| The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays P Kushwaha, AC Gupta, PJ Wiita, M Pal, H Gaur, EM de Gouveia Dal Pino, ... Monthly Notices of the Royal Astronomical Society 479 (2), 1672-1684, 2018 | 41 | 2018 |
| Strong Soft X-Ray Excess in 2015 XMM-Newton Observations of BL Lac OJ 287 M Pal, P Kushwaha, GC Dewangan, PK Pawar The Astrophysical Journal 890 (1), 47, 2020 | 29 | 2020 |
| Correlated X-ray/ultraviolet/optical variability and the nature of accretion disc in the bare Seyfert 1 galaxy Fairall 9 M Pal, GC Dewangan, SD Connolly, R Misra Monthly Notices of the Royal Astronomical Society 466 (2), 1777-1787, 2017 | 28 | 2017 |
| X-ray/UV variability and the origin of soft X-ray excess emission from II Zw 177 M Pal, GC Dewangan, R Misra, PK Pawar Monthly Notices of the Royal Astronomical Society 457 (1), 875-886, 2016 | 27 | 2016 |
| Correlated X-ray/UV/optical emission and short-term variability in a Seyfert 1 galaxy NGC 4593 M Pal, S Naik Monthly Notices of the Royal Astronomical Society 474 (4), 5351-5362, 2018 | 22 | 2018 |
| Variable X-ray reflection from 1H 0419–577 M Pal, GC Dewangan Monthly Notices of the Royal Astronomical Society 435 (2), 1287-1299, 2013 | 16 | 2013 |
| Spectral States of OJ 287 blazar from Multiwavelength Observations with AstroSat KP Singh, P Kushwaha, A Sinha, M Pal, A Agarwal, GC Dewangan Monthly Notices of the Royal Astronomical Society 509 (2), 2696-2706, 2022 | 14 | 2022 |
| UV to X-ray Comptonization delay in Mrk 493 O Adegoke, GC Dewangan, P Pawar, M Pal The Astrophysical Journal Letters 870 (2), L13, 2019 | 13 | 2019 |
| Blazar OJ 287 after First VHE Activity: Tracking the Reemergence of the HBL-like Component in 2020 P Kushwaha, M Pal, N Kalita, N Kumari, S Naik, AC Gupta, EMG Dal Pino, ... The Astrophysical Journal 921 (1), 18, 2021 | 12 | 2021 |
| Complex optical/UV and X-ray variability of the Seyfert 1 galaxy 1H 0419–577 M Pal, GC Dewangan, AK Kembhavi, R Misra, S Naik Monthly Notices of the Royal Astronomical Society 473 (3), 3584-3597, 2018 | 11 | 2018 |
| Complex UV/X-ray variability of 1H 0707− 495 PK Pawar, GC Dewangan, IE Papadakis, MK Patil, M Pal, AK Kembhavi Monthly Notices of the Royal Astronomical Society 472 (3), 2823-2832, 2017 | 11 | 2017 |
| Short-Term X-ray Variability during Different Activity Phases of Blazars S5 0716+ 714 and PKS 2155-304 P Kushwaha, M Pal Galaxies 8 (3), 66, 2020 | 9 | 2020 |
| The Correlated Response of the Narrow FeKα Emission Line to the Primary Continuum Changes in the Seyfert Galaxy NGC 2992 R Ghosh, M Pal Research Notes of the AAS 5 (2), 35, 2021 | 3 | 2021 |
| AstroSat View of Blazar OJ 287: A complete evolutionary cycle of HBL Component from end-phase to disappearance and Re-emergence P Kushwaha, KP Singh, A Sinha, M Pal, G Dewangan, A Agarwal arXiv preprint arXiv:2107.10783, 2021 | 2 | 2021 |
| X-ray/UV variability of narrow-line Seyfert 1 galaxies GC Dewangan, PK Pawar, M Pal Astronomical Society of India Conference Series 12, 57-60, 2015 | 2 | 2015 |
| Late-time radio brightening and emergence of a radio jet in the changing-look AGN 1ES 1927+ 654 ET Meyer, S Laha, OI Shuvo, A Roychowdhury, DA Green, L Rhodes, ... arXiv preprint arXiv:2406.18061, 2024 | 1 | 2024 |
| Complex optical/UV and X-ray variability in Seyfert 1 galaxy Mrk 509 N Kumari, M Pal, S Naik, A Jana, GK Jaisawal, P Kushwaha Publications of the Astronomical Society of Australia 38, e042, 2021 | 1 | 2021 |
| Multi-wavelength activity of the BL Lac Blazar OJ 287 After its First VHE Activity: Spectro-temporal Evolution and Remergence of the HBL like Component P Kushwaha, M Pal, N Kalita, N Kumari, S Naik, AC Gupta, EMG Dal Pino, ... arXiv e-prints, arXiv: 2010.14431, 2020 | 1 | 2020 |
| Soft X-ray excess emission in NLS1 galaxies M Pal Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe, 33, 2018 | 1 | 2018 |
| Signature of a Seyfert-like Component in Blazar 3C 273 and Its Reflection-based Explanation H Gaur, M Pal, MS Anjum, K Wani, P Kushwaha, A Pandey, L Chen The Astrophysical Journal 981 (2), 186, 2025 | | 2025 |
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