Large Magellanic Cloud
r7959405010015_0015_wfi07 · CAL-0031 · WFI SCA07
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
The standard photometric calibration field. Its well-characterised stars set the flux zero points that every other Roman observation is measured against.
Product status
Scheduled but not yet taken. The observatory has not reached this pointing in its timeline.
Scheduled in 2 months · 12 Nov 2026, 04:54 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.
r7959405010015_0015_wfi07_l1.asdf
Open MASTMore of Large Magellanic Cloud
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.