SIMBAD references

2026A&A...705A.233B - Astronomy and Astrophysics, volume 705A233 (2026/1-1)

Exploring the connection between compact object mergers and fast X-ray transients The cases of LXT 240402A and EP250207b.

BECERRA R.L., YANG Y.-H., TROJA E., EL KABIR M., DICHIARA S., PASSALEVA N., O'CONNOR B., RICCI R., FRYER C., HU L., WU Q., YADAV M., WATSON A.M., TSVETKOVA A., ANGULO-VALDEZ C., CABALLERO-GARCIA M.D., CASTRO-TIRADO A.J., CHEUNG C.C., FREDERIKS D., GRITSEVICH M., GROVE J.E., KERR M., LEE W.H., LYSENKO A.L., PEREYRA M., RIDNAIA A., SANCHEZ-RAMIREZ R., SUN H., SVINKIN D., ULANOV M., WOOLF R. and ZHANG B.

Abstract (from CDS):

Context. The connection between compact object mergers and some extragalactic fast X-ray transients (FXRTs) has long been hypothesised but never ultimately established.
Aims. In this work, we investigate two FXRTs, the LEIA X-ray Transient LXT 240402A and the Einstein Probe EP 250207b, whose precise positions lie close to nearby (z ≲ 0.1) quiescent galaxies with a negligible probability of chance coincidence, identifying them as particularly promising cases of merger-driven explosions in the local Universe.
Methods. We used Chandra to derive accurate localisations for both events and secure otherwise ambiguous associations with their optical counterparts. Deep optical and near-infrared observations with VLT, GTC, and LBT were performed to characterise the surrounding environment and search for kilonova emission, the hallmark of neutron star mergers. Complementary early-time X-ray monitoring with Swift and Einstein Probe was used to constrain the non-thermal afterglow.
Results. We find that both FXRTs remain compatible with a compact binary merger progenitor, which produced low-mass ejecta and kilonova emission subdominant to the afterglow. However, alternative explanations such as a distant (z ≳ 1) core-collapse supernova cannot be conclusively ruled out.

Abstract Copyright: © The Authors 2026

Journal keyword(s): gamma-ray burst: general - gamma-ray burst: individual: EP250207b - gamma-ray burst: individual: LXT240402A

Simbad objects: 8

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