Progressive improvement of impaired visual acuity during the first year after transsphenoidal surgery for non-functioning pituitary macroadenoma

Improvement of visual field defects continues even years after the initial surgical treatment. Because this process of continuing improvement has not been documented for visual acuity, we audited our data to explore the pattern of recovery of visual acuity until 1 year after transsphenoidal surgery for non-functioning pituitary macroadenoma. Retrospective follow-up study. Forty-three patients (mean age 56 +/- 14 years), treated by transsphenoidal surgery for non-functioning pituitary macroadenoma, were included in this analysis. Visual acuity improved significantly within 3 months after transsphenoidal surgery. The mean visual acuity increased from 0.65 +/- 0.37 to 0.75 +/- 0.36 (P <0.01) (right eye), and from 0.60 +/- 0.32 to 0.82 +/- 0.30 (P <0.01) (left eye). Visual acuity was improved 1 year after transsphenoidal surgery compared to the 3 months postoperative values. The mean visual acuity increased from 0.75 +/- 0.36 to 0.82 +/- 0.34 (P <0.05) (right eye), and from 0.82 +/- 0.30 to 0.88 +/- 0.27 (P <0.05) (left eye). Visual acuity improves progressively after surgical treatment for non-functioning pituitary macroadenomas, at least within the first year after transsphenoidal surger

Search for gravitational waves associated with gamma-ray bursts detected by Fermi and Swift during the LIGO–Virgo run O3b

We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC–2020 March 27 17:00 UTC). We conduct two independent searches: a generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate