NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt
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| Main Authors: | , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| author | Szabo, Norton O. Sarneczky, Krisztian Kiss, Laszlo L. Velkei, Szabolcs Bodi, Attila Bora, Zsofia Csak, Balazs Cseh, Borbala Horti-David, Agoston Joo, Andras Kalup, Csilla Kuli, Zoltan Meszaros, Laszlo Pal, Andras Seli, Balint Sodor, Adam Szakats, Robert Takacs, Nora |
| author_facet | Szabo, Norton O. Sarneczky, Krisztian Kiss, Laszlo L. Velkei, Szabolcs Bodi, Attila Bora, Zsofia Csak, Balazs Cseh, Borbala Horti-David, Agoston Joo, Andras Kalup, Csilla Kuli, Zoltan Meszaros, Laszlo Pal, Andras Seli, Balint Sodor, Adam Szakats, Robert Takacs, Nora |
| contents | 2022 EB5, 2023 CX1 and 2024 BX1: these are the three recent imminent impactor discoveries from the Piszkéstető Mountain Station of the Konkoly Observatory. They make up about one percent of all NEO discoveries from our observatory and here we provide a detailed description of our approach and methodology that led to this noticeable observational sensitivity to these meter-sized impactors. After outlining the historical background of astronomical discoveries from Hungary, we introduce our recently upgraded survey instrumentation and outline the observational strategy and its implementation. We highlight the importance of strong feedback between analysis and ongoing data collection, maximizing the value of immediate follow-up. Finally, we discuss plans for moving forward to increase the sensitivity and the temporal coverage of our survey. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_06594 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt Szabo, Norton O. Sarneczky, Krisztian Kiss, Laszlo L. Velkei, Szabolcs Bodi, Attila Bora, Zsofia Csak, Balazs Cseh, Borbala Horti-David, Agoston Joo, Andras Kalup, Csilla Kuli, Zoltan Meszaros, Laszlo Pal, Andras Seli, Balint Sodor, Adam Szakats, Robert Takacs, Nora Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics 2022 EB5, 2023 CX1 and 2024 BX1: these are the three recent imminent impactor discoveries from the Piszkéstető Mountain Station of the Konkoly Observatory. They make up about one percent of all NEO discoveries from our observatory and here we provide a detailed description of our approach and methodology that led to this noticeable observational sensitivity to these meter-sized impactors. After outlining the historical background of astronomical discoveries from Hungary, we introduce our recently upgraded survey instrumentation and outline the observational strategy and its implementation. We highlight the importance of strong feedback between analysis and ongoing data collection, maximizing the value of immediate follow-up. Finally, we discuss plans for moving forward to increase the sensitivity and the temporal coverage of our survey. |
| title | NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2512.06594 |