HLWAS Tile C
sim_hlwas-c_f106_007 · CCS-HLWAS · WFI SCA18
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
Northern-cap tile covering the Extended Groth Strip, a heavily studied deep field that lets Roman's shape measurements be checked against existing high-resolution imaging.
Product status
A pre-flight simulation product. Generated on the ground to build and test the calibration pipeline before launch — useful for developing analysis code, but it is synthetic, not sky.
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.
sim_hlwas-c_f106_007_l2.asdf
Open MASTMore of HLWAS Tile C
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.