RST·DATA

HLWAS Tile B

sim_hlwas-b_f129_006 · CCS-HLWAS · WFI SCA12

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

A wide-survey tile centred on the COSMOS region, where three decades of multiwavelength imaging give Roman's photometric redshifts an unusually strong calibration anchor.

Program
High Latitude Wide Area Survey
Program ID
CCS-HLWAS
Field centre RA
10h00m24.00s
Field centre Dec
+02°12′00.0″
Galactic latitude
42.1°
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_hlwas-b_f129_006
Instrument
WFI
Detector
SCA12
Optical element
F129
Data level
L2
Integration
8m 56s
Resultants
45
Mid-exposure
25 Dec 2025, 05:04 UTC
Mission day
L+-248.09
Product size
191 MB
5σ point-source depth
25.53 AB

Pointing

RA (J2000)
10h00m26.31s
Dec (J2000)
+02°00′21.8″
RA (deg)
150.109609
Dec (deg)
2.006055
Footprint
0.125° on a side
Pixel scale
0.11″/px

Band

F1291.293 µm pivot
0.4 µmvisible → near-infrared2.4 µm

J-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.

sim_hlwas-b_f129_006_l2.asdf

Open MAST

More of HLWAS Tile B

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.