Atlas Image Tiling Geometry

Introduction

We present the tiling geometry to represent the layout of Atlas Image (coadd) footprints over the sky. A script "TileWISEsky" was written which takes as input a linear (square) tile size, a pixel scale, and a minimum linear overlap between any two adjacent tiles. It generates the equatorial and ecliptic coordinates of the tile centers and corners, and their corresponding x, y, z coordinates on a unit sphere. The position angles of all tiles are zero, i.e., a vector from the center of each tile in the +Y-axis direction points to equatorial north. The tiles are optimally arranged in separate iso-declination bands. Example coverages at an equatorial pole and on the equator are shown below.

Specifics:

 Number of tiles (footprints) on sky = 18240
 Number of iso-declination bands = 119
 Storage assuming 4 Bytes/pixel, 12 coadd products/tile = 14.69 TB (uncompressed)
 Input pixel size = 1.375000 arcsec/pixel
 Input linear tile size = 4096 pixels = 1.564444 deg
 Input linear minimum tile overlap = 180.000000 arcsec
 Position metadata: coadd_layout-a.tbl

Figure 1 - Mosaic of WISE Atlas Image tiles inside a declination band of ~|82.4°| (=5th band from the center). This mosaic can be downloaded in FITS format here. Click on panel to enlarge.


Figure 2 - Mosaic of WISE Atlas Image tiles using same sizes/scales as in Figure 1 but on the celestial equator. Mosaic spans ~ 6° × 6°. This can be downloaded in FITS format here. Click on panel to enlarge.



Last update - 18 June 2010
F. Masci - IPAC/Caltech