RST·DATA

Roman Ultra Deep Field

r8553301008001_0001_wfi03 · GO-1042 · WFI SCA03

planned

Procedural preview

Not sky data · awaiting first light

1:1 footprint

27.6′ 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

Pointed at the Hubble Ultra Deep Field. Roman covers in a single exposure a patch of sky that took Hubble hundreds of orbits, with the same angular resolution.

Program
Guest Observer
Program ID
GO-1042
Field centre RA
03h32m38.40s
Field centre Dec
−27°47′24.0″
Galactic latitude
-54.4°
Field character
deep

Product status

Scheduled but not yet taken. The observatory has not reached this pointing in its timeline.

Scheduled in 4 months · 01 Jan 2027, 11:53 UTC

Exposure

Exposure ID
r8553301008001_0001_wfi03
Instrument
WFI
Detector
SCA03
Optical element
F213
Data level
L3
Integration
5m 44s
Resultants
29
Mid-exposure
01 Jan 2027, 11:53 UTC
Mission day
L+124.19
Product size
765 MB
5σ point-source depth
27.55 AB

Pointing

RA (J2000)
03h32m01.55s
Dec (J2000)
−27°41′34.7″
RA (deg)
53.006452
Dec (deg)
-27.692973
Footprint
0.460° on a side
Pixel scale
0.11″/px

Band

F2132.125 µm pivot
0.4 µmvisible → near-infrared2.4 µm

Reddest band; probes the most obscured and most distant objects.

Access

Roman products are distributed through MAST at STScI. Files follow the naming convention below; nothing is downloadable from this site.

r8553301008001_0001_wfi03_l3.asdf

Open MAST

More of Roman Ultra Deep Field

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.