LRD Watch DR1 · catalog object

LRDW J141924.13+525157.6

catalogTENTATIVEBH* channelEGS (CEERS pointing 3)

RA 14:19:24.139 214.8505804°

Dec +52:51:57.68 52.8660226°

SIMBAD within 2″ · ESASky

Images

F115W image, 3.2 arcsec across, north up — F115W0.03″ px

F150W image, 3.2 arcsec across, north up — F150W0.03″ px

F200W image, 3.2 arcsec across, north up — F200W0.03″ px

F277W image, 3.2 arcsec across, north up — F277W0.06″ px

F356W image, 3.2 arcsec across, north up — F356W0.06″ px

F410M image, 3.2 arcsec across, north up — F410M0.06″ px

F444W image, 3.2 arcsec across, north up — F444W0.06″ px

Colour composite: F444W red, F356W green, F277W blue, 3.2 arcsec across, north up — compositebar 1″

3.2″ across, north up, east left, resampled from the deepest mosaic covering the object in each band; ticks mark the catalogue position. Each band is stretched on its own noise; the composite shares one flux scale, so its colour is real. No coverage in F090W.

Spectral energy distribution

NIRCam wide
NIRCam medium
2σ upper limit (S/N < 2)

Aperture fluxes in a 0.16″-radius circle, not corrected to total; the values are in the photometry table below. The gold line marks the Balmer limit (3646 Å rest) at z = 3.650.

At a glance

Tier: TENTATIVE
Found by: BH* channel
Redshift: 3.650 DJA grade 3, PRISM
Spectral shape: inconclusive de Graaff+25 criteria
F444W: 23.40 AB S/N 390, 0.16″ aperture
F277W − F444W: not in the colour lane
BH* share: 0.67 cliff_degraaff25; Δχ² galaxy 4.3, dwarf 154.1
Compactness: growth ratio 2.250 stars 2.257
Balmer break: 4.79 ± 0.21 F200W/F150W, clean
Image vetting: half-stack pass; 1 flag(s)
Literature: 0 catalogue(s), 6 AGN paper(s) within 0.032″

Vetting

Image vettingnot applicable
Half-stack testpass
Artifact risknone
Neighbourflagged
Extendedno

BH* channelevidence dchi2_gal=4.3 dchi2_bd=154.1
BH* channelBH* share 0.67 below 0.8 (composite)
BH* channelneighbor-contam footprint-overlap id 5989 at 1.43" (npix=2207, r_eq=1.67")

Redshifts

Each redshift keeps its own column. Photometric redshifts of little red dots are unreliable: against spectra, about a third of AGN-template redshifts (z_agn; 31 of 95 in the last purity run) and about half of galaxy-template redshifts at z > 3 were catastrophic outliers (methods Section 8).

Column	What it is	z	Source
`z_spec`	Spectroscopic, DJA grade 3	3.6501	glazebrook-egs-v4_prism-clear_2565_118854.spec.fits
`z_vet`	Adopted by vetting	3.6501	zspec:dja:glazebrook-egs-v4_prism-clear_2565_118854.spec.fits (pipeline z_vet 3.649 from zspec:vizier_J_A+A_691_A240_ceersp.csv:70720)
`z_phot`	Photometric (P(z) peak)	—	not fitted
`z_bhs`	BH* channel fit	2.918	cliff_degraaff25
`z_agn`	Colour-lane fit	—	—

Spectral checks

V-shape (spectrum): inconclusive
Star (spectrum): no
V-shape (photometry): not measurable β_UV not measured, β_opt not measured at z_agn
Line in F410M: none 1 line-free optical band(s)
Line-ambiguous: no
Settling verdict: not evaluated

Literature

Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.

Baccus+2026 (DJA census) broad-line AGN
Hviding+2025 broad-line AGN
Jones+2025 broad-line AGN
Rusakov+2026 broad-line AGN
Scholtz+2026 (LRD/LBD BLR) broad-line AGN
Taylor+2025 (CEERS/RUBIES) broad-line AGN

Photometry

Circular aperture of radius 0.16″ at each band's native resolution, background from a 0.40–0.65″ annulus, programmes combined by inverse variance. For a point source multiply by the field's aperture correction (r = 0.16″ → 0.70″). Grey rows are below S/N 2.

Band	Instrument	Pivot (µm)	f (nJy)	σ (nJy)	AB mag	S/N	Ap. corr.
F115W	NIRCam wide	1.154	18.16	3.07	28.25	5.9	1.35
F150W	NIRCam wide	1.501	80.78	3.37	26.63	24.0	1.34
F200W	NIRCam wide	1.989	386.55	4.00	24.93	96.6	1.35
F277W	NIRCam wide	2.762	944.27	3.74	23.96	252.7	1.44
F335M	NIRCam medium	3.362	1116.59	7.25	23.78	154.0	1.49
F356W	NIRCam wide	3.568	1183.94	3.97	23.72	298.5	1.51
F360M	NIRCam medium	3.624	1219.31	7.37	23.68	165.5	1.50
F410M	NIRCam medium	4.082	1441.45	6.89	23.50	209.1	1.53
F444W	NIRCam wide	4.404	1588.92	4.08	23.40	389.8	1.58

Provenance

Field: EGS (CEERS pointing 3) (miri3)
Programmes: 01345, 08559 behind every mosaic the field measured
Pipeline rows merged: 1 all at one position
Detection pass: original
Release build: 33af9933d1cc 2026-10-17T14:29:44Z

Image sources

Band	Mosaic	Native pixel	Coverage
F115W	`jw01345-o003_t023_nircam_clear-f115w_i2d.fits`	0.031″	1.00
F150W	`jw01345-o003_t023_nircam_clear-f150w_i2d.fits`	0.031″	1.00
F200W	`jw01345-o003_t023_nircam_clear-f200w_i2d.fits`	0.031″	1.00
F277W	`jw01345-o003_t023_nircam_clear-f277w_i2d.fits`	0.063″	1.00
F356W	`jw01345-o003_t023_nircam_clear-f356w_i2d.fits`	0.063″	1.00
F410M	`jw01345-o003_t023_nircam_clear-f410m_i2d.fits`	0.063″	1.00
F444W	`jw01345-o003_t023_nircam_clear-f444w_i2d.fits`	0.063″	1.00

Cite

Anderson, Jordan (2026). LRD Watch DR1: little red dot candidates from an independent search of public JWST imaging (Version DR1) [Data set]. Cerin Amroth Research. Zenodo. https://doi.org/10.5281/zenodo.23062632 Object LRDW J141924.13+525157.6.

CC BY 4.0. Please also acknowledge the JWST programmes that took the data. LRD Watch DR1 is a vetted candidate catalogue, not a complete census: it has no selection function and cannot on its own give number densities. About the release.