LRD Watch DR1 · catalog object

LRDW J141942.18+525644.4

catalogSILVERmain classBH* channelcolour laneEGS (CEERS pointing 2)

RA 14:19:42.181 214.9257562°

Dec +52:56:44.40 52.9456668°

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
MIRI
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 = 5.088.

At a glance

Tier: SILVER main class
Found by: BH* channel + colour lane
Redshift: 5.088 DJA grade 3, PRISM
Spectral shape: V-shaped de Graaff+25 criteria
F444W: 26.49 AB S/N 40, 0.16″ aperture
F277W − F444W: 1.47 mag strict redness
BH* share: 0.93 bhs_bb4200_b4; Δχ² galaxy 20.7, dwarf 32.2
Compactness: growth ratio 1.731 stars 2.336
Balmer break: 2.68 ± 0.79 F277W/F200W, red:Hb+OIII
Image vetting: half-stack pass; no flags raised
Literature: 3 catalogue(s), 1 AGN paper(s) within 0.020″

Vetting

Image vettingpassed
Half-stack testpass
Artifact risknone
Neighbournone
Extendedno

No vetting notes.

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	5.0884	ceers-ddt-v4_prism-clear_2750_1768.spec.fits
`z_vet`	Adopted by vetting	5.0884	zspec:dja_specz_grade3.csv:1768
`z_phot`	Photometric (P(z) peak)	7.085	68%: 2.250–7.202
`z_bhs`	BH* channel fit	5.210	bhs_bb4200_b4
`z_agn`	Colour-lane fit	7.08	AGN-inclusive templates

Spectral checks

V-shape (spectrum): V-shaped
Star (spectrum): no
V-shape (photometry): passes β_UV −0.88, β_opt 0.56 at z_agn
Line in F410M: Ha 2 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.

Barro et al. (2025)
de Graaff et al. (2025)
Kocevski et al. (2024)
Kocevski+2026 Skyfire 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	4.81	1.74	29.70	2.8	1.33–1.39
F150W	NIRCam wide	1.501	5.55	3.70	29.54	1.5	1.36
F200W	NIRCam wide	1.989	8.86	2.54	29.03	3.5	1.37
F277W	NIRCam wide	2.762	23.86	1.73	27.96	13.8	1.49
F356W	NIRCam wide	3.568	45.48	0.96	27.26	47.6	1.54–1.55
F360M	NIRCam medium	3.624	40.73	3.03	27.38	13.4	1.56
F410M	NIRCam medium	4.082	128.71	3.79	26.13	33.9	1.57
F430M	NIRCam medium	4.281	65.70	5.42	26.86	12.1	1.61
F444W	NIRCam wide	4.404	92.31	2.32	26.49	39.8	1.61
F460M	NIRCam medium	4.630	70.94	7.61	26.77	9.3	1.60
F1000W	MIRI	9.947	75.37	19.89	26.71	3.8	2.63

Provenance

Field: EGS (CEERS pointing 2) (miri2)
Programmes: 01345, 04586, 05398, 07814, 08559 behind every mosaic the field measured
Pipeline rows merged: 3 all at one position
Detection pass: original
Release build: 33af9933d1cc 2026-10-17T14:29:44Z

Image sources

Band	Mosaic	Native pixel	Coverage
F115W	`jw05398-c1208_t000_nircam_clear-f115w_i2d.fits`	0.031″	1.00
F150W	`jw01345-o002_t022_nircam_clear-f150w_i2d.fits`	0.031″	1.00
F200W	`jw01345-o002_t022_nircam_clear-f200w_i2d.fits`	0.031″	1.00
F277W	`jw01345-o002_t022_nircam_clear-f277w_i2d.fits`	0.063″	1.00
F356W	`jw05398-c1207_t000_nircam_clear-f356w_i2d.fits`	0.063″	1.00
F410M	`jw01345-o002_t022_nircam_clear-f410m_i2d.fits`	0.063″	1.00
F444W	`jw01345-o002_t022_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 J141942.18+525644.4.

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.