Zobrazeno 1 - 10
of 1 039
pro vyhledávání: '"Czerny B"'
Autor:
Jaiswal, V. K., Prince, R., Pandey, A., Naddaf, M. H., Czerny, B., Panda, S., Mandal, Amit Kumar, Nunez, F. Pozo
The dynamical and geometric structures of the Broad Line Region (BLR), along with the origins of continuum time delays in active galaxies, remain topics of ongoing debate. In this study, we aim to reproduce the broadband spectrum, the H$\beta$ line d
Externí odkaz:
http://arxiv.org/abs/2410.03597
Autor:
Floris, A., Marziani, P., Panda, S., Sniegowska, M., D'Onofrio, M., Deconto-Machado, A., Del Olmo, A., Czerny, B.
Publikováno v:
A&A 689, A321 (2024)
The 4D eigenvector 1 (E1) sequence has emerged as a powerful tool for organizing the observational and physical characteristics of type-1 active galactic nuclei (AGNs). In this study, we present a comprehensive analysis of the metallicity of the broa
Externí odkaz:
http://arxiv.org/abs/2405.04456
Autor:
Ballantyne, D. R., Sudhakar, V., Fairfax, D., Bianchi, S., Czerny, B., De Rosa, A., De Marco, B., Middei, R., Palit, B., Petrucci, P. -O., Rozanska, A., Ursini, F.
The soft excess in active galactic nuclei (AGNs) may arise through a combination of relativistic reflection and the effects of a warm corona at the surface of the accretion disc. Detailed examination of the soft excess can therefore constrain models
Externí odkaz:
http://arxiv.org/abs/2404.03040
Publikováno v:
2024 Res. Notes AAS 8 47
The Legacy Survey of Space and Time (LSST) at the Vera C. Rubin Observatory is poised to observe thousands of quasars using the Deep Drilling Fields (DDF) across six broadband filters over a decade. Understanding quasar accretion disc (AD) time delay
Externí odkaz:
http://arxiv.org/abs/2402.10969
Autor:
Saha, T., Markowitz, A., Homan, D., Krumpe, M., Haemmerich, S., Czerny, B., Graham, M., Frederick, S., Gromadzki, M., Gezari, S., Winkler, H., Buckley, D. A. H., Brink, J., Naddaf, M. H., Rau, A., Wilms, J., Gokus, A., Liu, Z., Grotova, I.
Context. Multiwavelength studies of transients in actively accreting supermassive black holes have revealed that large-amplitude variability is frequently linked to significant changes in the optical spectra -- a phenomenon referred to as changing-lo
Externí odkaz:
http://arxiv.org/abs/2309.08956
Autor:
Zajaček, M., Czerny, B., Jaiswal, V. K., Štolc, M., Karas, V., Pandey, A., Pasham, D. R., Śniegowska, M., Witzany, V., Suková, P., Münz, F., Werner, N., Řípa, J., Merc, J., Labaj, M., Kurfürst, P., Krtička, J.
In this review (the third in the series focused on a small two-band UV-photometry mission), we assess possibilities for a small UV two-band photometry mission in studying accreting supermassive black holes (SMBHs; mass range $\sim 10^6$-$10^{10}\,M_{
Externí odkaz:
http://arxiv.org/abs/2306.15082
Publikováno v:
Proc. IAU 19 (2023) 95-99
We investigated a scenario where the presence of a broad absorption line (BAL) feature in quasars (QSOs) is contingent upon the line of sight being situated within an outflow cone emanating from the source. We examined the mechanism of dust-driven wi
Externí odkaz:
http://arxiv.org/abs/2306.03224
Autor:
Nuñez, F. Pozo, Bruckmann, C., Desamutara, S., Czerny, B., Panda, S., Lobban, A. P., Pietrzyński, G., Polsterer, K. L.
Photometric reverberation mapping can detect the radial extent of the accretion disc (AD) in Active Galactic Nuclei by measuring the time delays between light curves observed in different continuum bands. Quantifying the constraints on the efficiency
Externí odkaz:
http://arxiv.org/abs/2212.09161
Autor:
Marziani, P., Bon, E., Bon, N., D'Onofrio, M., Punsly, B., Sniegowska, M., Czerny, B., Panda, S., Aldama, M. L. Martinez, del Olmo, A., Deconto-Machado, A., Negrete, C. A., Dultzin, D., Buendia, T., Garnica, K.
The last few years have seen the confirmation of several trends associated with the quasar main sequence. The idea of a main sequence for quasars is relatively recent, and its full potential for the observational classification and contextualization
Externí odkaz:
http://arxiv.org/abs/2111.04140
Autor:
Czerny, B., Martínez-Aldama, M. L., Wojtkowska, G., Zajaček, M., Marziani, P., Dultzin, D., Naddaf, M. H., Panda, S., Prince, R., Przyluski, R., Ralowski, M., Śniegowska, M.
Recent measurements of the parameters of the Concordance Cosmology Model ($\Lambda$CDM) done in the low-redshift Universe with Supernovae Ia/Cepheids, and in the distant Universe done with Cosmic Microwave Background (CMB) imply different values for
Externí odkaz:
http://arxiv.org/abs/2011.12375