Information The WEAVE Open-Time Programme | Latest Announcement of Opportunity
Proposal information
Principal investigator
E-mail
If more than one email, separate with commas.
Affiliation
Your primary affiliation, e.g. 'University of Bristol (UK)', 'University of Amsterdam (NL)'.
Time Allocation Committee
The proposal will be sent to the following time-allocation committee for assessment:
Co-investigators
Please separate by commas, e.g. 'John Maxwell (Leicester University), Pedro Hernandez (IAC)'. Title
Related WEAVE survey(s) List related WEAVE Surveys
(if any) separated by commas. E.g. GA, SCIP, Gal Clus, StePS, WEAVE-Apertif, WEAVE-LOFAR, WEAVE-QSO, WEAVE-WD.
Scheduling requirements
Check below for any non-standard scheduling requirements .
Summary
Please state here the overarching goals of your proposal, the relevance to the broader scientific field and the immediate science objectives of the proposal. Text should contain no more than 200 words.
Scientific and technical information
Information about WEAVE/LIFU's observational capabilities (e.g. spectroscopic resolutions, wavelength ranges and expected signal-to-noise ratios) can be found on the
WEAVE instrumental overview page. For additional information, or advice about e.g. observing strategy, or about observations with unusual setup, acquisition, tracking or scheduling requirements, contact Chris Benn (crb
ing.iac.es).
The detector on each arm of the spectrograph is a mosaic of two 6k×6k
e2V CCDs. The default readout mode is slow, with no binning in the spatial direction. A
requirement for a different readout mode should be justified in the
technical case above. More detailed infomation, required to construct the WEAVE observing
blocks, will be sought in phase 2.
File upload
Upload a PDF file extending no more than four pages and including two sections to justify the scientific case and the observations requested. Figures and captions can be included. Maximum file size is 3M. In observations requested, mention specifically what feature(s) you want to measure and how. Justify what signal-to-noise is necessary and the estimated integration time to realise this. Specify the airmass, FWHM and sky brightness used for such calculation. Justify the instrument mode and the setup choice.
Upload:
Instrument setup
Focal-plane mode
Spectrograph mode
Spectral binning
Consider spectral binning for reducing the exposure time.
Targets
Targets
Provide summary information about the fields to be observed. Use
object visibility ,
sexagesimal to degree coordinate convertor ,
exposure time calculator ,
PROGTEMP builder ,
OBSTEMP builder .
For a field with multiple targets, specify maximum and minimum point-source magnitudes (Pmin and Pmax) if MOS, or maximum and minimum surface-brightness magnitudes (Smin and Smax, magnitudes/arcsec
2 ) if mIFU. For LIFU-mode observations, specify whether the provided magnitude is for a point-source target (P) or extended (S, mag/arcsec
2 ). Follow this format (leave one single blank space between columns):
Target RA(degrees) Declination(degrees) Equinox Band=Mag PROGTEMP OBSTEMP
Examples follow:
NGC3379 161.95666666666665 -12.581638888888889 J2000 V=9.3P 41331 SEFEE
Requested time
