Zobrazeno 1 - 10
of 1 145
pro vyhledávání: '"D'Eugenio, F"'
Autor:
Ulivi, L., Perna, M., Lamperti, I., Arribas, S., Cresci, G., Del Pino, B. Rodríguez, Boeker, T., Bunker, A. J., Ceci, M., Charlot, S., Eugenio, F. D, Fahrion, K., Maiolino, R., Marconi, A., Pereira-Santaella, M.
The study of starburst and AGN feedback is crucial for understanding the regulation of star formation and the evolution of galaxies across cosmic time. Arp 220, the closest ultraluminous infrared galaxy (ULIRG), is in an advanced phase of a major mer
Externí odkaz:
http://arxiv.org/abs/2407.08505
Autor:
Bagge, R. S., Foster, C., D'Eugenio, F., Battisti, A., Bellstedt, S., Derkenne, C., Vaughan, S., Mendel, T., Barsanti, S., Harborne, K. E., Croom, S. M., Bland-Hawthorn, J., Grasha, K., Lagos, C. D. P., Sweet, S. M., Mailvaganam, A., Mukherjee, T., Valenzuela, L. M., van de Sande, J., Wisnioski, E., Zafar, T.
We present a study of kinematic asymmetries from the integral field spectroscopic surveys MAGPI and SAMI. By comparing the asymmetries in the ionsied gas and stars, we aim to disentangle the physical processes that contribute to kinematic disturbance
Externí odkaz:
http://arxiv.org/abs/2405.11292
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:
Croom, S. M., van de Sande, J., Vaughan, S. P., Rutherford, T. H., Lagos, C. P., Barsanti, S., Bland-Hawthorn, J., Brough, S., Bryant, J. J., Colless, M., Cortese, L., D'Eugenio, F., Fraser-McKelvie, A., Goodwin, M., Lorente, N. P. F., Richards, S. N., Ristea, A., Sweet, S. M., Yi, S. K., Zafar, T.
Publikováno v:
MNRAS, Volume 529, Issue 4, April 2024, Pages 3446-3468
We use the SAMI Galaxy Survey to examine the drivers of galaxy spin, $\lambda_{R_e}$, in a multi-dimensional parameter space including stellar mass, stellar population age (or specific star formation rate) and various environmental metrics (local den
Externí odkaz:
http://arxiv.org/abs/2402.06877
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
Saliency maps have become one of the most widely used interpretability techniques for convolutional neural networks (CNN) due to their simplicity and the quality of the insights they provide. However, there are still some doubts about whether these i
Externí odkaz:
http://arxiv.org/abs/2309.12913
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
Autor:
Perna, M., Arribas, S., Marshall, M., D'Eugenio, F., Übler, H., Bunker, A., Charlot, S., Carniani, S., Jakobsen, P., Maiolino, R., Del Pino, B. Rodríguez, Willott, C. J., Böker, T., Circosta, C., Cresci, G., Curti, M., Husemann, B., Kumari, N., Lamperti, I., Pérez-González, P. G., Scholtz, J.
Publikováno v:
A&A 679, A89 (2023)
LBQS 0302-0019 is a blue quasar (QSO) at z ~ 3.3, hosting powerful outflows, and residing in a complex environment consisting of an obscured AGN candidate, and multiple companions, all within 30 kpc in projection. We use JWST NIRSpec IFS observations
Externí odkaz:
http://arxiv.org/abs/2304.06756
Autor:
Robertson, B. E., Tacchella, S., Johnson, B. D., Hainline, K., Whitler, L., Eisenstein, D. J., Endsley, R., Rieke, M., Stark, D. P., Alberts, S., Dressler, A., Egami, E., Hausen, R., Rieke, G., Shivaei, I., Williams, C. C., Willmer, C. N. A., Arribas, S., Bonaventura, N., Bunker, A., Cameron, A. J., Carniani, S., Charlot, S., Chevallard, J., Curti, M., Curtis-Lake, E., D'Eugenio, F., Jakobsen, P., Looser, T. J., Lützgendorf, N., Maiolino, R., Maseda, M. V., Rawle, T., Rix, H. -W., Smit, R., Übler, H., Willott, C., Witstok, J., Baum, S., Bhatawdekar, R., Boyett, K., Chen, Z., de Graaff, A., Florian, M., Helton, J. M., Hviding, R. E., Ji, Z., Kumari, N., Lyu, J., Nelson, E., Sandles, L., Saxena, A., Suess, K. A., Sun, F., Topping, M., Wallace, I. E. B.
Surveys with James Webb Space Telescope (JWST) have discovered candidate galaxies in the first 400 Myr of cosmic time. Preliminary indications have suggested these candidate galaxies may be more massive and abundant than previously thought. However,
Externí odkaz:
http://arxiv.org/abs/2212.04480