Zobrazeno 1 - 10
of 20 650
pro vyhledávání: '"A Camus"'
Publikováno v:
European Cells & Materials, Vol 45, Pp 72-87 (2023)
Intervertebral disc degeneration (IDD) involves cellular changes in the nucleus pulposus (NP) characterised by a decline of the large vacuolated notochordal cells (vNCs) and a rise of smaller vacuole-free mature chondrocyte-like NP cells. An increasi
Externí odkaz:
https://doaj.org/article/a44e13446ca14b588779ec04fba55c06
Autor:
Telikova, K., González-López, J., Aravena, M., Posses, A., Villanueva, V., Baeza-Garay, M., Jones, G. C., Solimano, M., Lee, L., Assef, R. J., De Looze, I., Santos, T. Diaz, Ferrara, A., Ikeda, R., Herrera-Camus, R., Übler, H., Lamperti, I., Mitsuhashi, I., Relano, M., Perna, M., Tadaki, K.
The history of gas assembly in early galaxies is reflected in their complex kinematics. While a considerable fraction of galaxies at z~5 are consistent with rotating disks, current studies indicate that the dominant galaxy assembly mechanism correspo
Externí odkaz:
http://arxiv.org/abs/2411.09033
Autor:
Lee, Lilian L., Schreiber, Natascha M. Förster, Price, Sedona H., Liu, Daizhong, Genzel, Reinhard, Davies, Richard I, Tacconi, Linda J., Shimizu, Thomas T., Shachar, Amit Nestor, Salcedo, Juan M. Espejo, Pastras, Stavros, Wuyts, Stijn, Lutz, Dieter, Renzini, Alvio, Übler, Hannah D., Herrera-Camus, Rodrigo, Sternberg, Amiel
Spatially-resolved emission line kinematics are invaluable to investigating fundamental galaxy properties and have become increasingly accessible for galaxies at $z\gtrsim0.5$ through sensitive near-infrared imaging spectroscopy and millimeter interf
Externí odkaz:
http://arxiv.org/abs/2411.07312
Autor:
Arriagada-Neira, Sebastián, Herrera-Camus, Rodrigo, Villanueva, Vicente, Schreiber, Natascha M. Förster, Lee, Minju, Bolatto, Alberto, Chen, Jianhang, Genzel, Reinhard, Liu, Daizhong, Renzini, Alvio, Tacconi, Linda J., Tozzi, Giulia, Übler, Hannah
We present deep ($\sim$ 20 hr), high-angular resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations of the $\rm CO ~ (4-3)$ and $\rm [CI] ~ (1-0)$ transitions, along with the rest-frame 630 $\mu$m dust continuum, in BX610 --a mas
Externí odkaz:
http://arxiv.org/abs/2410.14781
Autor:
Li, Juno, Da Cunha, Elisabete, González-López, Jorge, Aravena, Manuel, De Looze, Ilse, Schreiber, N. M. Förster, Herrera-Camus, Rodrigo, Spilker, Justin, Tadaki, Ken-ichi, Barcos-Munoz, Loreto, Battisti, Andrew J., Birkin, Jack E., Bowler, Rebecca A. A., Davies, Rebecca, Díaz-Santos, Tanio, Ferrara, Andrea, Fisher, Deanne B., Hodge, Jacqueline, Ikeda, Ryota, Killi, Meghana, Lee, Lilian, Liu, Daizhong, Lutz, Dieter, Mitsuhashi, Ikki, Naab, Thorsten, Posses, Ana, Relaño, Monica, Solimano, Manuel, Übler, Hannah, van der Giessen, Stefan Anthony, Villanueva, Vicente
Using a combination of HST, JWST, and ALMA data, we perform spatially resolved spectral energy distributions (SED) fitting of fourteen 4
Externí odkaz:
http://arxiv.org/abs/2409.10961
Autor:
Lines, N. E. P., Bowler, R. A. A., Adams, N. J., Fisher, R., Varadaraj, R. G., Nakazato, Y., Aravena, M., Assef, R. J., Birkin, J. E., Ceverino, D., da Cunha, E., Cullen, F., De Looze, I., Donnan, C. T., Dunlop, J. S., Ferrara, A., Grogin, N. A., Herrera-Camus, R., Ikeda, R., Koekemoer, A. M., Killi, M., Li, J., McLeod, D. J., McLure, R. J., Mitsuhashi, I., Pérez-González, P. G., Relano, M., Solimano, M., Spilker, J. S., Villanueva, V., Yoshida, N.
We present a spatially resolved analysis of four star-forming galaxies at $z = 4.44-5.64$ using data from the JWST PRIMER and ALMA-CRISTAL surveys to probe the stellar and inter-stellar medium properties on the sub-kpc scale. In the $1-5\,\mu{\rm m}$
Externí odkaz:
http://arxiv.org/abs/2409.10963
Publikováno v:
International Conference on Radar (Radar 2024), SEE Society, Oct 2024, Rennes, France
In this paper, we detail the high-performance implementation of our spaceborne radar simulator for satellite oceanography. Our software simulates the sea surface and the signal to imitate, as far as possible, the measurement process, starting from it
Externí odkaz:
http://arxiv.org/abs/2408.11472
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, Bowler, Rebecca A. A., 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 and structure 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 interferometric visibility, we derive the effective radius of [C
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