LRD Watch DR1 · catalog object
LRDW J010403.05-550856.4
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
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 8.02 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 25.67 AB S/N 46, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.69 cliff_degraaff25; Δχ² galaxy 3.6, dwarf 5.7
- Compactness
- growth ratio 1.822 stars 2.156
- Balmer break
- 6.05 ± 0.75 F444W/F277W, red:Hb+OIII
- Image vetting
- half-stack no-coverage; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.005″
Vetting
- Image vettingnot applicable
- Half-stack testno-coverage
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=3.6 dchi2_bd=5.7
- BH* channelBH* share 0.69 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 | 8.0220 | bhstar:cliff_degraaff25 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 8.022 | cliff_degraaff25 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured at z_agn
- Line in F410M
- none 0 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.
- Weibel et al. (2026), BH*-dominated sample
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 | 17.39 | 13.55 | 28.30 | 1.3 | 1.16 |
| F150W | NIRCam wide | 1.501 | 30.03 | 10.28 | 27.71 | 2.9 | 1.23 |
| F200W | NIRCam wide | 1.989 | 19.39 | 8.90 | 28.18 | 2.2 | 1.27 |
| F277W | NIRCam wide | 2.762 | 32.43 | 3.96 | 27.62 | 8.2 | 1.38 |
| F356W | NIRCam wide | 3.568 | 79.94 | 3.50 | 26.64 | 22.9 | 1.41 |
| F444W | NIRCam wide | 4.404 | 196.26 | 4.24 | 25.67 | 46.3 | 1.45 |
Provenance
- Field
- PANORAMIC J010408-5508 (
panoramicj010408m5508) - Programmes
02514behind every mosaic the field measured- Pipeline rows merged
- 1 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | panoramic-j010408m5508-grizli-v7.2-f115w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F150W | panoramic-j010408m5508-grizli-v7.2-f150w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F200W | panoramic-j010408m5508-grizli-v7.2-f200w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F277W | panoramic-j010408m5508-grizli-v7.2-f277w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F356W | panoramic-j010408m5508-grizli-v7.2-f356w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F444W | panoramic-j010408m5508-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 J010403.05-550856.4.
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.