South Ecliptic Pole (SEP) Mosaics |
Below are links to JPEGs of mosaics at eight different bands, all mapped onto a common footprint. The size of the footprint is 1.5 × 1.5 deg2 centered at the SEP: R.A. = 90.0°, Dec = -66.5607° (J2000.0); galactic coordinates: l = 276.3840°, b = -29.8112°. Its orientation (CROTA2) is 287.79297°, chosen to be the average orientation of MIPS scans from Director's Discretionary Time (DDT) observations. The pixel scale is 1″ throughout. All coordinate grid overlays are in the ecliptic system.
Mosaics were made exclusively using modules proposed for the WISE Science Data processing System (WSDS): Bmatch for background (offset) matching; AWOD for temporal outlier detection and masking; AWAIC for frame co-addition. For the 2MASS mosaics, outlier masking was omitted due to insufficient depth-of-covarage, but throughput (gain) matching was performed to get all inputs on the same photometric calibration scale. IRAC and MIPS mosaics have pixel units of MJy/sr, while 2MASS mosaics are in counts (DN/pixel) with the photometric zeropoint (in magnitudes) given by MAGZP in their FITS headers. Please contact the author for actual FITS data.
• J(blue)_H(green)_K(red)_Mosaic
• ZOOM_J(blue)_H(green)_K(red)_Mosaic
• J(blue)_3.6μm(green)_8μm(red)_Mosaic
• ZOOM_J(blue)_3.6μm(green)_8μm(red)_Mosaic
• 4.5μm(blue)_8μm(green)_24μm(red)_Mosaic
• ZOOM_4.5μm(blue)_8μm(green)_24μm(red)_Mosaic