| The quasar main sequence explained by the combination of eddington ratio, metallicity, and orientation S Panda, P Marziani, B Czerny The Astrophysical Journal 882 (2), 79, 2019 | 98 | 2019 |
| Modeling of the quasar main sequence in the optical plane S Panda, B Czerny, TP Adhikari, K Hryniewicz, C Wildy, J Kuraszkiewicz, ... The Astrophysical Journal 866 (2), 115, 2018 | 89 | 2018 |
| Failed radiatively accelerated dusty outflow model of the broad line region in active galactic nuclei. I. Analytical solution B Czerny, YR Li, K Hryniewicz, S Panda, C Wildy, M Sniegowska, ... The Astrophysical Journal 846 (2), 154, 2017 | 85 | 2017 |
| Can reverberation-measured quasars be used for cosmology? ML Martínez-Aldama, B Czerny, D Kawka, V Karas, S Panda, M Zajaček, ... The Astrophysical Journal 883 (2), 170, 2019 | 71 | 2019 |
| Time delay measurement of Mg II line in CTS C30. 10 with SALT B Czerny, A Olejak, M Rałowski, S Kozłowski, MLM Aldama, M Zajacek, ... The Astrophysical Journal 880 (1), 46, 2019 | 54 | 2019 |
| CLOUDY view of the warm corona S Panda, B Czerny, C Done, A Kubota The Astrophysical Journal 875 (2), 133, 2019 | 45 | 2019 |
| Time Delay of Mg ii Emission Response for the Luminous Quasar HE 0435-4312: toward Application of the High-accretor Radius–Luminosity Relation in Cosmology M Zajaček, B Czerny, ML Martinez–Aldama, M Rałowski, A Olejak, ... The Astrophysical Journal 912 (1), 10, 2021 | 43 | 2021 |
| High metal content of highly accreting quasars M Śniegowska, P Marziani, B Czerny, S Panda, ML Martínez-Aldama, ... The Astrophysical Journal 910 (2), 115, 2021 | 43 | 2021 |
| Time-delay Measurement of Mg ii Broad-line Response for the Highly Accreting Quasar HE 0413-4031: Implications for the Mg ii–based Radius–Luminosity Relation M Zajaček, B Czerny, ML Martinez–Aldama, M Rałowski, A Olejak, ... The Astrophysical Journal 896 (2), 146, 2020 | 41 | 2020 |
| Current and future applications of Reverberation-mapped quasars in Cosmology S Panda, ML Martínez-Aldama, M Zajaček Frontiers in Astronomy and Space Sciences 6, 75, 2019 | 41 | 2019 |
| The CaFe project: Optical Fe II and near-infrared Ca II triplet emission in active galaxies: simulated EWs and the co-dependence of cloud size and metal content S Panda Astronomy & Astrophysics 650, A154, 2021 | 34 | 2021 |
| Interpretation of Departure from the Broad-line Region Scaling in Active Galactic Nuclei B Czerny, JM Wang, P Du, K Hryniewicz, V Karas, YR Li, S Panda, ... The Astrophysical Journal 870 (2), 84, 2019 | 32 | 2019 |
| Scatter Analysis along the Multidimensional Radius–Luminosity Relations for Reverberation-mapped Mg ii Sources ML Martínez–Aldama, M Zajaček, B Czerny, S Panda The Astrophysical Journal 903 (2), 86, 2020 | 31 | 2020 |
| The CaFe project: Optical Fe ii and near-infrared Ca ii triplet emission in active galaxies. I. Photoionization modeling S Panda, ML Martínez-Aldama, M Marinello, B Czerny, P Marziani, ... The Astrophysical Journal 902 (1), 76, 2020 | 30 | 2020 |
| Dark energy constraints from quasar observations B Czerny, ML Martínez-Aldama, G Wojtkowska, M Zajaček, P Marziani, ... arXiv preprint arXiv:2011.12375, 2020 | 27 | 2020 |
| Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius–luminosity relation luminosity distances N Khadka, M Zajaček, R Prince, S Panda, B Czerny, ML Martínez-Aldama, ... Monthly Notices of the Royal Astronomical Society 522 (1), 1247-1264, 2023 | 23 | 2023 |
| Standardizing reverberation-measured C iv time-lag quasars, and using them with standardized Mg ii quasars to constrain cosmological parameters S Cao, M Zajaček, S Panda, ML Martínez-Aldama, B Czerny, B Ratra Monthly Notices of the Royal Astronomical Society 516 (2), 1721-1740, 2022 | 23 | 2022 |
| Consistency study of high- and low-accreting Mg ii quasars: no significant effect of the Fe ii to Mg ii flux ratio on the radius–luminosity relation dispersion N Khadka, M Zajaček, S Panda, ML Martínez-Aldama, B Ratra Monthly Notices of the Royal Astronomical Society 515 (3), 3729-3748, 2022 | 22 | 2022 |
| The physical driver of the optical Eigenvector 1 in Quasar Main Sequence S Panda, B Czerny, C Wildy Frontiers in Astronomy and Space Sciences 4, 33, 2017 | 20 | 2017 |
| A novel black hole mass scaling relation based on coronal gas, and its dependence with the accretion disc A Prieto, A Rodríguez-Ardila, S Panda, M Marinello Monthly Notices of the Royal Astronomical Society 510 (1), 1010-1030, 2022 | 19 | 2022 |
Bozena CzernyCenter for Theoretical Physics在 cft.edu.pl 的电子邮件经过验证
