HST and FUSE DADS retrievals will be down from Tuesday, September 2 through Wednesday Sept 3 for a DADS/OPUS installation. See list of alternative data sources.
During part of this time, the database will also be down and so searches will be down during that time (HLA and GALEX are unaffected by this downtime).
Retrieval of FUSE Data from MAST
This page explains the Retrieval Options and gives information on contents
of FUSE data.
Once observations of interest are found,
registered and anonymous users can
retrieve the data. We describe here the
various retrieval options for FUSE data and explain the various terms
involved, which you will encounter on the retrieval page.
Note that the browsing capabilities on this page may differ depending on
whether FUSE data were last processed after early-September 2002, corresponding
to the implementation of CALFUSE 2.2 pipeline processing software.
Subsequent to this date, browse images are availabe for the two dimensional
spectral images and for count rate (vs. time) plots for individual
exposures of an observation. Reprocessing of older data is currently
underway, and ultimately these plots will be made available for them
as well; for a discussion of this point see the
"Changes in data products..." section below.
Your archive username. This is the username you were given when you
registered for an archive account.
If you don't have an archive account, you can register for one on the web at
http://archive.stsci.edu/registration/ or use the anonymous method for public data.
If you register, you should receive your archive username and password via email in a few minutes.
Your archive password. This is the password that was given to you
when you registered for your archive account (See Archive Username,
above) or your email address if you are using the anonymous method for nonproprietary data.
The data will be written to the Archive staging disk. You will be able
to pull from the staging disk using FTP and logging in with your archive username and password. If you used the
anonymous method, you can use either your username and password or anonymous ftp.
Only non-proprietary data
may be retrieved. You can delete your data when you are done.
This is where you would like the data sent. These fields are required
if you select the FTP or SFTP retrieval option. The data will be delivered
to this destination via the delivery option selected.
The name of the directory to which the data will be written.
Please make sure that this directory exists, is writeable,
and has enough space. The retrieval will fail otherwise.
(Unfortunately, for technical reasons, we can't reliably estimate the size of your retrieval until
the files are read from the optical platters, so we can't tell you whether there is enough space there,
but generally, retrievals are rarely more than a gigabyte in total size.)
There are five characters which, if present in a password, will cause the retrieval
to fail: (, ), *, ", and /.
Retrieval Security
All the information you enter in this form will be sent to ST ScI through
an SSL (encrypted) web connection using a Verisign
certificate. The password remains encrypted until it is needed to transfer the data
to you. The password is not retained after the data are transferred.
If your local system disallows FTP or sftp access and you are requesting only public data,
you can use the STAGE option.
The default set of files delivered to the requestor is the first option
under "Files Requested" on the Retrieval Options page. This option returns
just 12 calibrated files (rootname "*fcal") per exposure - 8 for each
detector/side, and 4 trailer
files (trailer files are the logs of the pipeline processing history of
the observation), irrespective of the TTAG or HIST observing mode.
The files in this package are only those unique to a given observation.
Quick-look gif files are not included in this package.
It is important to note that for most (TTAG) observations files are returned
for all three spectral entrance apertures, even though only one is normally
used. For HIST observations only the target aperture admits light and
therefore only one set of aperture files is generated (see the FUSE
Instrument and Data Handbook,
Section 3.2: Spectral Image (HIST) Mode)
Parsing FUSE file names can be daunting to the uninitiated.
For information on the FUSE file naming conventions and contents
see the table in Data Handbook,
Section 4.1: Data Filenames.
Hint: the project defines "rootname" with 11 characthers through the
exposure number (3 characters). As defined, this name not includes
the detector number & side (1a, 1b, 2a, 2b), observing mode, and data
product type.
NOTE:
All FUSE data are now processed with CalFUSE v3.1 or beyond.
Currently, v3.2 data is gradually supplanting
v3.1 data. Summaries of CalFUSE for v3.0, v3.1, and v3.2 relative to the
previous versions as given by the Project are contained in the link to these
versions. We also list information on v2.2 for users who may wish to know
what upgrades are contained in older data that they possess on their computers.
However, these data are no longer available through MAST.
Observations with an Archive Date later than March 2007 were processed
CalFUSE v3.2.
Observations with an Archive Date between October, 2005 and
March, 2007 were processed
CalFUSE v3.1.
Observations with an Archive Date between August 19, 2004 and September
2005 processed with
CalFUSE v3.0
a>.
These data have an Archive Date between September 5, 2002 and August
18, 2004.
CalFuse v2.2.1 included new "jitter" and "housekeeping" files associated with
guiding techniques that utilize the satellite's magnetic torsion bars.
The jitter file (file
root name ends in "jitrf") is used to correct exposure times for small deviation
s
from nominal positioning of the target in the aperture. The housekeeping file
(root name ends in "hskpf") provides satellite-attitude
vector information used to compute the jitter file.
Most users will probably not need the jitter files, but see the
white paper on jitter correction in FUSE pipeline processing as
well as in the Data Handbook
(
Frequently Asked Questions about Retrievals
I'm the PI on proposal nnnn, why can't I retrieve the data?
You can, but you'll need to let us know you want it.
Currently, PIs do not receive automatic electronic access to their data.
(This is a technical limitation, not a policy.)
If you are the PI and want electronic access to your proposal,
contact archive@stsci.edu
and let us know the proposal ID and your archive username.
We will attach the proper access priveleges to your account to allow you
to retrieve this data electronically.
You can also authorize co-investigators and co-workers to have electronic access as well.
Just tell us the proposal ID and the names and archive usernames
of those to whom you wish to grant access.
(If they don't have accounts, or you're not sure if they do,
then let us know their email addresses to we can help them set up accounts for access.)
Authorization may be set up only on a per-proposal basis;
we cannot restrict access to certain data within the proposal.
OK, I'm now an authorized user on this proposal,
and it still says the data is proprietary...
Then one of the following has happened:
You are trying to retrieve the data to the Archive Host staging disk.
The staging disk is an anonymous FTP area, so we can allow only
non-proprietary data to be written to it.
Have the data sent directly to your disk or sent to you on tape instead.
We made a mistake and didn't properly authorize your account.
This may be particularly true if you (for some reason) have
more than one archive account.
The data are under restriction, which means that they were found
to duplicate planned or existing proprietary observations, and an
access restriction has been placed on them until the data with which
it conflicts is released.
If a retrieval fails due to lack of disk space
(or for any other reason), do I have to resubmit it
or will it be resubmitted for me?
Requests are deleted out of our system after they are completed,
so you will need to resubmit your request.
I don't need the whole dataset. How do I retrieve just one file extension?
Select the extensions
from the scrollbox or enter them into the space provided on the Retrieval Options page (or the File Options screen in StarView.)