Accès ouvert
2026
article
OpenAlex
Runduo Liang, Wenxiong Li, Liang-Duan Liu, K. Smith et autres
Abstract Extragalactic fast X-ray transients (eFXTs) represent a rapidly growing class of high-energy phenomena, whose physical origins remain poorly understood. With its wide-field, sensitive all-sky monitoring, the Einstein Probe (EP) has greatly increased the discovery rate of eFXTs. The search for and …
cn, gb, de, cl, us, tw, nl, th
(code pays fourni par la source)
Accès ouvert
2026
preprint
OpenAlex
Jialian Liu, Bao Wang, Xiaofeng Wang, David Aguado et autres
Fast blue optical transients (FBOTs) represent one of the most exotic astrophysical transients, exhibiting unusually strong emission across X-ray, optical, and radio wavelengths. Their physical origins remain highly debated, with proposed explanations ranging from stellar explosion to tidal disruption event (TDE). Here …
Accès ouvert
2026
preprint
OpenAlex
Jialian Liu, Bao Wang, Xiaofeng Wang, David Aguado et autres
Fast blue optical transients (FBOTs) represent one of the most exotic astrophysical transients, exhibiting unusually strong emission across X-ray, optical, and radio wavelengths. Their physical origins remain highly debated, with proposed explanations ranging from stellar explosion to tidal disruption event (TDE). Here …
Accès ouvert
2026
preprint
OpenAlex
Xiaofeng Wang, Qichun Liu, Jie Lin, Y. Wang et autres
cn, au, us, th, gb, ro, ca
(code pays fourni par la source)
Accès ouvert
2026
preprint
OpenAlex
Runduo Liang, Wen-Xiong Li, Liang-Duan Liu, Ken Smith et autres
Extragalactic fast X-ray transients (eFXTs) represent a rapidly growing class of high-energy phenomena, whose physical origins remain poorly understood. With its wide-field, sensitive all-sky monitoring, the Einstein Probe (EP) has greatly increased the discovery rate of eFXTs. The search and identification of …
Accès ouvert
2026
article
OpenAlex
Qiang Xi, Ning-Chen Sun, David Aguado, Ismael Pérez-Fournon et autres
Abstract SN 2024aecx is a nearby (∼11 Mpc) Type IIb SN discovered within ∼1 day after explosion. In this paper we report high-cadence photometric (typically 0.5 ∼ 1 day) and spectroscopic follow-up observations, conducted from as early as 0.27 day post discovery …
Accès ouvert
2026
preprint
OpenAlex
Xiaohan Chen, Ning-Chen Sun, Qiang Xi, Chun Chen et autres
Type IIP supernovae (SNe IIP) exhibit a significant diversity in their explosion properties, yet the physical mechanisms driving this diversity remain unknown. In this work, we present photometric and spectroscopic observations of SN 2024abfl, a SN IIP in NGC 2146 with a …
cn, th, es, gb, cl
(code pays fourni par la source)
Accès ouvert
2026
preprint
OpenAlex
Samaporn Tinyanont, Kittipong Wangnok, Jennifer E. Andrews, Ryan J. Foley et autres
We present near-infrared (NIR) spectroscopy of the hydrogen- and helium-poor (Type Ic) supernova (SN) 2024aecx, which displays a strong NIR excess emerging 32 days post peak. SN 2024aecx is a peculiar SN Ic that exhibited luminous shock-cooling emission at early times, suggestive …
Accès ouvert
2026
preprint
OpenAlex
Sahana Kumar, Raphael Baer-Way, Aravind P. Ravi, Maryam Modjaz et autres
Calcium-strong transients (CaSTs) are a subclass of faint and rapidly evolving supernovae (SNe) that exhibit strong calcium features and notably weak oxygen features. The small but growing population of CaSTs exhibits some aspects similar to thermonuclear supernovae but others similar to massive …
Accès ouvert
2026
article
OpenAlex
Chun Chen, Ning-chen Sun, Qiang Xi, Samaporn Tinyanont et autres
Abstract SN 2025coe is a calcium-strong transient located at an extremely large projected offset ∼39.3 kpc from the center of its host, the nearby early-type galaxy NGC 3277 at a distance of ∼25.5 Mpc. In this paper, we present multiband photometric and …
Accès ouvert
2026
article
OpenAlex
Natalie LeBaron, Raffaella Margutti, Ryan Chornock, Nayana A. J. et autres
Abstract We present an extensive photometric and spectroscopic ultraviolet–optical–infrared campaign on the luminous fast blue optical transient (LFBOT) AT 2024wpp over the first ∼100 days. AT 2024wpp is the most luminous LFBOT discovered to date, with L pk ≈ (2–4) × 10 …
Accès ouvert
2025
article
OpenAlex
Zikun Lin, Yanan Wang, Shuyuan Wei, Yongkang Sun et autres
Abstract The black hole low-mass X-ray binary (LMXB) candidate IGR J17091–3624 experienced a hard-state-only outburst in 2025. In this paper, we show that IXPE detected a series of intermittent X-ray dips, spanning a total interval of ∼1 day. Subsequent observations with NICER, …