2nd year Practicum
There are a total of 7 groups, with two groups (4 & 5) targeting the same galaxies.
The airmass of the targets is given in this PDF file, and their visibility (above airmass 1.56 or altitude 40 degrees), can be found in this PDF file.
A telescope generally consists of a scientific and a technical part - further sections might be present for some proposals but in the following I will only discuss the telescope proposal you shall write. We will refer to these as the scientific and technical justifications respectively. The slides provided (see below) contain some further details. The format of the telescope proposal must satisfy the following requirements:
The scientific justification
The aim of this is to tell the reader what question you want to address, what observational data you need for this and how this will be used to tackle the question.
In general the structure is a compressed version of a report. You start with an introduction which outlines what previous work has been done in this field and where your proposed science fits into this. This introduction, and indeed the justification in general, should be written at an accessible level - the person reading your proposal is unlikely to be an expert on what you are proposing. Where necessary include the most relevant references
The introduction is also the logical place to introduce your topic which you then expand on and subsequently discuss the observations needed for your work. Here you typically focus on the physical quantities needed which are then translated into practical observing requirements in the technical justification.
The technical justification
This is where you provide all the technical details for your observing. In the scientific justification you would have provided e.g. the flux limit you need to reach, or the temporal stability needed. Here you translate this into how long you need to expose on the target, what filters you need to use etc.
We will be observing using the Wide Field Camera (WFC) which is a CCD imager working in the optical range. The WFC is mounted on the 2.5m Isaac Newton Telescope (INT). This telescope in turn is part of the Isaac Newton Group of telescopes (ING), which is part of the Observatorio del Roque de los Muchachos on the island of La Palma.
You will also find it useful to refer to this document which has some more details on the technical side of observing. As pointed out in that document this web-based exposure time estimation tool is very useful.
Questions for the proposal
Some pointers to tackle these questions are provided in the document linked above.
Useful links