Zobrazeno 1 - 10
of 9 074
pro vyhledávání: '"Habel A"'
Autor:
De Marchi, Guido, Giardino, Giovanna, Piazzo, Katia, Panagia, Nino, Sabbi, Elena, Beck, Tracy L., Robberto, Massimo, Zeidler, Peter, Jones, Olivia C., Meixner, Margaret, Fahrion, Katja, Habel, Nolan, Nally, Conor, Hirschauer, Alec S., Soderblom, David R., Nayak, Omnarayani, Lenkic, Laura, Rogers, Ciaran, Brandl, Bernhard, Keyes, Charles D.
Publikováno v:
ApJ, 977 (2024) 214
Previous Hubble Space Telescope (HST) observations of the star-forming cluster NGC 346 in the Small Magellanic Cloud (SMC) had revealed a large population of pre-main sequence (PMS) candidates, characterised by Halpha excess emission in their photome
Externí odkaz:
http://arxiv.org/abs/2412.10361
Autor:
Tyagi, Himanshu, P., Manoj, Narang, Mayank, Megeath, S T., Rocha, Will Robson M., Brunken, Nashanty, Rubinstein, Adam E., Gutermuth, Robert A., Evans, Neal J., van Dishoeck, Ewine, Federman, Sam, Watson, Dan M., Neufeld, David A., Anglada, Guillem, Beuther, Henrik, Garatti, Alessio Caratti o, Looney, Leslie W., Nazari, Pooneh, Osorio, Mayra, Stanke, Thomas, Yang, Yao-Lun, Bourke, Tyler L., Fischer, William J., Furlan, Elise, Green, Joel D., Habel, Nolan, Klaassen, Pamela, Karnath, Nicole, Linz, Hendrik, Muzzerolle, James, Tobin, John J., Atnagulov, Prabhani, Rahatgaonkar, Rohan, Sheehan, Patrick D., Slavicinska, Katerina, Stutz, Amelia M., Tychoniec, Łukasz, Wolk, Scott J.
The composition of protoplanetary disks, and hence the initial conditions of planet formation, may be strongly influenced by the infall and thermal processing of material during the protostellar phase. Composition of dust and ice in protostellar enve
Externí odkaz:
http://arxiv.org/abs/2410.06697
Autor:
Cioppa, Anthony, Giancola, Silvio, Somers, Vladimir, Joos, Victor, Magera, Floriane, Held, Jan, Ghasemzadeh, Seyed Abolfazl, Zhou, Xin, Seweryn, Karolina, Kowalczyk, Mateusz, Mróz, Zuzanna, Łukasik, Szymon, Hałoń, Michał, Mkhallati, Hassan, Deliège, Adrien, Hinojosa, Carlos, Sanchez, Karen, Mansourian, Amir M., Miralles, Pierre, Barnich, Olivier, De Vleeschouwer, Christophe, Alahi, Alexandre, Ghanem, Bernard, Van Droogenbroeck, Marc, Gorski, Adam, Clapés, Albert, Boiarov, Andrei, Afanasiev, Anton, Xarles, Artur, Scott, Atom, Lim, ByoungKwon, Yeung, Calvin, Gonzalez, Cristian, Rüfenacht, Dominic, Pacilio, Enzo, Deuser, Fabian, Altawijri, Faisal Sami, Cachón, Francisco, Kim, HanKyul, Wang, Haobo, Choe, Hyeonmin, Kim, Hyunwoo J, Kim, Il-Min, Kang, Jae-Mo, Tursunboev, Jamshid, Yang, Jian, Hong, Jihwan, Lee, Jimin, Zhang, Jing, Lee, Junseok, Zhang, Kexin, Habel, Konrad, Jiao, Licheng, Li, Linyi, Gutiérrez-Pérez, Marc, Ortega, Marcelo, Li, Menglong, Lopatto, Milosz, Kasatkin, Nikita, Nemtsev, Nikolay, Oswald, Norbert, Udin, Oleg, Kononov, Pavel, Geng, Pei, Alotaibi, Saad Ghazai, Kim, Sehyung, Ulasen, Sergei, Escalera, Sergio, Zhang, Shanshan, Yang, Shuyuan, Moon, Sunghwan, Moeslund, Thomas B., Shandyba, Vasyl, Golovkin, Vladimir, Dai, Wei, Chung, WonTaek, Liu, Xinyu, Zhu, Yongqiang, Kim, Youngseo, Li, Yuan, Yang, Yuting, Xiao, Yuxuan, Cheng, Zehua, Li, Zhihao
The SoccerNet 2024 challenges represent the fourth annual video understanding challenges organized by the SoccerNet team. These challenges aim to advance research across multiple themes in football, including broadcast video understanding, field unde
Externí odkaz:
http://arxiv.org/abs/2409.10587
Autor:
Bortolini, Giacomo, Östlin, Göran, Habel, Nolan, Hirschauer, Alec S., Jones, Olivia C., Justtanont, Kay, Meixner, Margaret, Boyer, Martha L., Blommaert, Joris A. D. L., Crouzet, Nicolas, Lenkić, Nally, Conor, Sargent, Beth A., van der Werf, Paul, Güdel, Manuel, Henning, Thomas, Lagage, Pierre O.
