Zobrazeno 1 - 10
of 595
pro vyhledávání: '"Curti, M"'
Autor:
Marconcini, C., D'Eugenio, F., Maiolino, R., Arribas, S., Bunker, A., Carniani, S., Charlot, S., Perna, M., Del Pino, B. Rodríguez, Übler, H., Pérez-González, P. G., Willott, C. J., Böker, T., Cresci, G., Curti, M., Lamperti, I., Scholtz, J., Parlanti, E., Venturi, G.
We present JWST/NIRSpec integral field spectroscopic (IFS) observations of the \Lyalpha emitter CR7 at z ~ 6.6, observed as part of the GA-NIFS program. Using low-resolution PRISM (R ~ 100) data, we confirm a bright \Lyalpha emitter, and a diffuse \L
Externí odkaz:
http://arxiv.org/abs/2411.08627
Autor:
Scholtz, J., Curti, M., D'Eugenio, F., Übler, H., Maiolino, R., Marconcini, C., Smit, R., Perna, M., Witstok, J., Arribas, S., Böker, T., Bunker, A. J., Carniani, S., Charlot, S., Cresci, G., Pérez-González, P. G., Lamperti, I., Del Pino, B. Rodríguez, Parlanti, E., Venturi, G.
We present deep JWST/NIRSpec integral-field spectroscopy (IFS) and ALMA [CII]$\lambda$158$\mu$m observations of COS-3018, a star-forming galaxy at z$\sim$6.85, as part of the GA-NIFS programme. Both G395H (R$\sim$ 2700) and PRISM (R$\sim$ 100) NIRSpe
Externí odkaz:
http://arxiv.org/abs/2411.07695
Autor:
Simmonds, C., Tacchella, S., Hainline, K., Johnson, B. D., Puskás, D., Robertson, B., Baker, W. M., Bhatawdekar, R., Boyett, K., Bunker, A. J., Cargile, P. A., Carniani, S., Chevallard, J., Curti, M., Curtis-Lake, E., Ji, Z., Jones, G. C., Kumari, N., Laseter, I., Maiolino, R., Maseda, M. V., Rinaldi, P., Stoffers, A., Übler, H., Villanueva, N. C., Williams, C. C., Willot, C., Witstok, J., Zhu, Y.
We use NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) to study the ionising properties of a sample of 15721 galaxies at $3 \leq z_{\rm{phot}} \leq 9$, 90\% complete in stellar mass down to log(M$_{\star}$/[M$_{\odot}$])$\appr
Externí odkaz:
http://arxiv.org/abs/2409.01286
Autor:
Pierel, J. D. R., Engesser, M., Coulter, D. A., Decoursey, C., Siebert, M. R., Rest, A., Egami, E., Chen, W., Fox, O. D., Jones, D. O., Joshi, B. A., Moriya, T. J., Zenati, Y., Bunker, A. J., Cargile, P. A., Curti, M., Eisenstein, D. J., Gezari, S., Gomez, S., Guolo, M., Johnson, B. D., Karmen, M., Maiolino, R., Quimby, Robert M., Robertson, B., Shahbandeh, M., Strolger, L. G., Sun, F., Wang, Q., Wevers, T.
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS$+53.13485$$-$$27.82088$ with a host spectroscopic redshift of $2.903\pm0.007$. The transient was identified in deep James Webb Space Telescope (JWST)/N
Externí odkaz:
http://arxiv.org/abs/2406.05089
Autor:
Siebert, M. R., Decoursey, C., Coulter, D. A., Engesser, M., Pierel, J. D. R., Rest, A., Egami, E., Shahbandeh, M., Chen, W., Fox, O. D., Zenati, Y., Moriya, T. J., Bunker, A. J., Cargile, P. A., Curti, M., Eisenstein, D. J., Gezari, S., Gomez, S., Guolo, M., Johnson, B. D., Joshi, B. A., Karmen, M., Maiolino, R., Quimby, R. M., Robertson, B., Strolger, L. G., Sun, F., Wang, Q., Wevers, T.
We present JWST NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at $z = 2.83$. This SN (named SN 2023adta) was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from th
Externí odkaz:
http://arxiv.org/abs/2406.05076
Autor:
Mazzolari, G., Übler, H., Maiolino, R., Ji, X., Nakajima, K., Feltre, A., Scholtz, J., D'Eugenio, F., Curti, M., Mignoli, M., Marconi, A.
The James Webb Space Telescope (JWST) is revolutionizing our understanding of black holes formation and growth in the early Universe. However, JWST has also revealed that some of the classical diagnostics, such as the BPT diagrams and X-ray emission,
Externí odkaz:
http://arxiv.org/abs/2404.10811
Autor:
Venturi, G., Carniani, S., Parlanti, E., Kohandel, M., Curti, M., Pallottini, A., Vallini, L., Arribas, S., Bunker, A. J., Cameron, A. J., Castellano, M., Ferrara, A., Fontana, A., Gallerani, S., Gelli, V., Maiolino, R., Ntormousi, E., Pacifici, C., Pentericci, L., Salvadori, S., Vanzella, E.
Publikováno v:
A&A 691, A19 (2024)
The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the early Universe. Here we study the spatially resolved metallicity in three
Externí odkaz:
http://arxiv.org/abs/2403.03977
Autor:
Marconi, A., Amiri, A., Feltre, A., Belfiore, F., Cresci, G., Curti, M., Mannucci, F., Bertola, E., Brazzini, M., Carniani, S., Cataldi, E., D'Amato, Q., de Rosa, G., Di Teodoro, E., Ginolfi, M., Kumari, N., Marconcini, C., Maiolino, R., Magrini, L., Marasco, A., Mingozzi, M., Moreschini, B., Nagao, T., Oliva, E., Scialpi, M., Tomicic, N., Tozzi, G., Ulivi, L., Venturi, G.
Publikováno v:
A&A 689, A78 (2024)
We present HOMERUN (Highly Optimized Multi-cloud Emission-line Ratios Using photo-ionizatioN), a new approach to modelling emission lines from photoionized gas that can simultaneously reproduce all observed line intensities from a wide range of ioniz
Externí odkaz:
http://arxiv.org/abs/2401.13028
Autor:
Del Pino, B. Rodríguez, Perna, M., Arribas, S., D'Eugenio, F., Lamperti, I., Pérez-González, P. G., Übler, H., Bunker, A., Carniani, S., Charlot, S., Maiolino, R., Willott, C. J., Böker, T., Chevallard, J., Cresci, G., Curti, M., Jones, G. C., Parlanti, E., Scholtz, J., Venturi, G.
We present NIRSpec IFS observations of a galaxy group around the massive GS_4891 galaxy at z=3.7 in GOODS-South that includes two other two systems, GS_4891_n to the north and GS_28356 to the east. These observations, obtained as part of the GTO GA-N
Externí odkaz:
http://arxiv.org/abs/2309.14431
Autor:
Jones, G. C., Ubler, H., Perna, M., Arribas, S., Bunker, A. J., Carniani, S., Charlot, S., Maiolino, R., Del Pino, B. Rodriguez, Willott, C., Bowler, R. A. A., Boker, T., Cameron, A. J., Chevallard, J., Cresci, G., Curti, M., D'Eugenio, F., Kumari, N., Saxena, A., Scholtz, J., Venturi, G., Witstok, J.
Massive, starbursting galaxies in the early Universe represent some of the most extreme objects in the study of galaxy evolution. One such source is HFLS3 (z~6.34), which was originally identified as an extreme starburst galaxy with mild gravitationa
Externí odkaz:
http://arxiv.org/abs/2308.16620