Workshop Preparation
Return to the Main Workshop Page
If you are planning on attending an upcoming workshop, please read the
following preparation suggestions. It is especially important to note
the information on working with your
own data.
- CIAO/Chandra Data questions
-
If you have already worked with CIAO and/or Chandra data and
have questions you would like to ask, we suggest to send them
in advance to cxchelp@head-cfa.harvard.edu.
We will make sure
that an answer is ready for you at the time of the workshop.
- Suggested pre-workshop reading
-
You can find introductory (and detailed) information about the
Chandra mission in the latest version of the
Chandra Proposer's Observatory Guide (POG).
If you have CIAO already installed at your home institution we also
suggest reading and/or trying some of the introductory threads found on
the Introductory Threads
page.
- **IMPORTANT** Working on your own Chandra data:
-
Some of you have asked to analyze your own Chandra data during the
hands-on session. Given the potential proprietary nature of data,
participants who wish to analyze their own should be aware of the
following conditions:
- we will download the requested ObsID from the archive beforehand
and put them in a working area accessible to workshop participants. We
cannot have data brought on tapes or CDs on the day of the workshop,
since this would be too time consuming.
- data may have to be shared with another participant given that pairs
of people are working at the computer during the hands-on session. If
the working partner wishes to work on a different ObsID, some rotation
will be decided by the pairs.
- it is the responsibility of the participants to ftp back to their
home institutions any resulting data products they wish to keep: we
cannot offer the service of backing data products up.
If you wish to work on proprietary Chandra data:
The PI of the observation needs to send an
e-mail to cxchelp@head-cfa.harvard.edu to confirm:
- that you agree on these conditions
- the ObsID you would like to be downloaded from the archive.
If you decide to not use your own dataset, there will be of
course sample data to analyze for various instrument configurations.
|