Zobrazeno 1 - 10
of 6 154
pro vyhledávání: '"Camus P"'
Autor:
Levy, Rebecca C., Bolatto, Alberto D., Mayya, Divakara, Cuevas-Otahola, Bolivia, Tarantino, Elizabeth, Boyer, Martha L., Boogaard, Leindert A., Böker, Torsten, Cronin, Serena A., Dale, Daniel A., Donaghue, Keaton, Emig, Kimberly L., Fisher, Deanne B., Glover, Simon C. O., Herrera-Camus, Rodrigo, Jiménez-Donaire, María J., Klessen, Ralf S., Lenkić, Laura, Leroy, Adam K., De Looze, Ilse, Meier, David S., Mills, Elisabeth A. C., Ott, Juergen, Relaño, Mónica, Veilleux, Sylvain, Villanueva, Vicente, Walter, Fabian, van der Werf, Paul P.
We present a near infrared (NIR) candidate star cluster catalog for the central kiloparsec of M82 based on new JWST NIRCam images. We identify star cluster candidates using the F250M filter, finding 1357 star cluster candidates with stellar masses $>
Externí odkaz:
http://arxiv.org/abs/2408.04135
Autor:
Ikeda, Ryota, Tadaki, Ken-ichi, Mitsuhashi, Ikki, Aravena, Manuel, De Looze, Ilse, Schreiber, Natascha M. Förster, González-López, Jorge, Herrera-Camus, Rodrigo, Spilker, Justin, Barcos-Muñoz, Loreto, da Cunha, Elisabete, Davies, Rebecca, Díaz-Santos, Tanio, Ferrara, Andrea, Killi, Meghana, Lee, Lilian L., Li, Juno, Lutz, Dieter, Smit, Renske, Solimano, Manuel, Telikova, Kseniia, Übler, Hannah, Veilleux, Sylvain, Villanueva, Vicente
We investigate the spatial extent of the [CII] line emission in a sample of 34 galaxies at $z=4-6$ from the ALMA-CRISTAL Survey. By modeling the [CII] line emission in the visibility data directly, we derive the effective radius of [CII] line emissio
Externí odkaz:
http://arxiv.org/abs/2408.03374
Autor:
Lenkić, Laura, Fisher, Deanne B., Bolatto, Alberto D., Teuben, Peter J., Levy, Rebecca C., Sun, Jiayi, Herrera-Camus, Rodrigo, Glazebrook, Karl, Obreschkow, Danail, Abraham, Roberto
The gas-phase velocity dispersions in disk galaxies, which trace turbulence in the interstellar medium, are observed to increase with lookback time. However, the mechanisms that set this rise in turbulence are observationally poorly constrained. To a
Externí odkaz:
http://arxiv.org/abs/2408.02730
Autor:
Parlanti, Eleonora, Carniani, Stefano, Venturi, Giacomo, Herrera-Camus, Rodrigo, Arribas, Santiago, Bunker, Andrew J., Charlot, Stephane, D'Eugenio, Francesco, Maiolino, Roberto, Perna, Michele, Übler, Hannah, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Lamperti, Isabella, Zamora, Sandra
Galactic outflows driven by star formation or active galactic nuclei are typically formed by multi-phase gas whose temperature spans over 4 orders of magnitude. Probing the different outflow components requires multi-wavelength observations and long
Externí odkaz:
http://arxiv.org/abs/2407.19008
We propose and implement an optical technique to access the local temperature of an erbium doped crystal by probing the electron spin population under magnetic field. We reliably extract the sample temperature in the range 2-7K. We additionally discu
Externí odkaz:
http://arxiv.org/abs/2407.14222
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
We present new JWST/NIRSpec IFU observations of the J1000+0234 system at $z=4.54$, the dense core of a galaxy protocluster hosting a massive, dusty star forming galaxy (DSFG) with a low luminosity radio counterpart. The new data reveals two extended,
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Villanueva, V., Herrera-Camus, R., Gonzalez-Lopez, J., Aravena, M., Assef, R. J., Baeza-Garay, Mauricio, Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., da Cunha, E., De Looze, I., Diaz-Santos, T., Ferrara, A., Foerster-Schreiber, N., Algera, H., Iked, R., Killi, M., Mitsuhashi, I., Naab, T., Relano, M., Spilker, J., Solimano, M., Palla, M., Price, S. H., Posses, A., Tadaki, K., Telikova, K., Übler, H.
We present new $\lambda_{\rm rest}=77$ $\mu$m dust continuum observations from the ALMA of HZ10 (CRISTAL-22), a dusty main-sequence galaxy at $z$=5.66 as part of the [CII] Resolved Ism in STar-forming Alma Large program, CRISTAL. The high angular res
Externí odkaz:
http://arxiv.org/abs/2407.09681
Autor:
Chen, Yuguang, Jones, Tucker, Sanders, Ryan L., Fadda, Dario, Sutter, Jessica, Minchin, Robert, Prusinski, Nikolaus Z., Rhoades, Sunny, GC, Keerthi Vasan, Steidel, Charles C., Huntzinger, Erin, Kelly, Paige, Berg, Danielle A., Bresolin, Fabio, Herrera-Camus, Rodrigo, Vaught, Ryan J. Rickards, Roberts-Borsani, Guido, Senchyna, Peter, Spilker, Justin S., Stark, Daniel P., Weiner, Benjamin, Martin, D. Christopher, Matuszewski, Mateusz, McGurk, Rosalie C., Neill, James D.
Accurate chemical compositions of star-forming regions are a critical diagnostic tool to characterize the star formation history and gas flows which regulate galaxy formation. However, the abundance discrepancy factor (ADF) between measurements from
Externí odkaz:
http://arxiv.org/abs/2405.18476
Autor:
Jones, Gareth C., Bunker, Andrew J., Telikova, Kseniia, Arribas, Santiago, Carniani, Stefano, Charlot, Stephane, D'Eugenio, Francesco, Maiolino, Roberto, Perna, Michele, Del Pino, Bruno Rodriguez, Ubler, Hannah, Willott, Chris, Aravena, Manuel, Boker, Torsten, Cresci, Giovanni, Curti, Mirko, Herrera-Camus, Rodrigo, Lamperti, Isabella, Parlanti, Eleonora, Perez-Gonzalez, Pablo G., Villanueva, Vicente
We present observations of the $z\sim5.7$ Lyman-break galaxy HZ10 with the JWST/NIRSpec IFU in high and low spectral resolution (G395H, $R\sim2700$ and PRISM, $R\sim100$, respectively), as part of the GA-NIFS program. By spatially resolving the sourc
Externí odkaz:
http://arxiv.org/abs/2405.12955
In this paper, we introduce HEEPS/MARE, the end-to-end simulator developed for the SAR oceanographic products of ESA Earth Explorer 10 mission, Harmony, expected to launch in Decembre 2029. Harmony is primarily dedicated to the observation of small-s
Externí odkaz:
http://arxiv.org/abs/2405.09938