LRD Watch DR1 · catalog object
LRDW J021658.32-051909.8
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.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 4.40 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 26.31 AB S/N 20, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.95 cliff_degraaff25; Δχ² galaxy 2.1, dwarf 27.9
- Compactness
- growth ratio 1.655 stars 2.245
- Balmer break
- 2.97 (lower limit) F277W/F150W, red:Hb+OIII+blue:far-uv+blue:2sig-limit
- Image vetting
- half-stack no-coverage; 1 flag(s)
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.040″
Vetting
- Image vettingnot applicable
- Half-stack testno-coverage
- Artifact riskflagged
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=2.1 dchi2_bd=27.9
- BH* channelartifact-risk low-coverage n_exp=2 < 3 (F356W)
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 | 4.3980 | bhstar:cliff_degraaff25 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 4.398 | cliff_degraaff25 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured at z_agn
- Line in F410M
- none 0 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.
- 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. |
|---|---|---|---|---|---|---|---|
| F090W | NIRCam wide | 0.902 | 0.02 | 10.50 | 35.50 | 0.0 | 1.14 |
| F115W | NIRCam wide | 1.154 | −2.84 | 10.57 | — | −0.3 | 1.12 |
| F150W | NIRCam wide | 1.501 | 6.40 | 8.31 | 29.39 | 0.8 | 1.10 |
| F200W | NIRCam wide | 1.989 | 3.88 | 6.78 | 29.93 | 0.6 | 1.09 |
| F277W | NIRCam wide | 2.762 | 49.41 | 4.05 | 27.16 | 12.2 | 1.20 |
| F356W | NIRCam wide | 3.568 | 105.17 | 4.06 | 26.34 | 25.9 | 1.24 |
| F410M | NIRCam medium | 4.082 | 110.59 | 7.31 | 26.29 | 15.1 | 1.26 |
| F444W | NIRCam wide | 4.404 | 108.37 | 5.37 | 26.31 | 20.2 | 1.28 |
Provenance
- Field
- UDS (PRIMER UDS-1) (
primeruds1) - Programmes
01837behind 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 |
|---|---|---|---|
| F090W | jw01837-c1002_t000_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01837-c1002_t000_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01837-c1002_t000_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01837-c1002_t000_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01837-c1002_t000_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01837-c1002_t000_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01837-c1002_t000_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01837-c1002_t000_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 J021658.32-051909.8.
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.