The Post-Cryo Preliminary Data Release is superseded by the 2013 Post-Cryo Data Release. Please use the Post-Cryo Single-Exposure (Level 1) Image Inventory Table.
The following table contains brief descriptions of all metadata information characterizing single-exposure image frames. The table also contains some processing-specific information, such as the date and time when the archive preparation software was run, and basic photometric parameters used for photometry.
The columns in the following table are:
Column Name | Format | Units | nulls | Description | |
---|---|---|---|---|---|
band | %1d | ---- | no | WISE band number for the image. | |
naxis | %1d | ---- | no | Number of data axes; it is always '2' for two-dimensional images. | |
naxis1 | %4d | pixels | no | Length of data axis 1 or number of columns in the image. | |
naxis2 | %4d | pixels | no | Length of data axis 2 or number of rows in the image. | |
wrelease | %20s | ---- | no | The version number of the WISE multiframe pipeline used for this current data release. | |
crpix1 | %6.1f | pixel | no | Axis 1 reference pixel at position crval1,crval2: 0.5*(naxis1+1) | |
crpix2 | %6.1f | pixel | no | Axis 2 reference pixel at position crval1,crval2: 0.5*(naxis2+1) | |
crval1 | %16.12f | degrees | no | Reference Right Ascension at crpix1,crpix2 for EQUINOX. | |
crval2 | %16.12f | degrees | no | Reference Declination at crpix1,crpix2 for EQUINOX. | |
ctype1 | %13s | ---- | no | Projection type for axis 1. It is always set to use the SIN (orthographic) projection; for the definition, see Calabretta & Greisen, 2002. | |
ctype2 | %13s | ---- | no | Projection type for axis 2. It is always set to use the SIN (orthographic) projection; for the definition, see Calabretta & Greisen, 2002. | |
equinox | %6.1f | degrees | no | Equinox of the World Coordinate System (WCS). | |
bunit | %20s | ---- | no | Image pixel units: Data Number (DN) for intensity and uncertainty filetypes; the mask filetype is unitless. Image filetypes are described in section IV.3a. | |
elon | %16.12f | degrees | no | Ecliptic longitude of the reference pixel. CAUTION: This coordinate should not be used as an astrometric reference. | |
elat | %16.12f | degrees | no | Ecliptic latitude of the reference pixel. CAUTION: This coordinate should not be used as an astrometric reference. | |
glon | %16.12f | degrees | no | Galactic longitude of the reference pixel. CAUTION: This coordinate should not be used as an astrometric reference. | |
glat | %16.12f | degrees | no | Galactic latitude of the reference pixel. CAUTION: This coordinate should not be used as an astrometric reference. | |
ra1 | %16.12f | degrees | no | Right ascension (J2000) at corner #1 (crpix1,crpix2=-0.5,-0.5) | |
dec1 | %16.12f | degrees | no | Declination (J2000) at corner #1 (crpix1,crpix2=-0.5,-0.5) | |
ra2 | %16.12f | degrees | no | Right ascension (J2000) at corner #2 (crpix1,crpix2=naxis1+0.5,-0.5) | |
dec2 | %16.12f | degrees | no | Declination (J2000) at corner #2 (crpix1,crpix2=naxis1+0.5,-0.5) | |
ra3 | %16.12f | degrees | no | Right ascension (J2000) at corner #3 (crpix1,crpix2=naxis1+0.5,naxis2+0.5) | |
dec3 | %16.12f | degrees | no | Declination (J2000) at corner #3 (crpix1,crpix2=naxis1+0.5,naxis2+0.5) | |
ra4 | %16.12f | degrees | no | Right ascension (J2000) at corner #4 (crpix1,crpix2=-0.5,naxis2+0.5) | |
dec4 | %16.12f | degrees | no | Declination (J2000) at corner #4 (crpix1,crpix2=-0.5,naxis2+0.5) | |
magzp | %9.5f | mag | no | Relative photometric zero-point magnitude for the image. | |
magzpunc | %9.6f | mag | no | 1-sigma uncertainty in the photometric zero-point magnitude for the image. | |
scan_id | %6s | ---- | no |
Scan identifier. This is a six character string that identifies a block of
survey exposures that are acquired between two flight system maneuvers,
such as reorientation of the instrument boresight near the ecliptic poles,
or slews to acquire TDRSS for data downlink contacts. Because
maneuvers often take place near the ecliptic poles, the scan number
is roughly associated with a half-orbit's worth of images. However,
scans can cover less or more than half of the arc between ecliptic poles.
