2022MNRAS.517L..21C

The properties of the disc/jet coupling in quiescent black hole low mass X-ray binaries (BH LMXBs) are still largely unknown. In this paper, we present the first quasi-simultaneous radio and X-ray detection in quiescence of the BH LMXB MAXI J1348-630, which is known to display a hybrid disc/jet connection that depends on the accretion rate. We performed deep X-ray and radio observations using the Chandra X-ray Observatory and the Australia Telescope Compact Array. MAXI J1348-630 is detected for the first time in quiescence at an X-ray luminosity L_X = (7.5 ± 2.9) × 10³⁰(D/2.2 kpc)² erg s^–1: one of the lowest X-ray luminosities observed for a quiescent BH LMXB, possibly implying a short orbital period for the system. MAXI J1348-630 is also detected in radio at L_R = (4.3 ± 0.9) × 10²⁶(D/2.2 kpc)² erg s^–1. These detections allow us to constrain the location of MAXI J1348-630 on the radio/X-ray diagram in quiescence, finding that the source belongs to the standard (radio-loud) track in this phase. This provides a strong confirmation that hybrid-correlation sources follow the standard track at low luminosities and down to quiescence, thus improving our knowledge of the disc/jet connection in BH LMXBs.