LRD Watch DR1 · catalog object
LRDW J100030.19+022322.9
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
- SILVER main class
- Found by
- BH* channel + colour lane
- Redshift
- 7.029 DJA grade 3, PRISM
- Spectral shape
- not V-shaped de Graaff+25 criteria
- F444W
- 27.21 AB S/N 23, 0.16″ aperture
- F277W − F444W
- 1.18 mag strict redness
- BH* share
- 0.67 bhs_bb4800_b4; Δχ² galaxy 0.8, dwarf 0.8
- Compactness
- growth ratio 1.767 stars 2.250
- Balmer break
- 0.80 (lower limit) F360M/F250M, blue:2sig-limit
- Image vetting
- half-stack pass; 1 flag(s)
- Literature
- 2 catalogue(s), 1 AGN paper(s) within 0.009″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact riskflagged
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=0.8 dchi2_bd=0.8
- BH* channelBH* share 0.67 below 0.8 (composite)
- BH* channelartifact-risk low-coverage n_exp=2 < 3 (F444W)
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 | 7.0290 | cosmos-transients-v4_prism-clear_6585_66964.spec.fits |
z_vet | Adopted by vetting | 7.0290 | zspec:dja:cosmos-transients-v4_prism-clear_6585_66964.spec.fits (pipeline z_vet 7.03 from zspec:dja_specz_grade3.csv:16252) |
z_phot | Photometric (P(z) peak) | 7.085 | 68%: 5.275–7.351 |
z_bhs | BH* channel fit | 7.093 | bhs_bb4800_b4 |
z_agn | Colour-lane fit | 5.36 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- not V-shaped
- Star (spectrum)
- no
- V-shape (photometry)
- passes βUV −1.48, βopt 0.57 at z_agn
- Line in F410M
- Hb, OIII 2 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)
- Kocevski et al. (2024)
- Akins+2025 (COS-66964) broad-line AGN
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 | 6.67 | 5.05 | 29.34 | 1.3 | 1.15–1.15 |
| F115W | NIRCam wide | 1.154 | 11.95 | 5.16 | 28.71 | 2.3 | 1.12–1.13 |
| F140M | NIRCam medium | 1.405 | 30.38 | 31.88 | 27.69 | 0.9 | 1.11 |
| F150W | NIRCam wide | 1.501 | 13.71 | 3.68 | 28.56 | 3.7 | 1.11–1.11 |
| F200W | NIRCam wide | 1.989 | 13.83 | 3.17 | 28.55 | 4.4 | 1.09–1.11 |
| F212N | NIRCam wide | 2.121 | −0.94 | 28.65 | — | −0.0 | 1.12–1.14 |
| F250M | NIRCam medium | 2.504 | 10.10 | 11.38 | 28.89 | 0.9 | 1.18 |
| F277W | NIRCam wide | 2.762 | 16.01 | 1.69 | 28.39 | 9.5 | 1.20–1.21 |
| F300M | NIRCam medium | 2.990 | 26.07 | 3.38 | 27.86 | 7.7 | 1.22–1.23 |
| F356W | NIRCam wide | 3.568 | 24.43 | 1.55 | 27.93 | 15.7 | 1.23–1.24 |
| F360M | NIRCam medium | 3.624 | 17.84 | 7.51 | 28.27 | 2.4 | 1.24–1.25 |
| F410M | NIRCam medium | 4.082 | 67.60 | 3.09 | 26.82 | 21.9 | 1.26–1.27 |
| F444W | NIRCam wide | 4.404 | 47.28 | 2.02 | 27.21 | 23.4 | 1.27–1.28 |
| F460M | NIRCam medium | 4.630 | 37.86 | 17.44 | 27.45 | 2.2 | 1.32 |
Provenance
- Field
- COSMOS (PRIMER); COSMOS (PRIMER COSMOS-2) (
cosmos,primercosmos2) - Programmes
01837, 02321, 07814behind every mosaic the field measured- Pipeline rows merged
- 5 largest separation 0.061″
- 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 J100030.19+022322.9.
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.