IMAPS-2
Currently, only the IMAPS-1 data is releaseable. IMAPS-2 is expected to become available some time in the near future.
IMAPS-1
The original IMAPS data was stored as IDL unformatted data
sets. The raw data
was later converted to FITS format files by the staff members at the
ADF.
The FITS headers were extensively modified by Goddard LASP personnel,
and the resulting raw image files are now available
via the WEB or anonymous FTP at archive.stsci.edu
in the /pub/orfeus/imaps/data/raw directory.
An effort is currently underway by LASP personnel to archive the
coadded, corrected raw data.
These data are corrected for image distortion, face plate artifacts,
etc. but the spectra must still be extracted (although wavelength
assignments will be included). IDL software will be
made available to read and extract data using these files.
IMAPS data sets are uniquely defined using the "Exposure Sequence Number". The first archived file is number 079 and the last image is number 721. The current naming convention is imaps1_0nnn.fits, where nnn is the exposure sequence number. The coadded files will use the naming convention imaps1_0nnn-0mmm.fits where nnn is the first coadded image and mmm is the last coadded image. (It is assumed that all intervening images are included in the coaddition.)
A table of the IMAPS1 observations (obtained from the EXPOLOG.DAT file written by Ed Jenkins) is shown below. The total integration time is an estimate for the total amount of observation time devoted to each object. The exposure sequence numbers describe the number and sequence of the individual observations. The numbers in parentheses indicate the number of frames used in the eta UMa exposures (511 frames were used for all others). Background exposures are not included in the table. in the table.
| Object Name |
Total Integration Time (sec) |
Exposure Sequence Numbers |
|---|---|---|
| gamma2 Vel | 1476 | 89-108 239-251 323-330 |
| zeta Ori | 2412 | 109-124 195-214 378-408 |
| zeta Pup | 1476 | 125-140 276-294 440-445 |
| gamma Cas | 1872 | 141-148 220-238 331-355 |
| epsilon Ori | 1836 | 150-173 296-322 |
| alpha Eri | 2088 | 175-194 253-274 416-424 715-721 |
| beta Cru | 946 | 356-375 410-415 |
| eta UMa (atmos. probe) | 3432 | 447-454 (511) 455-514 (255) 515-522 (511) 525-532 (511) 533-592 (255) 594-601 (511) |
| kappa Ori | 3456 | 602-649 653-700 |
| beta Cen | 288 | 702-713 |