LRD Watch DR1 · candidate
LRDW J100035.34+021933.0
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
- 2.831 DJA grade 3, PRISM
- Spectral shape
- not V-shaped de Graaff+25 criteria
- F444W
- 22.82 AB S/N 546, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.82 bhs_bb4200_b8; Δχ² galaxy 63.9, dwarf 131.0
- Compactness
- growth ratio 2.299 stars 2.248
- Balmer break
- 7.37 ± 0.15 F200W/F115W, red:Hb+OIII
- 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 | 2.8309 | gto-wide-cos03-v4_prism-clear_1214_2001.spec.fits |
z_vet | Adopted by vetting | 2.8309 | zspec:dja:gto-wide-cos03-v4_prism-clear_1214_2001.spec.fits (pipeline z_vet 2.836 from zspec:vizier_J_A+A_691_A240_primercp.csv:61878) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 2.044 | bhs_bb4200_b8 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- not V-shaped
- Star (spectrum)
- no
- 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.
- 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 | 98.40 | 5.35 | 26.42 | 18.4 | 1.15–1.15 |
| F115W | NIRCam wide | 1.154 | 263.71 | 5.36 | 25.35 | 49.2 | 1.12–1.13 |
| F140M | NIRCam medium | 1.405 | 567.10 | 14.09 | 24.52 | 40.2 | 1.11 |
| F150W | NIRCam wide | 1.501 | 970.77 | 5.76 | 23.93 | 168.6 | 1.11–1.11 |
| F200W | NIRCam wide | 1.989 | 1944.23 | 6.83 | 23.18 | 284.7 | 1.09–1.11 |
| F212N | NIRCam wide | 2.121 | 2095.85 | 34.43 | 23.10 | 60.9 | 1.12–1.14 |
| F250M | NIRCam medium | 2.504 | 2141.98 | 16.03 | 23.07 | 133.6 | 1.18 |
| F277W | NIRCam wide | 2.762 | 2258.65 | 5.22 | 23.02 | 432.4 | 1.20–1.21 |
| F300M | NIRCam medium | 2.990 | 2345.02 | 9.82 | 22.98 | 238.9 | 1.22–1.23 |
| F356W | NIRCam wide | 3.568 | 2481.08 | 5.21 | 22.91 | 476.1 | 1.23–1.24 |
| F360M | NIRCam medium | 3.624 | 2434.49 | 12.14 | 22.93 | 200.5 | 1.24–1.25 |
| F410M | NIRCam medium | 4.082 | 2546.74 | 8.24 | 22.89 | 309.1 | 1.26–1.27 |
| F444W | NIRCam wide | 4.404 | 2700.25 | 4.95 | 22.82 | 545.8 | 1.27–1.28 |
| F460M | NIRCam medium | 4.630 | 2708.85 | 19.98 | 22.82 | 135.6 | 1.32 |
| F770W | MIRI | 7.636 | 1566.36 | 14.79 | 23.41 | 105.9 | 1.83 |
| F1280W | MIRI | 12.809 | 674.42 | 68.44 | 24.33 | 9.8 | — |
| F1500W | MIRI | 15.048 | 448.64 | 82.77 | 24.77 | 5.4 | 4.24 |
| F1800W | MIRI | 17.970 | 118.76 | 115.95 | 26.21 | 1.0 | — |
Provenance
- Field
- COSMOS (PRIMER); COSMOS (PRIMER COSMOS-2) (
cosmos,primercosmos2) - Programmes
01837, 02321, 07814behind every mosaic the field measured- Pipeline rows merged
- 2 largest separation 0.038″
- 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 | jw02321-o002_t001_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 J100035.34+021933.0.
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.