RST·DATA

Time Domain — Southern Field

r1406407004014_0014_wfi03 · CCS-HLTDS · WFI SCA03

planned

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

Revisited every five days for two years to catch Type Ia supernovae out to redshift 2 and beyond. Continuous visibility from L2 is what makes a cadence this regular possible.

Program
High Latitude Time Domain Survey
Program ID
CCS-HLTDS
Field centre RA
00h38m00.00s
Field centre Dec
−44°06′00.0″
Galactic latitude
-70.2°
Field character
deep

Product status

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

Scheduled in 5 months · 26 Jan 2027, 10:58 UTC

Exposure

Exposure ID
r1406407004014_0014_wfi03
Instrument
WFI
Detector
SCA03
Optical element
F184
Data level
L2
Integration
8m 15s
Resultants
41
Mid-exposure
26 Jan 2027, 10:58 UTC
Mission day
L+149.16
Product size
191 MB
5σ point-source depth
27.31 AB

Pointing

RA (J2000)
00h38m03.77s
Dec (J2000)
−43°52′16.2″
RA (deg)
9.515703
Dec (deg)
-43.871164
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.

r1406407004014_0014_wfi03_l2.asdf

Open MAST

More of Time Domain — Southern Field

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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.