Zobrazeno 1 - 10
of 282
pro vyhledávání: '"Theule, P."'
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:
Kruczkiewicz, F., Dulieu, F., Ivlev, A. V., Caselli, P., Giuliano, B. M., Ceccarelli, C., Theulé, P.
To explain grain growth and destruction in warm media, ice mantle formation and sublimation in cold media, and gas line emission spectroscopy, astrochemical models must mimic the gas--solid abundance ratio. Ice-sublimation mechanisms determine the po
Externí odkaz:
http://arxiv.org/abs/2404.02695
Autor:
Poch, Olivier, Istiqomah, Istiqomah, Quirico, Eric, Beck, Pierre, Schmitt, Bernard, Theulé, Patrice, Faure, Alexandre, Hily-Blant, Pierre, Bonal, Lydie, Raponi, Andrea, Ciarniello, Mauro, Rousseau, Batiste, Potin, Sandra, Brissaud, Olivier, Flandinet, Laurène, Filacchione, Gianrico, Pommerol, Antoine, Thomas, Nicolas, Kappel, David, Mennella, Vito, Moroz, Lyuba, Vinogradoff, Vassilissa, Arnold, Gabriele, Erard, Stéphane, Bockelée-Morvan, Dominique, Leyrat, Cédric, Capaccioni, Fabrizio, de Sanctis, Maria Cristina, Longobardo, Andrea, Mancarella, Francesca, Palomba, Ernesto, Tosi, Federico
Publikováno v:
European Conference on Laboratory Astrophysics ECLA2020, Sep 2021, Anacapri, Italy. pp.271 - 279
The nucleus of comet 67P/Churyumov-Gerasimenko exhibits a broad spectral reflectance feature around 3.2 $\mu$m, which is omnipresent in all spectra of the surface, and whose attribution has remained elusive since its discovery. Based on laboratory ex
Externí odkaz:
http://arxiv.org/abs/2311.11712
Autor:
Béthermin, M., Accard, C., Guillaume, C., Dessauges-Zavadsky, M., Ibar, E., Cassata, P., Devereaux, T., Faisst, A., Freundlich, J., Jones, G. C., Kraljic, K., Algera, H., Amorin, R. O., Bardelli, S., Boquien, M., Buat, V., Donghia, E., Dubois, Y., Ferrara, A., Fudamoto, Y., Ginolfi, M., Guillard, P., Giavalisco, M., Gruppioni, C., Gururajan, G., Hathi, N., Hayward, C. C., Koekemoer, A. M., Lemaux, B. C., Magdis, G. E., Molina, J., Narayanan, D., Mayer, L., Pozzi, F., Rizzo, F., Romano, M., Tasca, L., Theulé, P., Vergani, D., Vallini, L., Zamorani, G., Zanella, A., Zucca, E.
The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density ($\Sigma_{\rm gas}$-$\Sigma_{\rm SFR}$) is essential to understand star formation processes in galaxies. So far, it has been measured up to z~2.5 in
Externí odkaz:
http://arxiv.org/abs/2311.08474
Autor:
Gururajan, G., Béthermin, M., Sulzenauer, N., Theulé, P., Spilker, J. S., Aravena, M., Chapman, S. C., Gonzalez, A., Greve, T. R., Narayanan, D., Reuter, C., Vieira, J. D., Weiss, A.
Publikováno v:
A&A 676, A89 (2023)
The nature and evolution of high-redshift dusty star-forming galaxies (high-z DSFGs) remain an open question. Their massive gas reservoirs play an important role in driving the intense star-formation rates hosted in these galaxies. We aim to estimate
Externí odkaz:
http://arxiv.org/abs/2306.03153
Autor:
Burgarella, Denis, Theulé, Patrice, Buat, Véronique, Gouiran, Lisa, Turco, Lorie, Boquien, Médéric, Bakx, Tom J. L. C., Inoue, Akio K., Fudamoto, Yoshinobu, Sugahara, Yuma, Zavala, Jorge
Publikováno v:
A&A 671, A123 (2023)
Infrared (IR), sub-millimetre (sub-mm) and millimetre (mm) databases contain a huge quantity of high quality data. However, a large part of these data are photometric, and are thought not to be useful to derive a quantitative information on the nebul
Externí odkaz:
http://arxiv.org/abs/2211.05744
Autor:
Mountrichas, G., Buat, V., Yang, G., Boquien, M., Ni, Q., Pouliasis, E., Burgarella, D., Theule, P., Georgantopoulos, I.
