RST·DATA

Galactic Bulge Time Domain

sim_gbtds_f158_017 · CCS-GBTDS · WFI SCA15

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 dense window toward the Galactic centre, imaged every fifteen minutes during six-week seasons. Microlensing here is expected to yield thousands of cold exoplanets, including free-floating worlds bound to no star at all.

Program
Galactic Bulge Time Domain Survey
Program ID
CCS-GBTDS
Field centre RA
17h52m00.00s
Field centre Dec
−28°53′60.0″
Galactic latitude
-1.1°
Field character
bulge

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_gbtds_f158_017
Instrument
WFI
Detector
SCA15
Optical element
F158
Data level
L2
Integration
17m 11s
Resultants
86
Mid-exposure
20 Nov 2025, 18:20 UTC
Mission day
L+-282.54
Product size
191 MB
5σ point-source depth
25.54 AB

Pointing

RA (J2000)
17h52m45.44s
Dec (J2000)
−29°03′24.0″
RA (deg)
268.189314
Dec (deg)
-29.056670
Footprint
0.125° 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.

sim_gbtds_f158_017_l2.asdf

Open MAST

More of Galactic Bulge Time Domain

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.