The scan_id has the general form SSSSSx, where
The first scan whose data are used in the Preliminary Data Release is scan 08745a. This was the first scan after the NEP crossing in the 4372nd WISE orbit. The final scan included in the Release is 12514a, the first scan after the SEP crossing in the 6257th WISE orbit. |
|
scangrp | %2s | ---- | no | Scan group identifier (the last two characters of the scan_id, used to group scan data on the disks). | |
frame_num | %3d | ---- | no | Number of the frameset for this image. The
identifier has the general form MMM, a zero-filled
three-digit number.
The frameset number is computed based on time bins which count from the scan start time: where
For example, a frame with a start time 1234 secs after the scan start time would have a frame number of 124. N.B.
|
|
l0file | %200s | ---- | no | The corresponding level 0 image file name. | |
date_obs | %24s | datetimeZ | no | The date and time of the mid-point of the frameset exposure, in UTC. The mid-point is defined as the time the optical boresight crosses the center of the WISE focal planes. This time is the same for both bands. | |
mjd_obs | %14.8f | mjdate | no | The Modified Julian Date of the mid-point of the frameset exposure. | |
dtanneal | %18.11f | seconds | no | Elapsed time in seconds since the last anneal. | |
utanneal | %24s | datetimeZ | no | The date and time of the last anneal, UTC. | |
unixt | %16.5f | seconds | no | UNIX date-time in seconds of the mid-point of the frameset exposure, in UTC. The mid-point is defined as the time the optical boresight crosses the center of the WISE focal planes. This time is the same for both bands. | |
ephemt | %16.6f | seconds | no | Ephemeris date-time in seconds of the mid-point of the frameset exposure, in UTC. The mid-point is defined as the time the optical boresight crosses the center of the WISE focal planes. This time is the same for all bands, whereas the exposure times in W1 and W2 are different than in W3 and W4. | |
exptime | %4.1f | seconds | no | Single image frame exposure time in seconds; exposure times in W1 and W2 are different than in W3 and W4. | |
tsamp | %4.1f | seconds | no | The time interval between non-destructively read samples-up-the-ramp in on-board processing. | |
wcdelt1 | %21.18f | degrees/pixel | no | Axis 1 pixel scale at the reference pixel crpix1, crpix2, in degrees per pixel. See pxscal1 for the arcsec equivalent. | |
wcdelt2 | %21.18f | degrees/pixel | no | Axis 2 pixel scale at the reference pixel crpix1, crpix2, in degrees per pixel. See pxscal2 for the arcsec equivalent. | |
crder1 | %20.14e | degrees | no | Uncertainty in crval1 (right ascension). | |
crder2 | %20.14e | degrees | no | Uncertainty in crval2 (declination). | |
csdradec | %20.14f | degrees | no | Costandard deviation in crval1 and crval2 (RA and Dec), the square root of the absolute value of the covariance between RA and Dec with the sign of the covariance re-attached to the square-root if it was originally negative. | |
pxscal2 | %17.14f | arcsec/pixel | no | Axis 1 arcsec per pixel scale at the reference pixel crpix1, crpix2. | |
pxscal2 | %17.14f | arcsec/pixel | no | Axis 2 arcsec per pixel scale at the reference pixel crpix1, crpix2. | |
uncrts1 | %20.14e | degrees/pixel | no | Uncertainty in the pixel scale wcdelt1. | |
uncrts2 | %20.14e | degrees/pixel | no | Uncertainty in the pixel scale wcdelt2. | |
wcrota2 | %18.13f | degrees | no | Image twist: the position of the image y-axis (axis2) West of North at the EQUINOX in the opposite direction of the conventional Position Angle, where position angle (P.A.) = -CROTA for J2000. | |
pa | %18.13f | degrees | no | The position angle of the positive image y-axis (axis2), East of North at the EQUINOX. | |
uncrtpa | %21.18f | degrees | no | The uncertainty in the position angle (PA). | |
