LRD Watch DR1 · catalog object
LRDW J100036.74+023249.7
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
- 25.89 AB S/N 67, 0.16″ aperture
- F277W − F444W
- 1.59 mag strict redness
- BH* share
- 0.76 bhs_bb4200_b4; Δχ² galaxy 4.1, dwarf 29.4
- Compactness
- growth ratio 1.741 stars 2.325
- Balmer break
- 3.73 ± 0.40 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 0.026″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=4.1 dchi2_bd=29.4
- BH* channelBH* share 0.76 below 0.8 (composite)
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%: 3.175–7.581 |
z_bhs | BH* channel fit | 6.252 | bhs_bb4200_b4 |
z_agn | Colour-lane fit | 2.42 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt −2.13 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 | 18.82 | 3.23 | 28.21 | 5.8 | 1.29 |
| F150W | NIRCam wide | 1.501 | 22.33 | 2.78 | 28.03 | 8.0 | 1.30 |
| F200W | NIRCam wide | 1.989 | 21.55 | 2.27 | 28.07 | 9.5 | 1.32 |
| F277W | NIRCam wide | 2.762 | 36.99 | 1.92 | 27.48 | 19.2 | 1.46 |
| F356W | NIRCam wide | 3.568 | 80.07 | 1.85 | 26.64 | 43.3 | 1.52 |
| F444W | NIRCam wide | 4.404 | 159.60 | 2.38 | 25.89 | 67.0 | 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 J100036.74+023249.7.
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.