La Silla: Important recent changes regarding Instrumentation and Facilities
Instruments and Facilities
- NIRPS: A Laser Frequency Comb for wavelength calibrations is expected to improve further the stability from Period 113 onwards.
- HARPS can be operated simultaneously with NIRPS starting from Period 111.
- HARPS: The bluer LFC, covering the range 420nm-689nm is available for Period 114
- The Visitor (Cassegrain) focus of the 3.6-m telescope is not offered due to the operation of NIRPS. The possibility of offering this visitor focus will be re-evaluated in the future.
- The Visitor focus of the NTT continues to be available.
- The installation and commissioning of SoXS - the Son of X-Shooter - will continue in Period 115.
- ULTRACAM:
- ULTRACAM is a high-speed imaging photometer designed to study faint astronomical objects at high temporal resolutions. ULTRACAM employs two dichroic beamsplitters and three frame-transfer CCD cameras to provide optical imaging with a field-of-view of 60 and at frame rates of up to 300 Hz simultaneously in the u'g'r', u'g'i' or u'g'z' bands.
- This PI instrument is offered to the ESO community for up to 5% of the observing time at the NTT in Period 109. Large Programmes will not be accepted.
- Operation of this PI instrument requires the presence of the instrument team, so ULTRACAM programmes will preferentially be scheduled contiguously on periods of several nights. For questions on the instrument and observation strategies, users shall contact the instrument PI, Prof. Vik Dhillon (vik.dhillon[AT]sheffield.ac.uk), at least two weeks prior to submitting their proposal.
- The ULTRACAM consortium is committed to support the PIs and observers from the ESO community that have been awarded telescope time with ULTRACAM. The ULTRACAM team will support the execution of the observations and the subsequent data reduction to allow the scientic exploitation of the data obtained with ULTRACAM.
- Proposers must check that their planned observations do not duplicate any protected targets specified for ULTRACAM in the Period 113 GTO target protection webpages.
- ULTRACAM is a high-speed imaging photometer designed to study faint astronomical objects at high temporal resolutions. ULTRACAM employs two dichroic beamsplitters and three frame-transfer CCD cameras to provide optical imaging with a field-of-view of 60 and at frame rates of up to 300 Hz simultaneously in the u'g'r', u'g'i' or u'g'z' bands.