RST·DATA

Roman Ultra Deep Field

r8553302008008_0008_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 · 10 Jan 2027, 09:34 UTC

Exposure

Exposure ID
r8553302008008_0008_wfi03
Instrument
WFI
Detector
SCA03
Optical element
F158
Data level
L3
Integration
18m 36s
Resultants
93
Mid-exposure
10 Jan 2027, 09:34 UTC
Mission day
L+133.10
Product size
765 MB
5σ point-source depth
27.62 AB

Pointing

RA (J2000)
03h32m33.38s
Dec (J2000)
−27°41′57.3″
RA (deg)
53.139104
Dec (deg)
-27.699262
Footprint
0.460° on a side
Pixel scale
0.11″/px

Band

F1581.577 µm pivot
0.4 µmvisible → near-infrared2.4 µm

H-band; a core survey filter.

Access

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

r8553302008008_0008_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.