LRD Watch DR1 · catalog object
LRDW J141935.92+524846.2
Images





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, F277W, F356W.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 5.002 DJA grade 3, PRISM
- Spectral shape
- V-shaped de Graaff+25 criteria
- F444W
- 25.95 AB S/N 85, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.81 bhs_bb5400_b4; Δχ² galaxy 2.3, dwarf −0.5
- Compactness
- growth ratio 1.627 stars 2.352
- Balmer break
- not measured
- Image vetting
- half-stack pass; no flags raised
- Literature
- 3 catalogue(s), 1 AGN paper(s) within 0.017″
Vetting
- Image vettingnot applicable
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channeldwarf grid fits better (dchi2_bd=-0.5) but z_spec confirms
- BH* channelevidence dchi2_gal=2.3 dchi2_bd=-0.5
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 | 5.0019 | capers-egs61-v4_prism-clear_6368_23961.spec.fits |
z_vet | Adopted by vetting | 5.0019 | zspec:dja_specz_grade3.csv:23961 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 5.010 | bhs_bb5400_b4 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- V-shaped
- Star (spectrum)
- no
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured at z_agn
- Line in F410M
- Ha 0 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- not evaluated
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- de Graaff et al. (2025)
- Kokorev et al. (2024)
- Weibel et al. (2026), BH*-dominated sample
- 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 | 5.59 | 3.66 | 29.53 | 1.5 | 1.40 |
| F150W | NIRCam wide | 1.501 | 1.89 | 3.14 | 30.71 | 0.6 | 1.43 |
| F200W | NIRCam wide | 1.989 | 9.38 | 2.66 | 28.97 | 3.5 | 1.42 |
| F410M | NIRCam medium | 4.082 | 199.02 | 3.73 | 25.65 | 53.3 | 1.56 |
| F430M | NIRCam medium | 4.281 | 133.80 | 6.60 | 26.08 | 20.3 | 1.63 |
| F444W | NIRCam wide | 4.404 | 151.91 | 1.79 | 25.95 | 84.8 | 1.60 |
Provenance
- Field
- EGS (CEERS NIRSpec P9) (
ceersnirspecp9mrmsata) - Programmes
01345, 08559behind every mosaic the field measured- Pipeline rows merged
- 1 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | jw01345-o069_t046_nircam_clear-f115w_i2d.fits | 0.031″ | 0.87 |
| F150W | jw01345-o069_t046_nircam_clear-f150w_i2d.fits | 0.031″ | 0.87 |
| F200W | jw01345-o069_t046_nircam_clear-f200w_i2d.fits | 0.031″ | 0.85 |
| F410M | jw01345-o069_t046_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01345-o069_t046_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 J141935.92+524846.2.
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.