RST·DATA

Roman Ultra Deep Field

sim_udf_f184_024 · GO-1042 · WFI SCA13

simulated

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

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

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

Exposure ID
sim_udf_f184_024
Instrument
WFI
Detector
SCA13
Optical element
F184
Data level
L2
Integration
12m 47s
Resultants
64
Mid-exposure
05 Feb 2026, 21:42 UTC
Mission day
L+-205.40
Product size
191 MB
5σ point-source depth
27.76 AB

Pointing

RA (J2000)
03h32m10.73s
Dec (J2000)
−27°54′31.3″
RA (deg)
53.044729
Dec (deg)
-27.908687
Footprint
0.125° on a side
Pixel scale
0.11″/px

Band

F1841.842 µm pivot
0.4 µmvisible → near-infrared2.4 µm

Reaches past the H band for the highest-redshift sources.

Access

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

sim_udf_f184_024_l2.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.