Zobrazeno 1 - 10
of 1 282
pro vyhledávání: '"Belli S."'
Autor:
Pierel, J. D. R., Newman, A. B., Dhawan, S., Gu, M., Joshi, B. A., Li, T., Schuldt, S., Strolger, L. G., Suyu, S. H., Caminha, G. B., Cohen, S. H., Diego, J. M., Dsilva, J. C. J., Ertl, S., Frye, B. L., Granata, G., Grillo, C., Koekemoer, A. M., Li, J., Robotham, A., Summers, J., Treu, T., Windhorst, R. A., Zitrin, A., Agarwal, S., Agrawal, A., Arendse, N., Belli, S., Burns, C., Cañameras, R., Chakrabarti, S., Chen, W., Collett, T. E., Coulter, D. A., Ellis, R. S., Engesser, M., Foo, N., Fox, O. D., Gall, C., Garuda, N., Gezari, S., Gomez, S., Glazebrook, K., Hjorth, J., Huang, X., Jha, S. W., Kamieneski, P. S., Kelly, P., Larison, C., Moustakas, L. A., Pascale, M., Pérez-Fournon, I., Petrushevska, T., Poidevin, F., Rest, A., Shahbandeh, M., Shajib, A. J., Siebert, M., Storfer, C., Talbot, M., Wang, Q., Wevers, T., Zenati, Y.
A bright ($m_{\rm F150W,AB}$=24 mag), $z=1.95$ supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply-imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detecte
Externí odkaz:
http://arxiv.org/abs/2404.02139
Post-starburst galaxies are sources that had the last major episode of star formation about 1 Gyr before the epoch of the observations and are on their way to quiescence. It is important to study such galaxies at redshift z > 1, during their main que
Externí odkaz:
http://arxiv.org/abs/2306.08120
Autor:
Popesso, P., Concas, A., Cresci, G., Belli, S., Rodighiero, G., Inami, H., Dickinson, M., Ilbert, O., Pannella, M., Elbaz, D.
By compiling a comprehensive census of literature studies, we investigate the evolution of the Main Sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift ($0 < z < 6$) and stellar mass ($10^{8.5}-10^{11.5}$ $M_{\odot}$) ever p
Externí odkaz:
http://arxiv.org/abs/2203.10487
Autor:
Davies, Rebecca L., Schreiber, N. M. Förster, Genzel, R., Shimizu, T. T., Davies, R. I., Schruba, A., Tacconi, L. J., Übler, H., Wisnioski, E., Wuyts, S., Fossati, M., Herrera-Camus, R., Lutz, D., Mendel, J. T., Naab, T., Price, S. H., Renzini, A., Wilman, D., Beifiori, A., Belli, S., Burkert, A., Chan, J., Contursi, A., Fabricius, M., Lee, M. M., Saglia, R. P., Sternberg, A.
We investigate what drives the redshift evolution of the typical electron density ($n_e$) in star-forming galaxies, using a sample of 140 galaxies drawn primarily from KMOS$^{\rm 3D}$ ($0.6\lesssim{z}\lesssim{2.6}$) and 471 galaxies from SAMI ($z<0.1
Externí odkaz:
http://arxiv.org/abs/2012.10445
Autor:
Davies, Rebecca L., Schreiber, N. M. Förster, Lutz, D., Genzel, R., Belli, S., Shimizu, T. T., Contursi, A., Davies, R. I., Herrera-Camus, R., Lee, M. M., Naab, T., Price, S. H., Renzini, A., Schruba, A., Sternberg, A., Tacconi, L. J., Übler, H., Wisnioski, E., Wuyts, S.
We use deep adaptive optics assisted integral field spectroscopy from SINFONI on the VLT to study the spatially resolved properties of ionized gas outflows driven by active galactic nuclei (AGN) in three galaxies at z~2.2 -- K20-ID5, COS4-11337 and J
Externí odkaz:
http://arxiv.org/abs/2004.02891
Autor:
Wilman, D. J., Fossati, M., Mendel, J. T., Saglia, R., Wisnioski, E., Wuyts, S., Schreiber, N. Förster, Beifiori, A., Bender, R., Belli, S., Übler, H., Lang, P., Chan, J. C. C., Davies, R. L., Nelson, E. J., Genzel, R., Tacconi, L. J., Galametz, A., Davies, R. I., Lutz, D., Price, S., Burkert, A., Tadaki, K., Herrera-Camus, R., Brammer, G., Momcheva, I., van Dokkum, P.
We present half-light sizes measured from H${\alpha}$ emission tracing star-formation in 281 star-forming galaxies from the KMOS3D survey at 0.7 < z < 2.7. Sizes are derived by fitting 2D exponential disk models, with bootstrap errors averaging 20%.
Externí odkaz:
http://arxiv.org/abs/2002.09499
Autor:
Wisnioski, E., Schreiber, N. M. Förster, Fossati, M., Mendel, J. T., Wilman, D., Genzel, R., Bender, R., Wuyts, S., Davies, R. L., Übler, H., Bandara, K., Beifiori, A., Belli, S., Brammer, G., Chan, J., Davies, R. I., Fabricius, M., Galametz, A., Lang, P., Lutz, D., Nelson, E. J., Momcheva, I., Price, S., Rosario, D., Saglia, R., Seitz, S., Shimizu, T., Tacconi, L. J., Tadaki, K., van Dokkum, P. G., Wuyts, E.
We present the completed KMOS$^\mathrm{3D}$ survey $-$ an integral field spectroscopic survey of 739, $\log(M_{\star}/M_{\odot})>9$, galaxies at $0.6
Externí odkaz:
http://arxiv.org/abs/1909.11096
Autor:
Popesso, P., Morselli, L., Concas, A., Schreiber, C., Rodighiero, G., Cresci, G., Belli, S., Ilbert, O., Erfanianfar, G., Mancini, C., Inami, H., Dickinson, M., Pannella, M., Elbaz, D.
By using the deepest available mid and far infrared surveys in the CANDELS, GOODS and COSMOS fields we study the evolution of the Main Sequence (MS) of star forming galaxies (SFGs) from z~0 to` ~2.5 at stellar masses larger than 10^{10} M_{\odot}. Th
Externí odkaz:
http://arxiv.org/abs/1909.07760
Autor:
Popesso, P., Concas, A., Morselli, L., Schreiber, C., Rodighiero, G., Cresci, G., Belli, S., Erfanianfar, G., Mancini, C., Inami, H., Dickinson, M., Ilbert, O., Pannella, M., Elbaz, D.
By using a set of different SFR indicators, including WISE mid-infrared and Halpha emission, we study the slope of the Main Sequence (MS) of local star forming galaxies at stellar masses larger than 10^{10} M_{\odot}. The slope of the relation strong
Externí odkaz:
http://arxiv.org/abs/1812.07057
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