Zobrazeno 1 - 10
of 1 956
pro vyhledávání: '"P. Buat"'
Autor:
Yang, J., Braun, S., Buat, Q., Ding, J., Harrison, M., Kammel, P., Mazza, S. M., McKinney-Martinez, F., Molnar, A., Ott, J., Seiden, A., Schumm, B., Zhao, Y., Zhang, Y., Tishchenko, V., Bisht, A., Centis-Vignali, M., Paternoster, G., Boscardin, M.
In recent years, the gain suppression mechanism has been studied for large localized charge deposits in Low-Gain Avalanche Detectors (LGADs). LGADs are a thin silicon detector with a highly doped gain layer that provides moderate internal signal ampl
Externí odkaz:
http://arxiv.org/abs/2502.02244
Autor:
Gandolfi, G., Rodighiero, G., Bisigello, L., Grazian, A., Finkelstein, S. L., Dickinson, M., Castellano, M., Merlin, E., Calabrò, A., Papovich, C., Bianchetti, A., Bañados, E., Benotto, P., Buitrago, F., Daddi, E., Girardi, G., Giulietti, M., Hirschmann, M., Holwerda, B. W., Haro, P. Arrabal, Lapi, A., Lucas, R. A., Lyu, Y., Massardi, M., Pacucci, F., Pérez-González, P. G., Ronconi, T., Tarrasse, M., Wilkins, S., Vulcani, B., Yung, L. Y. A., Zavala, J. A., Backhaus, B., Bagley, M., Buat, V., Burgarella, D., Kartaltepe, J., Khusanova, Y., Kirkpatrick, A., Kocevski, D., Koekemoer, A. M., Lambrides, E., Pirzkal, N., Yang, G.
The James Webb Space Telescope (JWST) is revolutionizing our understanding of the Universe by unveiling faint, near-infrared dropouts previously beyond our reach, ranging from exceptionally dusty sources to galaxies up to redshift $z \sim 14$. In thi
Externí odkaz:
http://arxiv.org/abs/2502.02637
Autor:
Zavala, Jorge A., Bakx, Tom, Mitsuhashi, Ikki, Castellano, Marco, Calabro, Antonello, Akins, Hollis, Buat, Veronique, Casey, Caitlin M., Fernandez-Arenas, David, Franco, Maximilien, Fontana, Adriano, Hatsukade, Bunyo, Ho, Luis C., Ikeda, Ryota, Kartaltepe, Jeyhan, Koekemoer, Anton M., McKinney, Jed, Napolitano, Lorenzo, Perez-Gonzalez, Pablo G., Santini, Paola, Serjeant, Stephen, Terlevich, Elena, Terlevich, Roberto, Yung, L. Y. Aaron
We present ALMA observations on the high-redshift galaxy GHZ2 and report a successful detection of the rest-frame 88um atomic transition from doubly-ionized Oxygen at z=12.3327+/-0.0005. Based on these observations, combined with additional constrain
Externí odkaz:
http://arxiv.org/abs/2411.03593
Autor:
Burgarella, Denis, Buat, Véronique, Theulé, Patrice, Zavala, Jorge, Haro, Pablo Arrabal, Bagley, Micaela B., Boquien, Médéric, Cleri, Nikko, Dewachter, Tim, Dickinson, Mark, Ferguson, Henry C., Fernández, Vital, Finkelstein, Steven L., Fontana, Adriano, Gawiser, Eric, Grazian, Andrea, Grogin, Norman, Holwerda, Benne W., Kartaltepe, Jeyhan S., Kewley, Lisa, Kirkpatrick, Allison, Kocevski, Dale, Koekemoer, Anton M., Long, Arianna, Lotz, Jennifer, Lucas, Ray A., Mobasher, Bahram, Papovich, Casey, Pérez-González, Pablo G., Pirzkal, Nor, Ravindranath, Swara, Rodighiero, Giulia, Roehlly, Yannick, Rose, Caitlin, Seillé, Lise-Marie, Somerville, Rachel, Wilkins, Steve, Yang, Guang, Yung, L. Y. Aaron
We investigate the coevolution of metals and dust for 173 galaxies at 4.0
Externí odkaz:
http://arxiv.org/abs/2410.23959
Autor:
Brooks, Madisyn, Simons, Raymond C., Trump, Jonathan R., Taylor, Anthony J., Backhaus, Bren, Davis, Kelcey, Buat, Véronique, Cleri, Nikko J., Finkelstein, Steven L., Hirschmann, Michaela, Holwerda, Benne W., Kocevski, Dale D., Koekemoer, Anton M., Lucas, Ray A., Pacucci, Fabio, Seillé, Lise-Marie
JWST spectroscopy has discovered a population of $z \gtrsim 3.5$ galaxies with broad Balmer emission lines, and narrow forbidden lines, that are consistent with hosting active galactic nuclei (AGN). Many of these systems, now known as ``little red do
Externí odkaz:
http://arxiv.org/abs/2410.07340
Autor:
Rakotondrainibe, N. A., Buat, V., Turpin, D., Dornic, D., LeFloc'h, E., Vergani, S. D., Basa, S.
