5 天之前 · UVES is the high-resolution optical spectrograph of the VLT located at the Nasmyth B focus of UT2. It is a cross-dispersed echelle spectrograph designed to operate with high …

When combined with the fibre system FLAMES (another spectrograph installed on UT2), UVES transforms from a single tree into a clump of trees! The two instruments together can provide …

“If you need high resolution to observe faint objects, UVES is most likely the instrument you are looking for.” UVES has provided us with a forest-full of detailed spectroscopic data of an …

As part of the "Pale Red Dot" program we reanalyzed the UVES data for proxima Centauri in 2016, starting with the reduced 1-D spectra from the UVES M Dwarf team. We were able to …

UVES (UltraViolet and Visible Echelle Spectrograph) is the high-dispersion spectrograph of the VLT, observing from 300 nm to 1100 nm, with a maximum spectral resolution of 110 000. …

2017年10月1日 · High-resolution VLT/UVES spectra of multiple OH bands taken between 2000 and 2015. OH intensities and rotational temperatures show strong solar cycle effects. Good …

UVES is the cross-dispersed, echelle spectrograph built at ESO for installation at the VLT in 3Q 1999. It has two separate blue (λλ 300–500nm) and red (λλ 420–11000nm) optical paths and …

3 天之前 · A continuous observing window of 4.5 h was obtained through directors discretionary time on the 8.2 m VLT with the UVES. Each exposure lasted for 730 s with a readout time …

UVES is a dual beam echelle spectrograph installed at the Nasmyth focus of the UT2 telescope (Kueyen) of the ESO VLT since October 1999. It can reach a resolution of 80000 and 115000 …

2021年2月1日 · We present a catalog of high-velocity C ivλ 1548,1551 mini-broad absorption lines (mini-BALs) in the archives of the Very Large Telescope-UV Visual Echelle Spectrograph and …