Space Telescope Science Institute
ACS Data Handbook 2011
help@stsci.edu
Table of Contents Previous Next Index Print


ACS Data Handbook > Chapter 2: ACS Data Structure > 2.4 Headers and Keywords

2.4
While the ACS image headers for WFC, HRC, HRC-ACQ, and SBC observations have very similar formats, two main differences are apparent. MAMA (SBC) headers require a slightly modified structure from the CCD (WFC, HRC) headers, and HRC-ACQ headers require several unique keywords.
ACS header keywords can be viewed in several ways. If you know the names of keywords you wish to look up, you can use the STSDAS tasks hedit or hselect tasks to query the images. The examples below show how these tasks are used to get the values for group (or extension) keywords CCDCHIP, CRVAL1, and CRVAL2. The contents of the entire primary or group header can be viewed on-screen, or by directing the output to a text file, using the task imheader.
ACS image header keywords are described in Tables 2.6 and 2.7. If you were to display the header using imheader, you’ll notice that the keywords are grouped together by their type, for example, “Target Information,” “Science Instrument Configuration,” “Calibration Switches,” and “Calibration Reference files.”
Keywords in the image’s primary header (FITS extension 0) contain parameter values that are common to the entire image dataset, and are given in Table 2.6.
Extension or group header keywords (FITS extensions > 0), as shown in Table 2.7, contain parameter values that are specific to the image group (however, many primary header keyword values are also accessible when querying an image group header).
Some keywords are no longer in use, but we include them for users who may have older data.
Most of the keywords described in Tables 2.6 and 2.7 are “user” keywords, i.e., keywords with values directly recorded in the image headers. A few keywords in the tables have the prefix “i_”; these are “standard” keywords. They cannot be accessed by tasks like eheader and imheader, but when queried by hedit and hselect, the values of standard keywords are determined on-the-fly by IRAF.
Text in normal font under the “Description” column are written as it appears in the image header. Entries in grey are keywords that do not appear in data from the current version of OTFR, but are retained here for historical reasons. Additional information is conveyed in italics.
TARGET INFORMATION (All Detectors)
PROPOSAL INFORMATION (All Detectors)
EXPOSURE INFORMATION (All Detectors)
Number of gyros scheduled, T=3+OBAD. (Number of gyros available for use.)
Exposure duration (seconds)--calculated. (Exposure time as executed.)
QUALCOM1, QUALCOM2, QUALCOM3, QUALITY
POINTING INFORMATION (All Detectors)
DIAGNOSTIC KEYWORDS (All Detectors)
SCIENCE INSTRUMENT CONFIGURATION (All Detectors, Except Where Noted)
MAMA OFFSETS (SBC Only)
CALIBRATION SWITCHES: PERFORM, OMIT (All Detectors, Except Where Noted)
CALIBRATION REFERENCE FILES (All Detectors, Except Where Noted)
Sky value computed by MultiDrizzle (in this section for SBC only).
PATTERN KEYWORDS (All Detectors)
POST FLASH PARAMETERS (WFC, HRC, HRC ACQ)
ENGINEERING PARAMETERS (WFC, HRC, HRC ACQ)
Commanded gain of CCD (electrons/DN).
ASSOCIATION KEYWORDS (All Detectors)
 
Many primary header keywords also appear in the extension headers. However, only keywords that are unique to extension headers are listed here. Text in normal font under the “Description” column are written as it appears in the image header. Entries in grey are keywords that do not appear in data from the current version of OTFR, but are retained here for historical reasons. Additional information is conveyed in italics.
ASSOCIATION KEYWORDS (All Detectors)
Number of data axes. (For ACS images, value is set to 2.)
Only one group (within the extension).
Brightness units (counts, electrons, electrons/sec).
Offset in X to subsection start. (x coordinate of the first science pixel in the SCI array.)
Offset in Y to subsection start. (y coordinate of the first science pixel in the SCI array.)
Reciprocal of sampling rate in X. (The reference pixel size in units of the current pixel size.)
Reciprocal of sampling rate in Y. (The reference pixel size in units of the current pixel size)
PHOTOMETRY KEYWORDS (All Detectors)
Number of segments containing fill. (Number of segments for which data was lost in transmission and filled with a fill pattern prior to arriving at STScI.)
PODPS fill present (T/F). (Indicates if there are missing packets in the data stream; in such cases, the OPUS pipeline inserts fill packets so that the image can be processed by analysis software.)
Science telemetry fill data present? (T=1/F=0). (Indicates if errors were found in the science dataset at the Space Telescope Data Capture Facility; if there are missing packets or failed segments, fill data is inserted as placeholders.)
MAMA jMDECODT pwb temp from eng snap 1 (deg. C) (Temperature at the start of observation.)
MAMA JMDECODT pwb temp from eng snap 2 (deg. C) (Temperature at the end of observation.)
REPEATED EXPOSURES INFO (WFC, HRC, HRC ACQ)
Serious data quality flags. (Bad pixels that are not included in calculations for header keyword image statistics, e.g., GOODMEAN, NGOODPIX.)
A_0_2, B_0_2, A_1_1, B_1_1, A_2_0, B_2_0, A_0_3, B_0_3, A_1_2, B_1_2, A_2_1, B_2_1, A_3_0, B_3_0, A_0_4, B_0_4, A_1_3, B_1_3, A_2_2, B_2_2, A_3_1, B_3_1, A_4_0, B_4_0
Non-linear or high-order polynomial coefficients, in the SIP convention, describe the geometric distortion model for each image group. They are present for use by SIP-enabled code such as DS9 and may be used by future versions of the pipeline software, multidrizzle, and other STSDAS tasks.
A_ORDER, B_ORDER

1
Values before geometric distortion corrections.


Table of Contents Previous Next Index Print