Please use this identifier to cite or link to this item: https://dspace.chmnu.edu.ua/jspui/handle/123456789/2959
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dc.contributor.authorGuziy, S. et al.-
dc.date.accessioned2025-09-25T08:54:45Z-
dc.date.available2025-09-25T08:54:45Z-
dc.date.issued2025-
dc.identifier.issn2075-4434 el.-
dc.identifier.urihttps://www.webofscience.com/wos/woscc/full-record/WOS:001514897900001-
dc.identifier.urihttps://www.mdpi.com/2075-4434/13/3/62-
dc.identifier.urihttps://dspace.chmnu.edu.ua/jspui/handle/123456789/2959-
dc.descriptionWu, S., Pérez-García, I., Castro-Tirado, A. J., Hu, Y., Gritsevich, M., Caballero-García, M. D., … Zhang, B.-B. (2025). Early Optical Follow-Up Observations of Einstein Probe X-Ray Transients During the First Year. Galaxies, 13 (3), art. no. 62. DOI: 10.3390/galaxies13030062uk_UA
dc.description.abstractWe present early follow-up observations of Einstein Probe (EP) X-ray transients, following its first year of operation. EP is a dedicated wide-field X-ray observatory that is transforming our understanding of the dynamic X-ray universe. During its first year, EP successfully detected a diverse range of high-energy transients-including gamma-ray bursts (GRBs), tidal disruption events (TDEs), and fast X-ray transients (FXTs), besides many stellar flares, disseminating 128 alerts in the aggregate. Ground-based optical follow-up observations, particularly those performed by our BOOTES telescope network, have played a crucial role in multi-wavelength campaigns carried out so far. Out of the 128 events, the BOOTES Network has been able to follow up 58 events, detecting 6 optical counterparts at early times. These complementary optical measurements have enabled rapid identification of counterparts, precise redshift determinations (such as EP250215a at z=4.61), and detailed characterization of the transient phenomena. The synergy between EP's cutting-edge X-ray monitoring and the essential optical follow-up provided by facilities, such as the above-mentioned BOOTES Global Network or other Spanish ground-based facilities we have access to, underscores the importance and necessity of coordinated observations in the era of time-domain and multi-messenger astrophysics.uk_UA
dc.language.isoenuk_UA
dc.publisherMDPIuk_UA
dc.subjectEinstein Probeuk_UA
dc.subjectX-ray transientsuk_UA
dc.subjectfollow-up observationsuk_UA
dc.subjectgamma-ray burstsuk_UA
dc.titleEarly Optical Follow-Up Observations of Einstein Probe X-Ray Transients During the First Yearuk_UA
dc.typeArticleuk_UA
Appears in Collections:Публікації науково-педагогічних працівників ЧНУ імені Петра Могили у БД Web of Science



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