LRD Watch DR1 · candidate
LRDW J100039.30+022253.0
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
- 2.51 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 23.12 AB S/N 459, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.81 bhs_bb5400_b4; Δχ² galaxy 10.9, dwarf 95.1
- Compactness
- growth ratio 2.249 stars 2.248
- Balmer break
- 2.54 ± 0.14 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 | 2.5130 | bhstar:bhs_bb5400_b4 (zpub 2.3 noted) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 2.513 | bhs_bb5400_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 | 70.59 | 6.23 | 26.78 | 11.3 | 1.15 |
| F115W | NIRCam wide | 1.154 | 189.79 | 6.39 | 25.70 | 29.7 | 1.13 |
| F140M | NIRCam medium | 1.405 | 482.94 | 22.11 | 24.69 | 21.8 | 1.11 |
| F150W | NIRCam wide | 1.501 | 661.64 | 6.20 | 24.35 | 106.7 | 1.11 |
| F200W | NIRCam wide | 1.989 | 1086.35 | 6.51 | 23.81 | 166.8 | 1.10 |
| F250M | NIRCam medium | 2.504 | 1319.88 | 20.48 | 23.60 | 64.4 | 1.18 |
| F277W | NIRCam wide | 2.762 | 1512.94 | 4.45 | 23.45 | 340.2 | 1.21 |
| F300M | NIRCam medium | 2.990 | 1602.25 | 8.40 | 23.39 | 190.7 | 1.23 |
| F356W | NIRCam wide | 3.568 | 1794.77 | 4.47 | 23.27 | 401.5 | 1.23 |
| F360M | NIRCam medium | 3.624 | 1762.67 | 16.49 | 23.29 | 106.9 | 1.25 |
| F410M | NIRCam medium | 4.082 | 1806.88 | 7.27 | 23.26 | 248.6 | 1.27 |
| F444W | NIRCam wide | 4.404 | 2042.09 | 4.45 | 23.12 | 459.4 | 1.28 |
| F460M | NIRCam medium | 4.630 | 1951.66 | 27.26 | 23.17 | 71.6 | 1.32 |
| F770W | MIRI | 7.636 | 1015.52 | 14.90 | 23.88 | 68.2 | 1.83 |
| F1280W | MIRI | 12.809 | 366.98 | 57.48 | 24.99 | 6.4 | — |
| F1500W | MIRI | 15.048 | 226.21 | 70.33 | 25.51 | 3.2 | — |
| F1800W | MIRI | 17.970 | 314.70 | 118.48 | 25.16 | 2.7 | — |
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 J100039.30+022253.0.
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.