The blue compact dwarf galaxy I Zw 18 is one of the most metal-poor ($Z \sim 3% Z_{\sun}$) star-forming galaxies in the local Universe. Its evolutionary status has sparked debate within the astronomical community. We aim to investigate the stellar po
Externí odkaz:
http://arxiv.org/abs/2406.17429
Autor:
Habel, Nolan, Nally, Conor, Lenkic, Laura, Meixner, Margaret, De Marchi, Guido, Kavanagh, Patrick J., Fahrion, Katja, Nayak, Omnarayani, Hirschauer, Alec S., Jones, Olivia C., Biazzo, Katia, Brandl, Bernhard R., Jaspers, Jeroen, Pontoppidan, Klaus M., Robberto, Massimo, Rogers, Ciaran, Sabbi, Elena, Sargent, B. A., Soderblom, David R., Zeidler, Peter
We present a JWST imaging survey with NIRCam and MIRI of NGC 346, the brightest star-forming region in the Small Magellanic Cloud (SMC). By combining aperture and point spread function (PSF) photometry of eleven wavelength bands across these two inst
Externí odkaz:
http://arxiv.org/abs/2404.16242
Autor:
Habel, Johannes (AUTHOR), Alavi, Sascha (AUTHOR) jhabel@bauer.uh.edu, Heinitz, Nicolas (AUTHOR)
Publikováno v:
Journal of Marketing Research (JMR). Aug2024, Vol. 61 Issue 4, p718-741. 24p.
Autor:
Alavi, Sascha1 (AUTHOR), Habel, Johannes2 (AUTHOR) jhabel@bauer.uh.edu, Vomberg, Arnd3 (AUTHOR)
Publikováno v:
Journal of Personal Selling & Sales Management. Sep2024, Vol. 44 Issue 3, p209-218. 10p.
Autor:
Hirschauer, Alec S., Crouzet, Nicolas, Habel, Nolan, Lenkić, Laura, Nally, Conor, Jones, Olivia C., Bortolini, Giacomo, Boyer, Martha L., Meixner, Kay Justtanont Margaret, Östlin, Göran, Wright, Gillian S., Azzollini, Ruyman, Blommaert, Joris A. D. L., Brandl, Bernhard, Decin, Leen, Nayak, Omnarayani, Royer, Pierre, Sargent, B. A., van der Werf, Paul
We present a JWST imaging survey of I Zw 18, the archetypal extremely metal-poor, star-forming (SF), blue compact dwarf galaxy. With an oxygen abundance of only $\sim$3% $Z_{\odot}$, it is among the lowest-metallicity systems known in the local Unive
Externí odkaz:
http://arxiv.org/abs/2403.06980
Autor:
Fransson, C., Barlow, M. J., Kavanagh, P. J., Larsson, J., Jones, O. C., Sargent, B., Meixner, M., Bouchet, P., Temim, T., Wright, G. S., Blommaert, J. A. D. L., Habel, N., Hirschauer, A. S., Hjorth, J., Lenkić, L., Tikkanen, T., Wesson, R., Coulais, A., Fox, O. D., Gastaud, R., Glasse, A., Jaspers, J., Krause, O., Lau, R. M., Nayak, O., Rest, A., Colina, L., van Dishoeck, E. F., Gudel, M., Henning, Th., Lagage, P. -O., Őstlin, G., Ray, T. P., Vandenbussche, B.
Publikováno v:
SCIENCE 22 Feb 2024 Vol 383, Issue 6685 pp. 898-903
The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There has been no direct observation of this compact object. In this work, w
Externí odkaz:
http://arxiv.org/abs/2403.04386
Autor:
Bouchet, P., Gastaud, R., Coulais, A., Barlow, M. J., Fransson, C., Kavanagh, P. J., Larsson, J., Temim, T., Jones, O. C., Hirschauer, A. S., Tikkanen, T., Blommaert, J. A. D. L., Fox, O. D., Glasse, A., Habel, N., Hjorth, J., Jaspers, J., Krause, O., Lau, R. M., Lenkić, L., Meixner, M., Nayak, O., Rest, A., Sargent, B., Wesson, R., Wright, G. S., Colina, L., Van Dishoeck, E. F., Güdel, M., Henning, Th., Lagage, P. -O., Östlin, G., Ray, T. P., Vandenbussche, B.
There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 years, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta and surrounding m
Externí odkaz:
http://arxiv.org/abs/2402.14014