Zobrazeno 1 - 10
of 6 300
pro vyhledávání: '"Koprowski, A."'
Autor:
Solar, Martín, Michałowski, Michał J., Nadolny, Jakub, Galbany, Lluís, Hjorth, Jens, Zapartas, Emmanouil, Sollerman, Jesper, Hunt, Leslie, Klose, Sylvio, Koprowski, Maciej, Leśniewska, Aleksandra, Małkowski, Michał, Guelbenzu, Ana M. Nicuesa, Ryzhov, Oleh, Savaglio, Sandra, Schady, Patricia, Schulze, Steve, Postigo, Antonio de Ugarte, Vergani, Susanna D., Watson, Darach, Wróblewski, Radosław
Publikováno v:
Nat Commun 15, 7667 (2024)
Core-collapse supernovae are explosions of massive stars at the end of their evolution. They are responsible for metal production and for halting star formation, having a significant impact on galaxy evolution. The details of these processes depend o
Externí odkaz:
http://arxiv.org/abs/2409.01906
Autor:
Postigo, A. de Ugarte, Michalowski, M., Thoene, C. C., Martin, S., Ashok, A., Fernandez, J. F. Agui, Bremer, M., Misra, K., Perley, D. A., Heintz, K. E., Cherukuri, S. V., Dimitrov, W., Geron, T., Ghosh, A., Izzo, L., Kann, D. A., Koprowski, M. P., Lesniewska, A., Leung, J. K., Levan, A., Omar, A., Oszkiewicz, D., Polinska, M., Resmi, L., Schulze, S.
GRBs produced by the collapse of massive stars are usually found near the most prominent star-forming regions of star-forming galaxies. GRB 171205A happened in the outskirts of a spiral galaxy, a peculiar location in an atypical GRB host. In this pap
Externí odkaz:
http://arxiv.org/abs/2406.16726
Autor:
Gao, Zhen-Kai, Lim, Chen-Fatt, Wang, Wei-Hao, Chen, Chian-Chou, Smail, Ian, Chapman, Scott C., Zheng, Xian Zhong, Shim, Hyunjin, Kodama, Tadayuki, Ao, Yiping, Chang, Siou-Yu, Clements, David L., Dunlop, James S., Ho, Luis C., Hsu, Yun-Hsin, Hwang, Chorng-Yuan, Hwang, Ho Seong, Koprowski, M. P., Scott, Douglas, Serjeant, Stephen, Toba, Yoshiki, Urquhart, Sheona A.
We present confusion-limited SCUBA-2 450-$\mu$m observations in the COSMOS-CANDELS region as part of the JCMT Large Program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps at 450 and 850 $\mu$m cover an area of 450 arcmin$^2$. We achieved
Externí odkaz:
http://arxiv.org/abs/2405.20616
Autor:
Koprowski, M. P., Wijesekera, J. V., Dunlop, J. S., McLeod, D. J., Michałowski, M. J., Lisiecki, K., McLure, R. J.
Publikováno v:
A&A 691, A164 (2024)
We present a new determination of the star-forming main sequence (MS), obtained through stacking 100k K-band-selected galaxies in the far-infrared (FIR) Herschel and James Clerk Maxwell Telescope (JCMT) imaging. By fitting the dust emission curve to
Externí odkaz:
http://arxiv.org/abs/2403.06575
Autor:
Michałowski, Michał J., Gall, C., Hjorth, J., Frayer, D. T., Tsai, A. -L., Rowlands, K., Takeuchi, T. T., Leśniewska, A., Behrendt, D., Bourne, N., Hughes, D. H., Koprowski, M. P., Nadolny, J., Ryzhov, O., Solar, M., Spring, E., Zavala, J., Bartczak, P.
Publikováno v:
2024, ApJ, 964, 129
Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that the dust removal timescale in early-type galaxies (ETGs) is about 2.5
Externí odkaz:
http://arxiv.org/abs/2401.04774
Autor:
Pearson, James, Serjeant, Stephen, Wang, Wei-Hao, Gao, Zhen-Kai, Babul, Arif, Chapman, Scott, Chen, Chian-Chou, Clements, David L., Conselice, Christopher J., Dunlop, James, Fan, Lulu, Ho, Luis C., Hwang, Ho Seong, Koprowski, Maciej, Michałowski, Michał, Shim, Hyunjin
Bright galaxies at sub-millimetre wavelengths from Herschel are now well known to be predominantly strongly gravitationally lensed. The same models that successfully predicted this strongly lensed population also predict about one percent of faint $4
Externí odkaz:
http://arxiv.org/abs/2309.00888
Publikováno v:
From Local to Global: Eco-entrepreneurship and Global Engagement with the Environment
Autor:
Itrich, Dominika, Karska, Agata, Sewiło, Marta, Kristensen, Lars E., Herczeg, Gregory J., Ramsay, Suzanne, Fischer, William J., Tabone, Benoît, Rocha, Will R. M., Koprowski, Maciej, Lê, Ngân, Deka-Szymankiewicz, Beata
The effects of metallicity on the evolution of protoplanetary disks may be studied in the outer Galaxy where the metallicity is lower than in the solar neighbourhood. We present the VLT/KMOS integral field spectroscopy in the near-infrared of $\sim$1
Externí odkaz:
http://arxiv.org/abs/2306.05502
Autor:
Koprowski, Przemysław
Polynomial factorization and root finding are among the most standard themes of computational mathematics. Yet still, little has been done for polynomials over quaternion algebras, with the single exception of Hamiltonian quaternions for which there
Externí odkaz:
http://arxiv.org/abs/2305.02072
Autor:
Le, N., Karska, A., Figueira, M., Sewiło, M., Mirocha, A., Fischer, Ch., Kaźmierczak-Barthel, M., Klein, R., Gawroński, M., Koprowski, M., Kowalczyk, K., Fischer, W. J., Menten, K. M., Wyrowski, F., König, C., Kristensen, L. E.
Publikováno v:
A&A 674, A64 (2023)
(abridged) Far-infrared (FIR) line emission provides key information about the gas cooling and heating due to shocks and UV radiation associated with the early stages of star formation. Gas cooling via FIR lines might, however, depend on metallicity.
Externí odkaz:
http://arxiv.org/abs/2304.08127