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IRTF: Getting Observing Time


Posted by bkloppenborg on February 23, 2010 - 1:33am

Before I entered graduate school, I had no idea about the complexity of research proposals, especially those in astronomy/astrophysics.

All telescope time for which I have applied has been peer reviewed.  This means that my proposal is read by fellow astronomers/astrophysicists and evaluated against some scoring method.  It is my responsibility, as the proposer, to convince the committee that not only is my research interesting, but also doable from a technical perspective. 

The basic outline of the proposal process is thus:

  1. Determine a facility that can do the type of science you need.  This often means locating a facility that first covers the wavelengths in which you are interested.  As I mentioned in yesterday's post, we hope to observe the appearance of CO lines in the infrared so we obviously need an infrared telescope.  Although it goes without saying, the facility needs to be in the correct hemisphere to observe your target.  Being quite new to research (presently I'm in the third year of my Ph.D.), I often go ask my adviser, Dr. Bob, or another professor in our department about instruments they have used in the past that might cover the wavelength region of intrest.
  2. See if the research facility has an instrument that can take the data you need.  The next step is to look at the facility's instrument list.  IRTF has a nice list of infrared instruments that can be used for spectroscopy and photometry.  We wanted to observe the CO spectral lines in the ~2.5 micron region so SpeX, and CSHELL are good options (there are separate observations looking in the mid-infrared with MIRSI and BASS).
  3. Next, we need to verify that the instrument can observe our target.  This involves looking at sensitivities, exposure times, and estimating signal-to-noise ratios based upon previously observed targets with similar properties (or a model of the machine's performance characteristics).  With eps Aur, we have no problems getting enough light and in the case of some instruments, eps is too bright to be observed  without very special pixel placement.
  4. After we have the basics down, we need to start looking at the proposal schedule.  Some observatories offer yearly, bi-yearly, or quarterly proposal opportunities.  We need to choose a proposal time that permits our target to be observed (in our case, any time in the winter is good).
  5. Now comes the hard part: paperwork.  There's a series of forms and check lists that must be filled out detailing our observations.  It is in this step that we start filling out a description and scientific justification for our observations for peer review.  Some telescope time comes with funds so you might have to fill out a budget and then run it by your institution's business department.  These budgets can be tricky as your hosting institution can get a considerable cut of your incoming funds.
  6. Then comes the easy part: submit and wait.  Most research facilities are good about getting proposals processed in a timely fashion, taking a month or two to get back to you.  Some of them can take six or more months.  During this time the reviewers are processing hundreds, possibly thousands of applications in order to pick the ones that offer the most interesting science.
  7. And the best/worse part.  Acceptance or Rejection of your proposal.  If your proposal was accepted, great!  If not... well, try again I suppose.  At the big research facilities, telescope time is very competitive and for the space-based telescopes, it is extremely competitive, especially if the observing time comes with funds.  I can't give you any details statistics, but getting a rejection letter is common.  Fortunately, the reviewers provide feedback which describes why your proposal wasn't accepted which can often help when you re-propose.

Be sure to stop by tomorrow in which I'll discuss how we prepared for our IRTF observing run.

amateurs

This is one area where amateurs have it easy. Our proposal method is usually asking "Honey, can I?" and our application to our spouse/significant other may consist of roses, taking out the trash, doing the dishes, etc.

I wonder what happens if an

Iwonder what happens if an event triggers a need for follow-up observations on short notice, e.g. super-novae or an impact on Jupiter. Is there an all-mighty astronomer-on-duty that can overrule observation schedules? CS HBE

follow-up

There are two main methods of getting timely observations (remember, for professional observatories, the proposals are generally submitted every 6 months to a year, so if something takes place between cycles, you need some mechanism to cover it): Director's Discretionary Time (DDT), and a friendly colleague. Usually every facility has a block of time that is allocated to the "director". This is available for transient events (our first V838 Mon observations were acquired through DDT on HST, for example). The review process is pretty simple - submit something short and sweet to the proper person, hear back shortly. You rarely get funding for a DDT proposal. Even for DDT, you may have to wait weeks before the observation is scheduled - "real time" means different things to different facilities! The friendly colleague approach has two paths: sometimes someone is observing on a telescope, and will interrupt their project to take data for you. This is pretty rare, as they have spent a lot of time and effort proposing for their time, and often get less than they requested, so they want to use every minute possible. On the other hand, sometimes conditions are not suitable for their main project and they are doing secondary science anyway. The other path is engineering time - a few percent of time on every major telescope is devoted to bringing up new instruments or calibrating existing ones. If your request happens to fall during one of these intervals, you can often ask the Instrument Scientist to slip in an observation of your object. You may get some pretty crappy data that way, but at least you get something. Those are the main ways to get "target of opportunity" observations. I often also data-mine, as many surveys are underway and on occasion they are taking data of a field of interest. Since your project may be completely unrelated to the survey's main goals, they will let you use the images/data for your own research with minimal crediting. Arne

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