HARPS Observing Tools
La Silla Phase2 tool (P2ls), how to delegate an observing run, NSTS
We expect our users to use the web-based La Silla P2 tool (www.eso.org/p2ls) to prepare their visitor mode observations. This is the standard ESO way of operating an instrument: Observing Blocks (OBs) are prepared from instrument-specific templates with the P2 tool before the observations. These OBs are automatically transferred to La Silla and can be loaded from the tool vOT, which is installed on the visitor's machine.
==> If a PI wishs to grant access to her/his OBs to another observer, then the PI should login into her/his ESO account via the ESO User Portal. When clicking on 'Delegate Phase 2 tasks', a new window will open. There, the run to be delegated can be selected and the email address of the ESO account associated with the observer can be specified. To delegate the run, the box 'Phase 2' must be ticked. Now the observer will be able to see, edit and execute the delegated OBs from the ESO account associated with her/him. Please note that delegating your run to another person / ESO account will not change the ID of the observing run.
Please note that the non-ESO tool NSTS for creating visitor mode observations can be used, at one's own risk. For NSTS, there is no support from ESO; this tool is maintained by the Geneva observatory. When using NSTS, please make sure that the program run ID of the OBs is correct.
Exposure Time Calculator
An Exposure Time Calculator (ETC) is available. It is modelled after the UVES ETC but uses the efficiencies relevant for HARPS (atmosphere, Cassegrain telescope, seeing, "slit loss", instrument optics (including fibre link), CCD).
Observing with HARPS: which TARGETS?
Users applying for time on HARPS should consult the following page to check for possible restricions on the allowed targets: Guaranteed Time Observations policies.
Radial velocity standards
Radial Velocity (RV) standard stars are available here. (for details see Udry et al. 1999).
Care has to be taken on the definition of "standard". What has been found to be a RV "standard" by an instrument with a low RV accuracy is not necessarily a "standard" anymore when measured by an instrument of much superior RV accuracy. We hope in few more periods to get a growing list of "HARPS RV standards".
Spectro-photometric standard stars
Extinction coefficients for La Silla
Extinction coefficients for La Silla can be found here
High resolution Thorium-Argon Atlases are available for
Almanach, airmass, other tools
Almanach, airmass plots, and other tools are available from this page