SVOM/VT: Instrument Overview, Science Objectives, and First-Year Performance

The 44-cm Visible Telescope (VT) aboard the Space-based Variable Objects Monitor (SVOM) is a dual-band (400-650 nm and 650-1000 nm) instrument designed to detect and characterize the optical counterparts of gamma-ray bursts (GRBs) and other high-energy transients. This paper presents the VT’s design, scientific objectives, observing strategies, and both space- and ground-based data processing pipelines, along with its first-year in-orbit performance. In-orbit commissioning tests confirm a sensitivity of 22.5 AB mag (300 s exposure), extendable to $\sim \text{\hspace{0.17em}⁣}24$ AB mag through stacking. This performance enables the VT to monitor over 100 GRBs in its first year with an exceptional $\sim \text{\hspace{0.17em}⁣}80\mathrm{\%}$ detection rate for $\mathit{\text{SVOM}}$/ECLAIRS-triggered bursts and ToO-observed bursts from other missions (e.g., $\mathit{\text{Swift,}}\mathit{\text{Fermi,}}\mathit{\text{Einstein}}\mathit{\text{Probe}}\mathit{\text{(EP)}}$), outperforming $\mathit{\text{Swift}}$/UVOT’s $\sim \text{\hspace{0.17em}⁣}40\mathrm{\%}$ detection rate. Beyond its exceptional detection efficiency, the VT played a key role in identifying high-redshift GRBs-most notably GRB 250314A (z = 7.3). Its deep upper limits at long wavelengths (up to 1 $\mu$m) were pivotal in guiding follow-up observations with large ground-based telescopes, enabling crucial near-infrared (NIR) detections. With its rapid response, deep sensitivity, and real-time processing capabilities, the VT is a key instrument for GRB research in $\mathit{\text{SVOM}}$-era, enabling critical studies of GRB optical afterglows, circumburst environments, relativistic jet dynamics, and the origins of optically dark bursts.