1st Chandra/CIAO Workshop Hands-on Session
Practical Information:
- There are 12 workstations called "DEMO1, DEMO2, ... DEMO12" and two people should work at each workstation.
- Users should log-in as "cxcguest1", "cxcguest2", etc. on the corresponding machines (passwords will be revealed on Tuesday).
- All the "cxcguest" accounts are already setup to run CIAO2.0.2.
On every window where you expect to run CIAO, you should simply
type "ciao". For example:
cxcguest-1: ciao Setting up to use release version of CIAO, from /soft/ciao I will automatically update the following files in your $HOME dir: .CXCdefaults if they are older than the files in the distribution, however backup copies will be saved with a .bak extension. CIAO configuration complete!
- Some useful checks:
cxcguest-2: ciao -v Your CIAO version is: 2.0.2 Your CXC_PROP_CLI version is: 3.0 cxcguest-3: echo $PDIRS /home/cxcguest/cxcds_param;/soft/ciao/param cxcguest-4: echo $CALDB /soft/ciao/CALDB cxcguest-5: echo $ATOMDB /soft/ciao/ATOMDB
- The workspace is in
/data/ciao_demo/
12 subdirectories have been created called cxcguest1 through cxcguest12; please use the one relative to your machine. - Chandra data useful for the analysis can be found in
/data/ciao_demo/data - All the CIAO scripts can be found in the directory
/data/ciao_demo/scripts - If you need to access CALDB files, they are in
/soft/ciao/CALDB, which is linked to /data/CALDB/ - If you need to access ATOMDB files, they are in
/soft/ciao/ATOMDB, which is linked to /data/axaf8/atomdb/
Suggested Analysis Sessions:
All the threads listed below can be found from the CIAO 2.0 threads page.
- Beginners:
Introduction To the Data Model
Introduction To Using Prism
Data Filtering
Create True Color Image
Extract an ACIS spectrum and make RMF and ARF
Getting Started With Sherpa
Introducing Sherpa: ASCII Data & Errors and Single-Component Source Models
Fitting Spectral Data: FITS Data & Responses and Multi-Component Source Models - Grating analysis:
Examining PHA2 Files
Obtain Grating Spectra
Create Grating ARFs
Extract Coadded and Grouped Nth-Order Source & Background Spectra and ARFs
Fitting Grating Data
GUIDE: Fitting and Identifying Spectral Lines
Extended Source Analysis: - Extended Source Analysis:
Create True Color Image
Obtain a Radial Profile
Exposure Map - Source Detection:
Exposure Maps
Source Detection
Estimate the Number of Counts in a Source