LRD Watch DR1 · catalog object
LRDW J100034.66+022039.8
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
- MIRI
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER main class
- Found by
- BH* channel + colour lane
- Redshift
- 3.926 DJA grade 3, PRISM
- Spectral shape
- V-shaped de Graaff+25 criteria
- F444W
- 24.58 AB S/N 164, 0.16″ aperture
- F277W − F444W
- 0.52 mag inclusive redness
- BH* share
- 0.87 bhs_bb5400_b8; Δχ² galaxy 45.6, dwarf 152.8
- Compactness
- growth ratio 1.891 stars 2.248
- Balmer break
- 5.86 ± 0.41 F250M/F150W, red:Hb+OIII
- Image vetting
- half-stack pass; no flags raised
- Literature
- 6 catalogue(s), 0 AGN paper(s) within 0.005″
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 | 3.9263 | cosmos-transients-v4_prism-clear_6585_58018.spec.fits |
z_vet | Adopted by vetting | 3.9263 | zspec:dja_specz_grade3.csv:58018 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 4.045 | bhs_bb5400_b8 |
z_agn | Colour-lane fit | 1.64 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- V-shaped
- Star (spectrum)
- no
- V-shape (photometry)
- not measurable βUV not measured, βopt −2.00 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.
- Barro et al. (2025)
- Barro et al. (2026)
- de Graaff et al. (2025)
- Kocevski et al. (2024)
- Kokorev et al. (2024)
- Leung et al. (2024)
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 | 89.50 | 7.68 | 26.52 | 11.7 | 1.15–1.15 |
| F115W | NIRCam wide | 1.154 | 74.45 | 7.07 | 26.72 | 10.5 | 1.12–1.13 |
| F140M | NIRCam medium | 1.405 | 58.35 | 10.69 | 26.98 | 5.5 | 1.11 |
| F150W | NIRCam wide | 1.501 | 81.82 | 5.52 | 26.62 | 14.8 | 1.11–1.11 |
| F200W | NIRCam wide | 1.989 | 127.82 | 5.00 | 26.13 | 25.6 | 1.09–1.11 |
| F250M | NIRCam medium | 2.504 | 480.64 | 9.00 | 24.70 | 53.4 | 1.18 |
| F277W | NIRCam wide | 2.762 | 333.37 | 2.93 | 25.09 | 113.9 | 1.20–1.21 |
| F300M | NIRCam medium | 2.990 | 340.77 | 4.83 | 25.07 | 70.6 | 1.22–1.23 |
| F356W | NIRCam wide | 3.568 | 570.60 | 3.21 | 24.51 | 177.6 | 1.23–1.24 |
| F360M | NIRCam medium | 3.624 | 458.05 | 6.02 | 24.75 | 76.1 | 1.24–1.25 |
| F410M | NIRCam medium | 4.082 | 467.86 | 5.06 | 24.73 | 92.4 | 1.26–1.27 |
| F444W | NIRCam wide | 4.404 | 536.00 | 3.27 | 24.58 | 164.1 | 1.27–1.28 |
| F460M | NIRCam medium | 4.630 | 590.38 | 12.22 | 24.47 | 48.3 | 1.32 |
| F770W | MIRI | 7.636 | 259.13 | 14.57 | 25.37 | 17.8 | 1.83 |
| F1280W | MIRI | 12.809 | 217.82 | 57.52 | 25.55 | 3.8 | — |
| F1500W | MIRI | 15.048 | 192.01 | 70.03 | 25.69 | 2.7 | 4.24 |
| F1800W | MIRI | 17.970 | 125.58 | 118.25 | 26.15 | 1.1 | — |
Provenance
- Field
- COSMOS (PRIMER); COSMOS (PRIMER COSMOS-2) (
cosmos,primercosmos2) - Programmes
01837, 02321, 07814behind every mosaic the field measured- Pipeline rows merged
- 6 largest separation 0.033″
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F090W | jw01837-o003_t003_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01837-o003_t003_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01837-o003_t003_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 J100034.66+022039.8.
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.