Notes:

[1] PIs employed or studying in, or affiliated with, a Dutch, Spanish or UK institution at the time of submission should submit their proposal/s to the Dutch (NL PC), Spanish (ES CAT) or UK (ING PATT) TAC respectively. A similar rule applies to PIs who are working at foreign institutions based in any of these three countries - they should submit their proposal/s to the TAC of the country in which they are based.

The NL PC cannot accept proposals submitted by PIs employed or studying in a country other than the Netherlands. The ING PATT and ES CAT can accept proposals submitted by PIs employed or studying in a country other than UK and Spain as long as the majority of the collaborators on the proposal are employed or studying in the UK or Spain respectively.

The NL PC, ES CAT and ING PATT can accept proposals from PIs employed or studying at the Isaac Newton Group of Telescopes at the time of submission.

[2] Observing programmes of less than one night are not accepted on the INT unless agreed in advance by the Director of ING or the Head of Astronomy.

[3] Typically ~ 4 - 5 months before the start of the semester.

[4] Specific nights are allocated each semester, flagged in the ING schedules as 'CAT S' (service) or 'CAT DDT' (DDT-IAC). CAT S observations are done by IAC support astronomers.

[5] Applications for override observations should be submitted to the TACs in the same way as proposals for scheduled time. This definition of a target of opportunity can be useful when planning your submission. Observations are made by the overridden observer.

[6] Up to 5% of ING science telescope time is available for large-scale international projects through the International Time Programme (ITP). This time is allocated on an annual basis by the International Scientific Committee (CCI). The proposal deadlines are usually in February, and the time is usually allocated over the following B and A semesters.

[7] In queue mode the observations are carried out by an ING astronomer. Programmes are selected from a queue of previously approved programmes on the basis of various criteria, such as the scientific rank of the programme, visibility of the targets, observing conditions (seeing, sky transparency, sky brightness), airmass limit, etc.

[8] On the INT it is possible that a regular proposal scheduled in visitor mode can be eventually observed in service mode. See the description of the INT service-mode observations of regular proposals.