ASTRONOMY 535 - PROBLEM SET #1 - DUE 01/22/03
- From looking at the specified Web sites, answer the following:
- APO web site (www.apo.nmsu.edu)
- List the detectors (number, type, and size) used in each of the
following instruments: DIS, SPICAM, GRIM
- Who will be observing during the night of January 29, 2003?
What instrument(s) will they be using?
- STScI web site (www.stsci.edu)
- What is the ACS?
- When are Cycle 12 HST proposals due? For what period of
time are people applying for? What instruments are available?
- NOAO web site (www.noao.edu)
- What is GEMINI?
- When are the next set of proposals due for NOAO telescopes? What
observing period do they cover?
- With your naked eye, the faintest star you can see on a dark site
is about mag 6. What would the faintest magnitude be that you could
see with your eye if you were looking through the eye-piece of a 5-m
telescope? Explain your various assumptions.
- A Jansky is a unit used to measure flux density, most often in the
radio; one Jansky is
. How bright is Vega
at 5500 Å in Janskys?
- In the UBVRI system, the star Vega is essentially defined to have
a magnitude of 0 in all bandpasses. What is the magnitude of Vega in
the I band (effective wavelength 8000 Å) in the STMAG system? in
the ABNU system? You can find the spectrum of vega in the computer
file: /home/catalogs/spec/vega/vegaobs.dat on the Linux machines, or
/home/charon1/holtz/vegaobs.dat on the Sun machines.
From the file,
.
In the STMAG system,
In the ABNU system,
- Using the ETC exposure time estimator available on our Linux cluster,
determine the faintest star (V band magnitude) you can observe (at S/N=10) with:
- ACS camera/ F555W filter
- ACS camera/ F606W filter
- WFPC2 camera/ F555W filter
- STIS camera/ clear filter (50ccd)
Rene Walterbos
2003-02-25