LRD Watch DR1 · candidate
LRDW J100020.70+020652.2
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
- 5.36 photometric
- Spectral shape
- no labelled spectrum
- F444W
- 26.07 AB S/N 50, 0.16″ aperture
- F277W − F444W
- 1.13 mag strict redness
- BH* share
- 0.66 cliff_degraaff25; Δχ² galaxy 0.0, dwarf 40.6
- Compactness
- growth ratio 1.643 stars 2.036
- Balmer break
- 2.73 ± 0.73 F277W/F200W, 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
- BH* channelevidence dchi2_gal=0.0 dchi2_bd=40.6
- BH* channelBH* share 0.66 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 | 5.3600 | pz:z_map |
z_phot | Photometric (P(z) peak) | 5.360 | 68%: 2.477–6.388 |
z_bhs | BH* channel fit | 5.372 | cliff_degraaff25 |
z_agn | Colour-lane fit | 5.36 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- passes βUV −1.00, βopt 0.40 at z_agn
- Line in F410M
- Ha 0 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- inconclusive
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. |
|---|---|---|---|---|---|---|---|
| F115W | NIRCam wide | 1.154 | 10.39 | 4.89 | 28.86 | 2.1 | 1.31 |
| F150W | NIRCam wide | 1.501 | 13.52 | 4.50 | 28.57 | 3.0 | 1.33 |
| F200W | NIRCam wide | 1.989 | 17.58 | 4.59 | 28.29 | 3.8 | 1.36 |
| F277W | NIRCam wide | 2.762 | 47.93 | 2.65 | 27.20 | 18.1 | 1.43 |
| F356W | NIRCam wide | 3.568 | 86.45 | 2.83 | 26.56 | 30.5 | 1.49 |
| F444W | NIRCam wide | 4.404 | 135.65 | 2.73 | 26.07 | 49.6 | 1.52 |
Provenance
- Field
- PANORAMIC J100024+0208 (
panoramicj100024p0208) - Programmes
02514behind 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 | panoramic-j100024p0208-grizli-v7.2-f115w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F150W | panoramic-j100024p0208-grizli-v7.2-f150w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F200W | panoramic-j100024p0208-grizli-v7.2-f200w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F277W | panoramic-j100024p0208-grizli-v7.2-f277w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F356W | panoramic-j100024p0208-grizli-v7.2-f356w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F444W | panoramic-j100024p0208-grizli-v7.2-f444w-clear_drc_sci.fits | 0.040″ | 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 J100020.70+020652.2.
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.