Publikováno v:
A&A 667, A145 (2022)
We use AGN with $\rm L_{X} \sim 10^{42.5-44}\,erg\,s^{-1}$, from the COSMOS-Legacy survey that lie within the UltraVISTA region and cross match them with the LEGA-C catalogue. The latter provides measurements of the calcium break, D$_n$4000, and H$_\
Externí odkaz:
http://arxiv.org/abs/2209.06960
Autor:
Gavdush, A. A., Kruczkiewicz, F., Giuliano, B. M., Müller, B., Komandin, G. A., Grassi, T., Theulé, P., Zaytsev, K. I., Ivlev, A. V., Caselli, P.
Publikováno v:
A&A 667, A49 (2022)
Context: Broadband optical constants of astrophysical ice analogues in the infrared (IR) and terahertz (THz) ranges are required for modeling the dust continuum emission and radiative transfer in dense and cold regions, where thick icy mantles are fo
Externí odkaz:
http://arxiv.org/abs/2207.11052
Autor:
Schutzer, A. de A., Rivera-Ortiz, P. R., Lefloch, B., Gusdorf, A., Favre, C., Segura-Cox, D., Lopez-Sepulcre, A., Neri, R., Ospina-Zamudio, J., De Simone, M., Codella, C., Viti, S., Podio, L., Pineda, J., O'Donoghue, R., Ceccarelli, C., Caselli, P., Alves, F., Bachiller, R., Balucani, N., Bianchi, E., Bizzocchi, L., Bottinelli, S., Caux, E., Chacón-Tanarro, A., Dulieu, F., Enrique-Romero, J., Fontani, F., Feng, S., Holdship, J., Jiménez-Serra, I., Al-Edhari, A. Jaber, Kahane, C., Lattanzi, V., Oya, Y., Punanova, A., Rimola, A., Sakai, N., Spezzano, S., Sims, I. R., Taquet, V., Testi, L., Theulé, P., Ugliengo, P., Vastel, C., Vasyunin, A. I., Vazart, F., Yamamoto, S., Witzel, A.
Publikováno v:
A&A 662, A104 (2022)
Protostellar jets are an important agent of star formation feedback, tightly connected with the mass-accretion process. The history of jet formation and mass-ejection provides constraints on the mass accretion history and the nature of the driving so
Externí odkaz:
http://arxiv.org/abs/2203.09383
Autor:
Burgarella, D., Bogdanoska, J., Nanni, A., Bardelli, S., Bethermin, M., Boquien, M., Buat, V., Faisst, A. L., Dessauges-Zavadsky, M., Fudamoto, Y., Fujimoto, S., Giavalisco, M., Ginolfi, M., Gruppioni, C., Hathi, N. P., Ibar, E., Jones, G. C., Koekemoer, A. M., Kohno, K., Lemaux, B. C., Narayanan, D., Oesch, P., Ouchi, M., Riechers, D. A., Pozzi, F., Romano, M., Schaerer, D., Talia, M., Theule, P., Vergani, D., Zamorani, G., Zucca, E., Cassata, P., team, the ALPINE
Publikováno v:
A&A 664, A73 (2022)
The luminosity functions at z < 4 - 5 suggest that most galaxies have a relatively low stellar mass (logM_star = 10) and a low dust attenuation (A_FUV = 1.0). The physical properties of these objects are quite homogeneous. We used an approach where w
Externí odkaz:
http://arxiv.org/abs/2203.02059