LRD Watch DR1 · catalog object
LRDW J100044.63+023451.7
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. No coverage in F090W, F410M.
Spectral energy distribution
- NIRCam wide
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER main class
- Found by
- BH* channel + colour lane
- Redshift
- 7.08 photometric
- Spectral shape
- no labelled spectrum
- F444W
- 25.50 AB S/N 100, 0.16″ aperture
- F277W − F444W
- 1.55 mag strict redness
- BH* share
- 0.82 bhs_bb4800_b4; Δχ² galaxy 2.0, dwarf 28.6
- Compactness
- growth ratio 1.932 stars 2.325
- Balmer break
- 3.56 ± 0.23 F356W/F200W, red:Hb+OIII+blue:far-uv
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.074″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=2.0 dchi2_bd=28.6
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 | 7.0850 | pz:z_map |
z_phot | Photometric (P(z) peak) | 7.085 | 68%: 6.833–7.178 |
z_bhs | BH* channel fit | 6.452 | bhs_bb4800_b4 |
z_agn | Colour-lane fit | 5.62 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- passes βUV −2.83, βopt 1.10 at z_agn
- Line in F410M
- Hb, OIII 0 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- no extraction
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- Akins 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. |
|---|---|---|---|---|---|---|---|
| F115W | NIRCam wide | 1.154 | 45.11 | 3.46 | 27.26 | 13.0 | 1.29 |
| F150W | NIRCam wide | 1.501 | 36.29 | 2.86 | 27.50 | 12.7 | 1.30 |
| F200W | NIRCam wide | 1.989 | 38.29 | 2.36 | 27.44 | 16.2 | 1.32 |
| F277W | NIRCam wide | 2.762 | 54.94 | 1.84 | 27.05 | 29.9 | 1.46 |
| F356W | NIRCam wide | 3.568 | 136.95 | 1.85 | 26.06 | 73.9 | 1.52 |
| F444W | NIRCam wide | 4.404 | 228.71 | 2.30 | 25.50 | 99.7 | 1.58 |
Provenance
- Field
- COSMOS (CAPERS P7) (
jw06368o019) - Programmes
06368behind every mosaic the field measured- Pipeline rows merged
- 3 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | jw06368-o019_t057_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw06368-o019_t057_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw06368-o019_t057_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw06368-o019_t057_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw06368-o019_t057_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F444W | jw06368-o019_t057_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 J100044.63+023451.7.
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.