0
Assigned ID: 7529
----- Attempting Submission 1 (Thu Apr 16 18:39:59 GMT 2026) -----
HST Phase I Proposal 7529 successfully submitted.
Receipt: # 7529-1
----- Attempting Submission 2 (Thu Apr 16 20:05:25 GMT 2026) -----
HST Phase I Proposal 7529 successfully submitted.
Receipt: # 7529-2
----- Attempting Submission 3 (Thu Apr 16 23:57:27 GMT 2026) -----
Setup for all targets. Correct some mistakes.
-508840322
----- Attempting Submission 1 (Sat Aug 01 08:52:15 GMT 2026) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 2 (Sat Aug 15 12:17:07 GMT 2026) -----
----- Attempting Submission 3 (Wed Aug 19 15:21:02 GMT 2026) -----
HST Phase II Proposal 18333 successfully submitted.
Receipt: # 18333-3
----- Attempting Submission 5 (Wed Aug 19 20:39:23 GMT 2026) -----
What Triggers Little Red Dots? An HST Survey of their Galactic Environments
Little Red Dots (LRDs), discovered by JWST, are an abundant and enigmatic AGN population unlike any previously known. They likely represent a common but unconventional phase of early black-hole growth. What galactic environments trigger the LRD phase, through which BH seeding and growth channels? Answering this requires high-S/N high resolution host-galaxy imaging. At high z, cosmological dimming makes resolving the host extremely challenging. Low-z LRDs, thanks to their proximity and brightness, offer the ideal laboratory.
We propose WFC3/UVIS imaging of 16 LRDs from a uniformly selected DESI DR1 sample at z=0.2-0.9, forming the largest statistical sample of low-z LRDs. We use F275W and F336W to map the rest-frame UV, and two optical medium bands to map the optical continuum. Orders of magnitude brighter than their high-z counterparts, these targets allow HST to resolve the host galaxies down to ~100 pc in the rest-frame UV. Optical imaging will cleanly separates the AGN-dominated continuum from the host through PSF decomposition. Our program will (1) reveal the galactic environments of LRDs and (2) map the host properties onto the full spectral diversity of the LRD population. This survey will pinpoint the formation channels of LRDs (e.g., dense stellar clusters, direct-collapse black holes, cold-gas accretion, or gas-rich mergers) and the conditions that trigger the LRD phase. Our program will also provide the empirical host-galaxy reference that high-z JWST samples currently lack. It will lay groundwork for upcoming LRD searches with Euclid, Roman, and Rubin, anchoring the cosmic evolution of LRDs from cosmic dawn to the present day.
Each target will be observed with WFC3/UVIS for four orbits: two orbits in F275W, one orbit in F336W, and one orbit shared between two optical filters. A four-point sub-pixel dither pattern will be used in each filter to improve PSF sampling, cosmic-ray rejection, and detector-defect mitigation. The UV observations use the full-frame CTE-optimized aperture, while the optical observations use a 1K subarray to accommodate both filters efficiently within a single orbit.
PI Xiaohui Fan is a world-leading expert in high-redshift quasars and early black-hole growth, with extensive HST and JWST program leadership.
Co-I Xiaojing Lin led the first identification of local LRDs from SDSS and the DESI DR1 assembly of the proposed sample. She leads the Magellan/FIRE near-IR campaign that characterized the optical-IR continua of the targets.
Co-Is Fuyan Bian, Zheng Cai, Mingyu Li, Yichen Liu, and Fengwu Sun are experts in AGN, galaxies, and their co-evolution, providing AGN and star-forming-galaxy spectroscopy, host-galaxy SED and morphology analysis, theoretical framing of LRD formation channels, and HST/JWST PSF decomposition required to interpret the resolved AGN/host maps delivered by this program.
Supermassive Black Holes and Active Galaxies
Galaxies
6
false
true
false
false
false
false
false
SUPPORTED
GALAXY
DWARF COMPACT
NUCLEUS
J2000
J2000
g mag=22.3 (AB), r mag = 21.3 (AB)
GALAXY
DWARF COMPACT
NUCLEUS
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J2000
g mag = 23.1 (AB), r mag = 22.5 (AB)
GALAXY
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NUCLEUS
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g mag = 22.2 AB, r mag = 20.8 AB
GALAXY
DWARF COMPACT
NUCLEUS
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GALAXY
DWARF COMPACT
NUCLEUS
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J2000
g mag = 22.8 AB, r mag = 23.4 AB
GALAXY
DWARF COMPACT
NUCLEUS
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J2000
g mag = 23.0 AB, r mag = 23.0 AB
GALAXY
DWARF COMPACT
NUCLEUS
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J2000
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GALAXY
DWARF COMPACT
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NUCLEUS
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J2000
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J2000
g mag = 23.3 AB, r mag = 22.3 AB
GALAXY
DWARF COMPACT
NUCLEUS
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J2000
g mag = 24.2 AB, r mag = 22.8 AB
GALAXY
DWARF COMPACT
NUCLEUS
J2000
J2000
g mag = 24.4 AB, r mag = 23.0 AB
WFC3/UVIS
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Imaging
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true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
1
0
The scheduling data was generated by CASM 34.2.
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 18333
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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:trans-version "20260618"
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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:low-sky "N"
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)
true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
true
1
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
(Tic-Visit
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true
3
0
The scheduling data was generated by CASM 34.2.
CASM was run in Phase II mode.
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true
1
0