Astronomy 731 Term Projects (Spring 2005)
Projects
1. VLA Project A: choose your own target
The VLA is in the B-array. Two hours of observing time has been
allocated by the NRAO/VLA for my class on March 14, between 04:30
and 06:30 LST (you can find a copy of the latest VLA schedule
at the VLA web page listed below).
Choose a target and a scientific project. Plan, carry out, and reduce
the data, and report the results with some scientific analysis.
- NRAO/VLA astronomer web page.
Lots of useful tools are here, including the current observing schedule,
sensitivity calculator, etc. Comprehensive details about the VLA itself
(for planning observations) are in the Observational Status Summary.
- A planning session for people working on this and the VLA
archive project (see below) will be held on March 9th in the
6th floor conference room between 10-11am.
2. VLA Project B: choose your own archive project
The VLA archive includes mostly successful projects. Choose your
favorite target available in the archive, retrieve and reduce
the appropriate data, and address your own
science questions (which may or may not be intended to be addressed
by the original PI).
- NRAO/VLA astronomer web page.
Lots of useful tools are here, including the current observing schedule,
sensitivity calculator, etc. The VLA archive search page is
here,
and I would recommend using the "original VLA" archive for searching
while the Advance Query Tool is better for data retrieval.
- A planning session for people working on all VLA
project (see above) will be held on March 9th in the
6th floor conference room between 10-11am.
3. FCRAO 14m Extra-galactic Line Survey of IC 342
Choose 10-15 most interesting lines for Maffei 2 or IC 342. Make
observations, reduce data. Develop and write a program that would
produce a cross-correlation redshift for the target. Consult Rob Goeller
who will provide some assistance with this project since it is related
to his PhD thesis project.
4. FCRAO 14m Recomb Line Survey of Orion HII Region
Map Orion HII region in H41 and H42 alpha line, and some molecular
transitions. Compare with the VLA+GBT
continuum (see Shepherd et al. paper below). Produce an
electron temperature map and derive velocity field and ionized
gas structure.
- "The Orion Nebula in 3.6cm Continuum Emission", Shepherd et al. 2002, AAS poster
- "Physical Conditions in the Orion HII Region", Ferland, G. J. 2001, PASP, 113, 41
- "Dense, Ionized, and Neutral Gas Surrounding Sagittarius A*", Shukla, Yun, & Scoville 2004, ApJ, 616, 231
A planning session for people working on all FCRAO
projects (see above) will be held on March 2nd in the
6th floor conference room between 3:30-4:30pm.
Proposal and Midterm Report
Your project proposal is due on March 1st.
It should be short (one page), briefly outlining which
project you decided to do and how you envision the project
to be executed.
Your midterm report is due on April 1st.
It should be short (one page), briefly outlining what
you have accomplished thus far. This is an opportunity to
formulate what you still need to do and ask further questions.
Final Report
As I mentioned at the organizational meeting, these projects should
be done in collaboration with a partner or partners. However, you should
write your own final written report (due May 1) individually,
in your own words. To guide your report, I suggest following
topics to be included in your report:
Orion Project
- Make recomb line maps and make overlays with the optical
and VLA+GBT continuum images. Compute an electron temperature map.
- Compute free-free opacity, electron density, ionized gas mass, etc.
- What is the ionizing photon production rate? Is this consistent
with the ionizing star(s) present in this HII region?
- Make a map of ionized gas velocity field and describe the gas
kinematics. Is the gas motion supersonic or subsonic?
VLA HI Projects
- Make a 1.4 GHz continuum image and a velocity integrated line
flux image. Make overlays of these images with a Second Digitized
Sky Survey (DSS2) red plate image. Compute an HI column density map.
- What is the star formation rate you compute from the continuum
data? How does it compare with the star formation rate computed from
the FIR luminosity (using IRAS data)?
- What is the average HI column density of the galaxies
found in your field? If no HI is detected, place a limit based on
the observed limits on HI emission and HI absorption.
- For all systems detected in HI, produce a map of the velocity
field and describe the gas kinematics. Compute a dynamical mass
by making some reasonable assumptions and compare with the HI and
stellar masses.
Project Presentation
You and your
partner should also make a joint presentation of your project
on May 17th. I suggest a format of 20 minute presentation
plus a 5 minute question-and-answer session for each project team.
Here is my proposed schedule:
- 2:30-2:55pm VLA HI Study of HCG 90 (Sanch & Prachi)
- 2:55-3:20pm Search for 21cm HI Emission from NGC 4319 (Kim)
- 3:20-3:45pm FCRAO Study of Orion Nebula in H41 & H42 Recombination Lines
(Ilsang, Jonathan, Sungryong, Will)
Important dates
- March 1: proposal due
- March 2: FCRAO project planning session (3:30pm in the 6th floor conference room)
- March 7/8: FCRAO projects scheduled (0-5 LST for ExGal project, 5-10 LST for Orion project)
- March 9: VLA project planning session (10am in the 6th floor conference room)
- March 14: VLA project scheduled (04:30-06:30 LST). "Observe" file
should be send to the operator by the 13th.
- April 1: Mid-term progress report
- May 1: Final report due
- May 16/17: Project presentations
Last modified on May 12, 2005