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| Home > Astronomy > Service Programme > Description |
Description of the ING Service ProgrammeThe aim of the ING Service Programme is to provide astronomers with a means to obtain small sets of observations, which would not justify a whole night or more of telescope time. On the WHT several nights per month are set aside especially for this purpose. During these nights, ING support astronomers perform observations for several service requests. The nights allocated to service are distributed across dark, grey and bright time, and more or less equally across the semester. They are shown in the ING schedules as 'S' or 'S/D' nights in the programme reference column. Please note that 'CAT S' nights are service nights set apart from the ING service programme by the Spanish CAT time allocating committee. Proposals are generally withdrawn from the scheme after a one year period. Typically service programmes are one of this type:
The following rules apply:
There is a monthly deadline for submission of proposals: midnight on the last day of each month. The proposals are scientifically assessed by referees from the three user-community time allocation committees (UK, NL, ES) according to the nationality of the principal investigator's host institution. If the principal investigator works in an institution not based in any of the formerly mentioned nationalities, then the proposal is assessed by all the referees. The referee is independent of the ING, and nominated by the Time Assignment Committee chairs panel. Referees will endeavour to assess the applications assigned to them within a week after the deadline (0 hr on the first day of each month). However, principal investigators should be aware that due to illness, travel etc., applications may not become active for up to one month after the deadline. The possible assigned grades are, in order of priority, the following:
Grade 1 proposals will be attempted at the earliest opportunity, and take priority over all other proposals in the queue. Grade 2 proposals will be attempted as high priority, and _should_ get done over the active 1-year lifetime of the proposal, weather and instrument availability permitting. Grade 3 and 4 proposals will only be attempted when there are no higher graded proposals in the queue, and there is therefore no guarantee that they will be attempted at all. Grade 5 and 6 proposals will not be attempted. ING support astronomers will attempt the highest graded proposals on service nights. Please note that the exact date when a proposal is attempted depends on weather conditions and on instrument and target availability. Remember that in general there will be several high priority proposals in the queue waiting to be done. Applicants should also be aware that service time is allocated to each hosting institution's nationality (UK, NL or ES) on a very strict time basis, and therefore not all highly-rated proposals from a particular nationality will necessarily be completed. The service time allocation (shown here as 'Service' on the WHT) provided by every time allocating committee is taken by the Service Manager for reference and tracks the use of service observing time to reflect this nationality time share over the semesters. Applicants with proposals for genuine targets of opportunity should still use the Service Form, but should also alert the service manager by email, who will arrange for rapid scientific assessment to be carried out. Principal investigators whose proposals are attempted will be contacted by the service manager, shortly after the service night, usually via an ING Service Night Report. They will normally be asked to FTP the data back to their home site. Currently we keep the data available on disk for about 2 weeks following a service night. After this time it can be retrievable from the ING archive. The ING Board and the International Scientific Committee (CCI) have decided that data belong exclusively to those who acquired it for a period of one year. After this time it enters the public domain. Service observations are similarly treated. However, calibration data may well be used for more than one observation and may therefore be available for several groups. It may happen that identical or similar service observations are requested by two or more groups. Requests which are approved before the data are taken may be satisfied by requiring the data to be held in common by the several groups. It is up to them how they organise themselves to process it, analyse it, relate it to other work, and eventually, presumably, publish it.
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