The contents of the header include:
Index Content Example ^^^^^^^^^^^^^ ^^^^^^^ 1 Disclaimer NOT ORIGINAL PROJECT DATA PRODUCT 2 EID + dispersion + aperture SWP1707LOWLARGE 3 Object ID NGC 7009 4 RA (1950) 21:01:30 5 DEC (1950) -11:34:00 6 IUE Object Class 70 7 Trailed flag NO-TRAIL 8 Segmented exposure flag NO 9 Exposure time (seconds) 119.473 10 Observation date dd/mm/yy 03/06/78 11 Observation time (UT) 17:47:00 12 Observation day of year 154 13 THDA at start of exposure 9.50 14 Processing date dd/mm/yy 12/10/95 15 Processing station GSFC 16 JD of observation 2443663.24097 17 Estimated max continuum in DN 79 18 Mean background in DN 23
Immediately following the header are 6 columns of numbers. There are 495 rows of data for the SWP files and 563 rows for the LWP/LWR files. The format of each row is f7.2, 2e10.2, 3i6, e.g.,
1150.58 4.75e-12 1.26e-12 272 85 0 1152.26 2.02e-12 1.09e-12 271 38 0 1153.93 2.57e-12 1.04e-12 270 51 0
These columns represent (in order):
Quantity Units ^^^^^^^^ ^^^^^ Wavelength Å Flux erg cm-2 sec-1 Å-1 Standard deviation erg cm-2 sec-1 Å-1 Background level IUE Flux Numbers (FN) Net spectrum IUE Flux Numbers (FN) IUE data quality (nu) flag numbered code
The contents of the header are:
These are followed immediately by 3 columns of numbers. There are 16500
or 12250 (for short or long wavelength spectra) rows for the SWP files.
The format of each row is 3e10.2, e.g.,
These columns are:
The MXHI gzip file
The files available for downloading from the browser page are gzipped
ASCII files which consist of an abbreviated header, a combined order
spectrum resampled onto a uniform grid with a spacing of either 0.05
or 0.10 Å (for short or long wavelength spectra), and
its accompanying noise and background vectors (all in ergs/cm^2/s/Ang)).
The flux and error vectors are the weighted mean of the original points
which fell in the 0.05 (0.10) Å bin and the weighted error in the
mean. An entry of -1 in the flux vector implies that all the nu flags for
the data in that bin were < -512 (see above). The corresponding noise
vector then has an entry of +1. Otherwise, the flags were ignored in the
rebinning procedure.
Index Content Example
^^^^^^^^^^^^^ ^^^^^^^
1 Disclaimer NOT ORIGINAL IUE PROJECT DATA PRODUCT
2 EID + dispersion + aperture SWP46933HIGHLARGE
3 Object ID HD 55857
4 RA (1950) 07:11:35
5 DEC (1950) -27:16:09
6 IUE Object Class 20
7 Trailed flag NO-TRAIL
8 Segmented exposure flag NO
9 Exposure time (seconds) 149.784
10 Observation date dd/mm/yy 13/02/93
11 Observation time (UT) 20:03:49
12 Observation day of year 44
13 THDA at start of exposure 9.51
14 Processing date dd/mm/yy 26/10/96
15 Processing station GSFC
16 JD of observation 2449032.33598
17 Estimated max continuum in DN 177
18 Mean background in DN 35
19 Formula for wavelength scale w(k) = 0.05*k +1150, k = 0, 16499 (SWP) or
w(k) = 0.10*k +1900, k = 0, 12249 (LWP and LWR)
1.55e-09 6.89e-10 -6.68e-10
1.23e-09 4.57e-10 -6.69e-10
9.77e-10 6.16e-10 -6.70e-10
1.07e-09 4.44e-10 -6.72e-10
4.87e-10 4.30e-10 -6.72e-10
1.45e-09 6.40e-10 -6.74e-10
Quantity Units
^^^^^^^^ ^^^^^
flux
The IUE browse files were conceived and originally implemented by Dr. Derck Massa, Dr. Nancy Oliversen, and Ms. Patricia Lawton, then members of the GSFC Astrophyics Data Facility (ADF) staff under direction of Dr. Michael Van Steenberg. Some modifications have been made as part of the transition to MAST maintenance.