skew | %5.1f | ---- | no | The measurement of non-orthogonality of the image frame axes. | |
cd1_1 | %21.18f | degrees/pixel | no | WCS rotation matrix element 1,1 encoding frame rotation and pixel scale. | |
cd1_2 | %21.18f | degrees/pixel | no | WCS rotation matrix element 1,2 encoding frame rotation and pixel scale. | |
cd2_1 | %21.18f | degrees/pixel | no | WCS rotation matrix element 2,1 encoding frame rotation and pixel scale. | |
cd2_2 | %21.18f | degrees/pixel | no | WCS rotation matrix element 2,2 encoding frame rotation and pixel scale. | |
debgain | %10.3f | e-/DEB ADU | no | On-board Digital Electronics Box gain (with units of e-/observed DN). This factor is used to convert DN to electrons. | |
febgain | %10.4f | e-/SUR ADU | no | Flight electronics box gain for individual non-destructive read samples up-the-ramp. | |
qa_status | %9s | ---- | no |
This string indicates Quality Assurance status for the scan and frameset:
|
|
qual_frame | %2d | ---- | no | This integer indicates the quality score value for the Single-exposure image frameset, with values of 0 (poor quality), 5, or 10 (high quality). The value is determined by the minimum of the quality factors qc_fact, qn_fact, and qi_fact, multiplied by ten. | |
qc_fact | %3.1f | ---- | no | This quality factor gauges the quality of completion of the Single-exposure image frameset. If the status value from the processing pipeline was equal to 0 (indicating a problem-free completion), then qc=1.0. Otherwise, qc=0.0 because the frameset failed to complete processing. All framesets in the Database have received qc values of 1.0. | |
qi_fact | %3.1f | ---- | no | This quality factor gauges the image shape quality of the Single-exposure image frameset. It checks for potential image smearing by using the axial ratio of the PSF calculated from a subset of sources in the frameset. The value of qi is 1.0 if the axial ratio b/a > 0.60; otherwise it is 0.0. | |
qn_fact | %3.1f | ---- | no | This quality factor indicates the background and noise characteristics quality of the Single-exposure frameset. | |
qa_fact | %3.1f | ---- | no | This quality factor gauges the astrometric quality. If the standard deviation of WISE positions with respect to the 2MASS Point Source Catalog positions is < 0.5 arcsec on each axis (or 0.71 arcsec RSS), for sources having SNR > 20 in at least one band, then qa=1.0. Otherwise, qa=0.0 | |
qual_scan | %2d | ---- | no | This integer indicates the quality score value for the scan containing the Single-exposure image frameset, with values of 0 (poor quality), 5, or 10 (high quality). The value is determined by the minimum of the quality factors qs1_fact, qs5_fact, and qp_fact, multiplied by ten. | |
qs1_fact | %3.1f | ---- | no | This quality factor indicates the quality of scan synchronization as judged from the overall 1x1 PSF grid computed by the PSF Moments routine and evaluated based on the effective number of noise pixels. | |
qs5_fact | %3.1f | ---- | no | This quality factor indicates the quality of scan synchronization as judged from the overall 5x5 PSF grid computed by the PSF Moments routine and evaluated based on the effective number of noise pixels. | |
qp_fact | %3.1f | ---- | no | This quality factor indicates the scan photometric quality. If the scan's photometric zero-point offset computed using profile-fit photometry (pzp) falls within a certain range about 0, the value of qp_fact is 1.0; otherwise it is 0.0. | |
qs_fact | %4.1f | ---- | no | This quality factor is not currently used. | |
cntr | %12d | ---- | no | Unique sequential identification number for the image metadata table entry. | |
x | %19.16f | ---- | yes | unit sphere (x,y,z) position x value | |
y | %19.16f | ---- | yes | Unit sphere (x,y,z) position y value | |
z | %19.16f | ---- | yes | Unit sphere (x,y,z) position z value | |
spt_ind | %9d | ---- | yes | HTM spatial (x,y,z) index key |
Last Update: 2013 April 11