RST·DATA

Time Domain — Northern Field

r1406407005013_0013_wfi15 · CCS-HLTDS · WFI SCA15

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

The northern time-domain pointing, close to the north ecliptic pole where the observatory's field of regard stays open year-round.

Program
High Latitude Time Domain Survey
Program ID
CCS-HLTDS
Field centre RA
18h00m00.00s
Field centre Dec
+66°30′00.0″
Galactic latitude
29.8°
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, 07:43 UTC

Exposure

Exposure ID
r1406407005013_0013_wfi15
Instrument
WFI
Detector
SCA15
Optical element
P127
Data level
L2
Integration
3m 17s
Resultants
16
Mid-exposure
26 Jan 2027, 07:43 UTC
Mission day
L+149.02
Product size
191 MB
5σ point-source depth
27.01 AB

Pointing

RA (J2000)
17h59m59.80s
Dec (J2000)
+66°33′27.2″
RA (deg)
269.999176
Dec (deg)
66.557555
Footprint
0.125° on a side
Pixel scale
0.11″/px

Band

P1271.050 µm pivot
0.4 µmvisible → near-infrared2.4 µm

Low-resolution prism for supernova classification.

Access

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

r1406407005013_0013_wfi15_l2.asdf

Open MAST

More of Time Domain — Northern 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.