Laparoscopic radical hepatectomy and lymphadenectomy for incidental gallbladder cancer. Surgical technique with ICG fluorescence enhancement

Background: Radical re-resection has been demonstrated beneficial in incidental gallbladder cancer (iGBC) stages ≥ pT1b [1]. Anatomical resection (AR) of segments IVb-V is recommended, particularly for iGBC and liver-sided tumors [2]. Laparoscopically, this is a challenging procedure, as well as the regional lymphadenectomy, since inflammation from previous surgery can hinder identification of extrahepatic bile ducts. This difficult minimally invasive procedure, facilitated with indocyanine green (ICG) fluorescence enhancement [3] is herein didactically demonstrated. Methods: A 73 y. o. female patient underwent laparoscopic cholecystectomy for cholelithiasis. An iGBC -pT2b with positive cystic node-was found. Completion radical surgery was decided. Before surgery, 1.5mg of ICG was intravenously administered. A regional lymphadenectomy (stations 5-8-9-12-13) was safely performed: ICG allowed for bile duct visualization despite scarring from previous procedure. AR (IVb-V) was performed based on a glissonian-pedicle approach. After completing the procedure, a new dose of ICG was administered to discard ischemic areas in the remnant. Results: Total operative time was 359 min. Intermittent Pringle maneuver resulted in <50 ml bleeding. Hospital stay was 3 days. Pathological examination revealed no residual tumor in the liver bed. Ten lymph nodes were resected; 3 of them (2 retroportal and 1 common hepatic artery) showing tumoral invasion. After surgery, 6 cycles of adjuvant chemotherapy (Gemcitabine-Oxaliplatin) was administered. Conclusions: Laparoscopic radical surgery (AR of segments IVb-V plus regional lymphadenectomy) for iGBC is feasible and safe [4]. ICG fluorescence can be of help to identify hilar structures and rule out areas of ischemia

Laparoscopic radical hepatectomy and lymphadenectomy for incidental gallbladder cancer. Surgical technique with ICG fluorescence enhancement

Background: Radical re-resection has been demonstrated beneficial in incidental gallbladder cancer (iGBC) stages ≥ pT1b [1]. Anatomical resection (AR) of segments IVb-V is recommended, particularly for iGBC and liver-sided tumors [2]. Laparoscopically, this is a challenging procedure, as well as the regional lymphadenectomy, since inflammation from previous surgery can hinder identification of extrahepatic bile ducts. This difficult minimally invasive procedure, facilitated with indocyanine green (ICG) fluorescence enhancement [3] is herein didactically demonstrated. Methods: A 73 y. o. female patient underwent laparoscopic cholecystectomy for cholelithiasis. An iGBC -pT2b with positive cystic node-was found. Completion radical surgery was decided. Before surgery, 1.5mg of ICG was intravenously administered. A regional lymphadenectomy (stations 5-8-9-12-13) was safely performed: ICG allowed for bile duct visualization despite scarring from previous procedure. AR (IVb-V) was performed based on a glissonian-pedicle approach. After completing the procedure, a new dose of ICG was administered to discard ischemic areas in the remnant. Results: Total operative time was 359 min. Intermittent Pringle maneuver resulted in <50 ml bleeding. Hospital stay was 3 days. Pathological examination revealed no residual tumor in the liver bed. Ten lymph nodes were resected; 3 of them (2 retroportal and 1 common hepatic artery) showing tumoral invasion. After surgery, 6 cycles of adjuvant chemotherapy (Gemcitabine-Oxaliplatin) was administered. Conclusions: Laparoscopic radical surgery (AR of segments IVb-V plus regional lymphadenectomy) for iGBC is feasible and safe [4]. ICG fluorescence can be of help to identify hilar structures and rule out areas of ischemia

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta