
http://arxiv.org/abs/2309.13008
Autor:
Polletta, M., Nonino, M., Frye, B., Gargiulo, A., Bisogni, S., Garuda, N., Thompson, D., Lehnert, M., Pascale, M., Willner, S. P., Kamieneski, P., Leimbach, R., Cheng, C., Coe, D., Cohen, S. H., Conselice, C. J., Dai, L., Diego, J., Dole, H., Driver, S. P., D'Silva, J. C. J., Fontana, A., Foo, N., Furtak, L. J., Grogin, N. A., Harrington, K., Hathi, N. P., Jansen, R. A., Kelly, P., Koekemoer, A. M., Mancini, C., Marshall, M. A., Pierel, J. D. R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Snigula, J. M., Summers, J., Tompkins, S., Willmer, C. N. A., Windhorst, R. A., Yan, H., Yun, M. S., Zitrin, A.
Publikováno v:
A&A 675, L4 (2023)
Supernova (SN) H0pe was discovered as a new transient in James Webb Space Telescope (JWST) NIRCam images of the galaxy cluster PLCK G165.7+67.0 taken as part of the "Prime Extragalactic Areas for Reionization and Lensing Science" (PEARLS) JWST GTO pr
Externí odkaz:
http://arxiv.org/abs/2306.12385
Autor:
Boselli, A., Fossati, M., Cote, P., Cuillandre, J. C., Ferrarese, L., Gwyn, S., Amram, P., Ayromlou, M., Balogh, M., Bellusci, G., Boquien, M., Gavazzi, G., Hensler, G., Longobardi, A., Nelson, D., Pillepich, A., Roediger, J., Sanchez-Jansen, R., Sun, M., Trinchieri, G.
Publikováno v:
A&A 675, A123 (2023)
We use a complete set of deep narrow-band imaging data for 384 galaxies gathered during the VESTIGE survey to derive the first Halpha luminosity function (LF) of the Virgo cluster within R200. The data allow us to cover the whole dynamic range of the
Externí odkaz:
http://arxiv.org/abs/2305.15919
Autor:
Robotham, A. S. G., D'Silva, J. C. J., Windhorst, R. A., Jansen, R. A., Summers, J., Driver, S. P., Wilmer, C. N. A., Bellstedt, S.
The James Webb Space Telescope (JWST) near-infrared camera (NIRCam) has been found to exhibit serious wisp-like structures in four of its eight short-wavelength detectors. The exact structure and strength of these wisps is highly variable with the po
Externí odkaz:
http://arxiv.org/abs/2305.01175
Autor:
Zhao, X., Civano, F., Fornasini, F. M., Alexander, D. M., Cappelluti, N., Chen, C. T., Cohen, S. H., Elvis, M., Gandhi, P., Grogin, N. A., Hickox, R. C., Jansen, R. A., Koekemoer, A., Lanzuisi, G., Maksym, W. P., Masini, A., Rosario, D. J., Ward, M. J., Willmer, C. N. A., Windhorst, R. A.
We present the $NuSTAR$ extragalactic survey of the $James$ $Webb$ $Space$ $Telescope$ ($JWST$) North Ecliptic Pole (NEP) Time-Domain Field. The survey covers a $\sim$0.16 deg$^2$ area with a total exposure of 681 ks acquired in a total of nine obser
Externí odkaz:
http://arxiv.org/abs/2109.13839
Akademický článek
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Autor:
Koekemoer, Anton M., Foley, R. J., Spergel, D. N., Bagley, M., Bezanson, R., Bianco, F. B., Bouwens, R., Bradley, L., Brammer, G., Capak, P., Davidzon, I., De Rosa, G., Dickinson, M. E., Doré, O., Dunlop, J. S., Ellis, R. S., Fan, X., Fazio, G. G., Ferguson, H. C., Filippenko, A. V., Finkelstein, S., Frye, B., Gawiser, E., Grogin, N. A., Hathi, N. P., Hirata, C. M., Hounsell, R., Illingworth, G. D., Jansen, R. A., Jauzac, M., Jha, S. W., Kartaltepe, J. S., Kim, A. G., Kelly, P., Kruk, J. W., Larson, R., Lotz, J., Lucas, R., Malhotra, S., Mandel, K., Margutti, R., Marrone, D., McLure, R. J., McQuinn, K., Melchior, P., Mobasher, B., Mould, J. R., Moustakas, L., Newman, J. A., Papovich, C., Peeples, M. S., Perlmutter, S., Pirzkal, N., Rhoads, J., Rhodes, J., Robertson, B., Rubin, D., Ryan, R., Scolnic, D., Shapley, A., Somerville, R., Steinhardt, C., Stiavelli, M., Street, R., Trenti, M., Treu, T., Wang, L., Wang, Y., Whalen, D., Windhorst, R. A., Wollack, E. J., Yan, H.
Studying the formation and evolution of galaxies at the earliest cosmic times, and their role in reionization, requires the deepest imaging possible. Ultra-deep surveys like the HUDF and HFF have pushed to mag \mAB$\,\sim\,$30, revealing galaxies at
Externí odkaz:
http://arxiv.org/abs/1903.06154