LRD Watch DR1 · catalog object
LRDW J123710.33+621937.9
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, F115W, F356W.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER main class
- Found by
- BH* channel + colour lane
- Redshift
- 5.49 colour-lane fit
- Spectral shape
- no labelled spectrum
- F444W
- 25.72 AB S/N 139, 0.16″ aperture
- F277W − F444W
- 1.81 mag strict redness
- BH* share
- 0.84 bhs_bb4800_b4; Δχ² galaxy 14.9, dwarf 4.3
- Compactness
- growth ratio 1.847 stars 2.426
- Balmer break
- 1.21 ± 0.04 F277W/F200W, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.046″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=14.9 dchi2_bd=4.3
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 | — | — |
z_vet | Adopted by vetting | 5.4900 | z_agn |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 7.386 | bhs_bb4800_b4 |
z_agn | Colour-lane fit | 5.49 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt 2.70 at z_agn
- Line in F410M
- Ha 1 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- inconclusive
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- Weibel et al. (2026), BH*-dominated sample
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. |
|---|---|---|---|---|---|---|---|
| F162M | NIRCam medium | 1.627 | 30.94 | 1.42 | 27.67 | 21.7 | 1.28–1.33 |
| F200W | NIRCam wide | 1.989 | 29.10 | 0.69 | 27.74 | 42.2 | 1.26–1.34 |
| F277W | NIRCam wide | 2.762 | 35.27 | 0.80 | 27.53 | 43.9 | 1.42–1.49 |
| F410M | NIRCam medium | 4.082 | 214.50 | 1.95 | 25.57 | 110.2 | 1.47–1.55 |
| F444W | NIRCam wide | 4.404 | 187.12 | 1.35 | 25.72 | 139.0 | 1.51–1.61 |
Provenance
- Field
- GOODS-N (GTO 1264 NIRCam parallel); GOODS-N (JADES 1181 with FRESCO, CONGRESS, GO 4762 and GO 6434) (
gnz11,goods) - Programmes
01181, 01264, 01895, 02674, 02926, 03577, 04762, 05407, 06434behind every mosaic the field measured- Pipeline rows merged
- 6 largest separation 0.048″
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F150W | jw01181-o011_t009_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw06434-c1035_t000_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw06434-c1035_t000_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01181-o011_t009_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01181-o011_t009_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 J123710.33+621937.9.
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.