HLWAS Tile A
r3055604001011_0011_wfi06 · CCS-HLWAS · WFI SCA06
Procedural preview
Not sky data · awaiting first light
1:1 footprint
7.5′ across
0 sources drawn
Band
Stretch
Gain 1.00×
Drag to pan, scroll to zoom, double-click to zoom in. Arrow keys pan, + and − zoom, 0 resets. Switching bands re-colours the same patch of sky rather than replacing it, so you can blink between filters the way you would with real multiband imaging.
About this field
One tile of the roughly 5,000 square degree wide survey. Chosen for low Galactic dust and overlap with existing deep optical imaging, it is the workhorse dataset for weak lensing and galaxy clustering cosmology.
Product status
Scheduled but not yet taken. The observatory has not reached this pointing in its timeline.
Scheduled in 5 months · 26 Jan 2027, 14:17 UTC
Exposure
Pointing
Band
Y-band; a core High Latitude Wide Area Survey filter.
Access
Roman products are distributed through MAST at STScI. Files follow the naming convention below; nothing is downloadable from this site.
r3055604001011_0011_wfi06_l2.asdf
Open MASTMore of HLWAS Tile A
All products in this field →The image above is procedurally generated. Source positions, colours and crowding are derived from the field's galactic latitude and character and from the band's pivot wavelength, and every exposure of a field draws the same sky so dithers line up — but none of it is data from the telescope.