Zobrazeno 1 - 10
of 2 026
pro vyhledávání: '"P. Aloisi"'
Autor:
Li, Jiazheng, Xu, Hainiu, Sun, Zhaoyue, Zhou, Yuxiang, West, David, Aloisi, Cesare, He, Yulan
Generating rationales that justify scoring decisions has been a promising way to facilitate explainability in automated scoring systems. However, existing methods do not match the accuracy of classifier-based methods. Plus, the generated rationales o
Externí odkaz:
http://arxiv.org/abs/2406.19949
Autor:
Abril-Melgarejo, Valentina, James, Bethan L., Aloisi, Alessandra, Mingozzi, Matilde, Lebouteiller, Vianney, Hernandez, Svea, Kumari, Nimisha
We present a pioneering spatially-resolved, multi-phase gas abundance study on the blue compact dwarf galaxy NGC~5253, targeting 10 star-forming (SF) clusters inside six FUV HST/COS pointings with co-spatial optical VLT/MUSE observations throughout t
Externí odkaz:
http://arxiv.org/abs/2406.16553
Autor:
Sirressi, Mattia, Adamo, Angela, Hayes, Matthew, Rivera-Thorsen, Thøger Emil, Aloisi, Alessandra, Bik, Arjan, Calzetti, Daniela, Chisholm, John, Fox, Andrew J., Fumagalli, Michele, Grasha, Kathryn, Hernandez, Svea, Messa, Matteo, Osborne, Shannon, Östlin, Göran, Sabbi, Elena, Schinnerer, Eva, Smith, Linda J., Usher, Christopher, Wofford, Aida
We analyze the far-ultraviolet spectroscopy of 20 young and massive star clusters (YSCs) in 11 nearby star-forming galaxies. We probe the interstellar gas intervening along the line of sight, detecting several metal absorption lines of a wide range o
Externí odkaz:
http://arxiv.org/abs/2402.10270
Autor:
Finn, Molly K., Johnson, Kelsey E., Indebetouw, Remy, Costa, Allison H., Adamo, Angela, Aloisi, Alessandra, Bittle, Lauren, Calzetti, Daniela, Dale, Daniel A., Dobbs, Clare L., Meyer, Jennifer Donovan, Elmegreen, Bruce G., Elmegreen, Debra M., Fumagalli, Michele, Gallagher, J. S., Grasha, Kathryn, Grebel, Eva K., Kennicutt, Robert C., Krumholz, Mark R., Lee, Janice C., Messa, Matteo, Nair, Preethi, Sabbi, Elena, Smith, Linda J., Thilker, David A., Whitmore, Bradley C., Wofford, Aida
We compare the molecular cloud properties in sub-galactic regions of two galaxies, barred spiral NGC 1313, which is forming many massive clusters, and flocculent spiral NGC 7793, which is forming significantly fewer massive clusters despite having a
Externí odkaz:
http://arxiv.org/abs/2401.01451
Autor:
Finn, Molly K., Johnson, Kelsey E., Indebetouw, Remy, Costa, Allison H., Adamo, Angela, Aloisi, Alessandra, Bittle, Lauren, Calzetti, Daniela, Dale, Daniel A., Dobbs, Clare L., Meyer, Jennifer Donovan, Elmegreen, Bruce G., Elmegreen, Debra M., Fumagalli, Michele, Gallagher, J. S., Grasha, Kathryn, Grebel, Eva K., Kennicutt, Robert C., Krumholz, Mark R., Lee, Janice C., Messa, Matteo, Nair, Preethi, Sabbi, Elena, Smith, Linda J., Thilker, David A., Whitmore, Bradley C., Wofford, Aida
We present a comparative study of the molecular gas in two galaxies from the LEGUS sample: barred spiral NGC 1313 and flocculent spiral NGC 7793. These two galaxies have similar masses, metallicities, and star formation rates, but NGC 1313 is forming
Externí odkaz:
http://arxiv.org/abs/2401.01450
Autor:
G. Tema, R. Lombardo, A. Sica, A. Zarraonandia Andraca, C. Plaza Alonso, J.A. Gonzalez-Dacal, H. Rodriguez Nunez, A. Mallo Barreiro, B.C. Gentile, F. Cancrini, L. Albanesi, L. Mavilla, A.L. Lopes Mendes, P. Tariciotti, F. Zammitti, G. Rizzo, P. Aloisi, M. Moldes Ruibal, R. Giulianelli
Publikováno v:
European Urology Open Science, Vol 19, Iss , Pp e384- (2020)
Externí odkaz:
https://doaj.org/article/8f6b08653aaf44f68788c4ca9c61358d
Autor:
Jones, Logan H., Hernandez, Svea, Smith, Linda J., James, Bethan L., Aloisi, Alessandra, Larsen, Søren
We present the first version release of SESAMME, a public, Python-based full spectrum fitting tool for Simultaneous Estimates of Star-cluster Age, Metallicity, Mass, and Extinction. SESAMME compares an input spectrum of a star cluster to a grid of st
Externí odkaz:
http://arxiv.org/abs/2310.09365
Autor:
Kumari, Nimisha, Smit, Renske, Leitherer, Claus, Witstok, Joris, Irwin, Mike J, Sirianni, Marco, Aloisi, Alessandra
Carbon spectral features are ubiquitous in the ultraviolet (UV) and far-infrared (FIR) spectra of galaxies in the epoch of reionization (EoR). We probe the ionized carbon content of a blue compact dwarf galaxy Pox 186 using the UV, optical, mid-infra
Externí odkaz:
http://arxiv.org/abs/2307.00059
Autor:
Mingozzi, Matilde, James, Bethan L., Berg, Danielle A., Arellano-Córdova, Karla Z., Plat, Adele, Scarlata, Claudia, Aloisi, Alessandra, Amorín, Ricardo O., Brinchmann, Jarle, Charlot, Stéphane, Chisholm, John, Feltre, Anna, Gazagnes, Simon, Hayes, Matthew, Heckman, Timothy, Hernandez, Svea, Kewley, Lisa J., Kumari, Nimisha, Leitherer, Claus, Martin, Crystal L., Maseda, Michael, Nanayakkara, Themiya, Ravindranath, Swara, Rigby, Jane R., Senchyna, Peter, Skillman, Evan D., Sugahara, Yuma, Wilkins, Stephen M., Wofford, Aida, Xu, Xinfeng
In the current JWST era, rest-frame UV spectra play a crucial role in enhancing our understanding of the interstellar medium (ISM) and stellar properties of the first galaxies in the epoch of reionization (EoR, $z>6$). Here, we compare well-known and
Externí odkaz:
http://arxiv.org/abs/2306.15062
Autor:
Magdolen, J., Dobrotka, A., Orio, M., Mikołajewska, J., Vanderburg, A., Monard, B., Aloisi, R., Bezák, P.
Publikováno v:
A&A 675, A140 (2023)
AIMS: We investigated the optical variability of the symbiotic binary FN Sgr, with photometric monitoring during $\simeq$55 years and with a high-cadence Kepler light curve lasting 81 days. METHODS: The data obtained in the V and I bands were reduced
Externí odkaz:
http://arxiv.org/abs/2306.05095