LRD Watch DR1 · catalog object
LRDW J033258.35-275143.3
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
- 7.09 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 26.34 AB S/N 131, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.81 bhs_bb4200_b4; Δχ² galaxy 11.2, dwarf 23.9
- Compactness
- growth ratio 1.985 stars 2.235
- Balmer break
- 3.75 ± 0.20 F356W/F200W, red:Hb+OIII+blue:far-uv
- Image vetting
- half-stack fail; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.019″
Vetting
- Image vettingnot applicable
- Half-stack testfail
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelhalfstack-inconsistent F444W (h1 0.35σ / h2 -2.3σ)
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 | 7.0920 | bhstar:bhs_bb4200_b4 |
z_phot | Photometric (P(z) peak) | 5.234 | 68%: 4.890–5.818 |
z_bhs | BH* channel fit | 7.092 | bhs_bb4200_b4 |
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
- Hb, OIII 0 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- not evaluated
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- Kocevski 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 | 17.42 | 0.68 | 28.30 | 25.6 | 1.30 |
| F150W | NIRCam wide | 1.501 | 16.18 | 0.79 | 28.38 | 20.4 | 1.30 |
| F200W | NIRCam wide | 1.989 | 15.19 | 0.79 | 28.45 | 19.2 | 1.30 |
| F277W | NIRCam wide | 2.762 | 19.53 | 0.42 | 28.17 | 46.3 | 1.42 |
| F356W | NIRCam wide | 3.568 | 56.96 | 0.47 | 27.01 | 121.5 | 1.48 |
| F444W | NIRCam wide | 4.404 | 105.59 | 0.80 | 26.34 | 131.2 | 1.53 |
Provenance
- Field
- GOODS-S (NGDEEP) (
ngdeep) - Programmes
01180, 01283, 02079, 02198behind 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 | ngdeep-grizli-v7.2-f115w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F150W | ngdeep-grizli-v7.2-f150w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F200W | ngdeep-grizli-v7.2-f200w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F277W | ngdeep-grizli-v7.2-f277w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F356W | ngdeep-grizli-v7.2-f356w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F444W | ngdeep-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 J033258.35-275143.3.
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.