LRD Watch DR1 · catalog object
LRDW J033221.53-275042.7
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.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- MIRI
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 4.78 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 25.65 AB S/N 290, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.67 cliff_degraaff25; Δχ² galaxy 9.2, dwarf 295.7
- Compactness
- growth ratio 2.051 stars 2.383
- Balmer break
- 1.91 ± 0.03 F250M/F182M, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.010″
Vetting
- Image vettingnot applicable
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelBH* share 0.67 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 | 4.7832 | bhstar:cliff_degraaff25 (zpub 4.7418 noted) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 4.783 | 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 2 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.
- Barro et al. (2026)
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. |
|---|---|---|---|---|---|---|---|
| F070W | NIRCam wide | 0.704 | 31.43 | 1.57 | 27.66 | 20.0 | 1.36–1.38 |
| F090W | NIRCam wide | 0.902 | 47.89 | 1.06 | 27.20 | 45.3 | 1.34–1.42 |
| F115W | NIRCam wide | 1.154 | 44.84 | 0.93 | 27.27 | 48.2 | 1.34–1.38 |
| F150W | NIRCam wide | 1.501 | 51.09 | 0.90 | 27.13 | 56.9 | 1.30–1.41 |
| F162M | NIRCam medium | 1.627 | 48.80 | 1.13 | 27.18 | 43.2 | 1.37–1.38 |
| F182M | NIRCam medium | 1.845 | 49.60 | 0.70 | 27.16 | 70.7 | 1.36–1.37 |
| F200W | NIRCam wide | 1.989 | 54.18 | 0.95 | 27.07 | 57.1 | 1.34–1.40 |
| F210M | NIRCam medium | 2.095 | 53.81 | 0.90 | 27.07 | 59.6 | 1.39–1.40 |
| F250M | NIRCam medium | 2.504 | 94.57 | 0.93 | 26.46 | 101.8 | 1.46–1.47 |
| F277W | NIRCam wide | 2.762 | 159.40 | 0.65 | 25.89 | 244.4 | 1.46–1.51 |
| F300M | NIRCam medium | 2.990 | 209.11 | 0.79 | 25.60 | 263.3 | 1.50–1.51 |
| F335M | NIRCam medium | 3.362 | 152.35 | 0.68 | 25.94 | 222.9 | 1.50–1.55 |
| F356W | NIRCam wide | 3.568 | 228.68 | 0.74 | 25.50 | 308.8 | 1.52–1.56 |
| F410M | NIRCam medium | 4.082 | 194.82 | 0.98 | 25.68 | 198.8 | 1.52–1.59 |
| F444W | NIRCam wide | 4.404 | 200.31 | 0.69 | 25.65 | 289.5 | 1.55–1.62 |
| F1800W | MIRI | 17.970 | 95.21 | 102.46 | 26.45 | 0.9 | — |
| F2100W | MIRI | 20.801 | 208.65 | 191.66 | 25.60 | 1.1 | — |
| F2550W | MIRI | 25.230 | 395.41 | 960.65 | 24.91 | 0.4 | — |
Provenance
- Field
- GOODS-S (JADES Origins Field); GOODS-S (JADES Medium/HST F2); GOODS-S (JADES Medium/HST F4) (
deep,jw01180o026,jw01180o028) - Programmes
01180, 01207, 01210, 03215, 04540behind every mosaic the field measured- Pipeline rows merged
- 3 largest separation 0.059″
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F090W | jw01210-o001_t002_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01210-o001_t002_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01210-o001_t002_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01210-o001_t002_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01210-o001_t002_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01210-o001_t002_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01210-o001_t002_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01210-o001_t002_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 J033221.53-275042.7.
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.