Gamma-ray burst (GRB) afterglows are powerful probes for studying the different properties of their host galaxies (e.g., the interstellar dust) at all redshifts. By fitting their spectral energy distribution (SED) over a large range of wavelengths, w
Externí odkaz:
http://arxiv.org/abs/2409.03570
Autor:
Kim, Helen Kyung, Malkan, Matthew A., Takagi, Toshinobu, Oi, Nagisa, Burgarella, Denis, Miyaji, Takamitsu, Shim, Hyunjin, Matsuhara, Hideo, Goto, Tomotsugu, Ohyama, Yoichi, Buat, Veronique, Kim, Seong Jin
Polycyclic aromatic hydrocarbon (PAH) dust emission has been proposed as an effective extinction-independent star formation rate (SFR) indicator in the mid-infrared (MIR), but this may depend on conditions in the interstellar medium. The coverage of
Externí odkaz:
http://arxiv.org/abs/2408.14005
Autor:
Braun, S., Buat, Q., Ding, J., Kammel, P., Mazza, S. M., McKinney-Martinez, F., Molnar, A., Lansdell, C., Ott, J., Seiden, A., Schumm, B., Zhao, Y.
Low-Gain Avalanche Detectors (LGADs) are a type of thin silicon detector with a highly doped gain layer that provides moderate internal signal amplification. One recent challenge in the use of LGADs, studied by several research groups, is the gain su
Externí odkaz:
http://arxiv.org/abs/2405.02550
Autor:
Bakx, Tom J. L. C., Berta, S., Dannerbauer, H., Cox, P., Butler, K. M., Hagimoto, M., Hughes, D. H., Riechers, D. A., van der Werf, P. P., Yang, C., Baker, A. J., Beelen, A., Bendo, G. J., Borsato, E., Buat, V., Cooray, A. R., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Ismail, D., Ivison, R. J., Jones, B., Krips, M., Lehnert, M. D., Marchetti, L., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Nanni, A., Chartab, N., Serjeant, S., Stanley, F., Tamura, Y., Urquhart, S. A., Vlahakis, C., Weiß, A., Young, A. J.
We report on deep SCUBA-2 observations at 850$\mu$m and NOEMA spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive ($M_{*} \approx 2 \times 10^{11}$ M$_{\odot}$) Herschel-selected source HerBS-70. This source was re
Externí odkaz:
http://arxiv.org/abs/2404.18991
Autor:
Seillé, L. -M., Buat, V., Fernández, V., Boquien, M., Roehlly, Y., Boselli, A., Calabrò, A., Amorín, R. O., Backhaus, B. E., Burgarella, D., Cleri, N. J., Dickinson, M., Hathi, N. P., Holwerda, B. W., Koekemoer, A. M., Napolitano, L., Pacucci, F., Robertson, C., Yung, L. Y. A.
Publikováno v:
A&A 689, A102 (2024)
The ultraviolet continuum traces young stars while the near-infrared unveils older stellar populations and dust-obscured regions. Balmer emission lines provide insights on gas properties and young stellar objects but are highly affected by dust atten
Externí odkaz:
http://arxiv.org/abs/2404.09659