LRD Watch DR1 · candidate
LRDW J100034.40+022019.0
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
- MIRI
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER z < 3 BH* class
- Found by
- BH* channel
- Redshift
- 2.62 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 24.10 AB S/N 228, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.81 bhs_bb4200_b4; Δχ² galaxy 27.2, dwarf 251.4
- Compactness
- growth ratio 2.080 stars 2.248
- Balmer break
- 3.45 ± 0.93 F140M/F115W, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- no published match within 1″
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 | — | — |
z_vet | Adopted by vetting | 2.6221 | bhstar:bhs_bb4200_b4 (zpub 2.82 noted) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 2.622 | bhs_bb4200_b4 |
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 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.
- No published JWST little red dot or broad-line AGN within 1″.
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 | 14.65 | 6.53 | 28.49 | 2.2 | 1.15 |
| F115W | NIRCam wide | 1.154 | 25.74 | 5.97 | 27.87 | 4.3 | 1.13 |
| F140M | NIRCam medium | 1.405 | 88.83 | 12.28 | 26.53 | 7.2 | 1.11 |
| F150W | NIRCam wide | 1.501 | 74.00 | 4.86 | 26.73 | 15.2 | 1.11 |
| F200W | NIRCam wide | 1.989 | 225.88 | 4.81 | 25.52 | 47.0 | 1.10 |
| F250M | NIRCam medium | 2.504 | 492.74 | 11.35 | 24.67 | 43.4 | 1.18 |
| F277W | NIRCam wide | 2.762 | 499.86 | 3.33 | 24.65 | 150.2 | 1.21 |
| F300M | NIRCam medium | 2.990 | 569.99 | 5.60 | 24.51 | 101.8 | 1.23 |
| F356W | NIRCam wide | 3.568 | 676.87 | 3.36 | 24.32 | 201.4 | 1.23 |
| F360M | NIRCam medium | 3.624 | 661.05 | 8.40 | 24.35 | 78.7 | 1.25 |
| F410M | NIRCam medium | 4.082 | 777.12 | 5.92 | 24.17 | 131.4 | 1.27 |
| F444W | NIRCam wide | 4.404 | 835.11 | 3.66 | 24.10 | 228.0 | 1.28 |
| F460M | NIRCam medium | 4.630 | 757.88 | 16.29 | 24.20 | 46.5 | 1.32 |
| F770W | MIRI | 7.636 | 757.00 | 14.74 | 24.20 | 51.3 | 1.83 |
| F1280W | MIRI | 12.809 | 350.03 | 56.54 | 25.04 | 6.2 | — |
| F1500W | MIRI | 15.048 | 300.70 | 68.50 | 25.20 | 4.4 | — |
| F1800W | MIRI | 17.970 | 310.90 | 117.16 | 25.17 | 2.6 | — |
Provenance
- Field
- COSMOS (PRIMER COSMOS-2) (
primercosmos2) - Programmes
01837, 02321, 07814behind 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-o004_t004_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01837-o004_t004_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01837-o004_t004_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01837-o004_t004_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01837-o004_t004_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01837-o004_t004_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01837-o004_t004_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01837-o004_t004_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 J100034.40+022019.0.
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.