LRD Watch DR1 · catalog object
LRDW J033223.13-275111.0
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
- SILVER main class
- Found by
- colour lane
- Redshift
- 5.38 published
- Spectral shape
- no labelled spectrum
- F444W
- 27.43 AB S/N 50, 0.16″ aperture
- F277W − F444W
- 1.31 mag strict redness
- BH* share
- not in the BH* channel
- Compactness
- FWHM 0.156″
- Balmer break
- 1.10 ± 0.15 F250M/F210M, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- 5 catalogue(s), 0 AGN paper(s) within 0.012″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- No vetting notes.
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 | 5.3810 | zpub:simbad.csv:JADES-GS NC 184838 [2024ApJ...968...34W] |
z_phot | Photometric (P(z) peak) | 5.360 | 68%: 3.142–6.398 |
z_bhs | BH* channel fit | — | — |
z_agn | Colour-lane fit | 0.23 | AGN-inclusive templates |
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
- Ha 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.
- Barro et al. (2026)
- Kocevski et al. (2024)
- Pérez-González et al. (2024)
- Rinaldi et al. (2024)
- 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. |
|---|---|---|---|---|---|---|---|
| F070W | NIRCam wide | 0.704 | 0.33 | 1.50 | 32.60 | 0.2 | 1.36–1.38 |
| F090W | NIRCam wide | 0.902 | 5.12 | 0.95 | 29.63 | 5.4 | 1.34–1.40 |
| F115W | NIRCam wide | 1.154 | 6.37 | 0.87 | 29.39 | 7.3 | 1.34–1.39 |
| F150W | NIRCam wide | 1.501 | 6.29 | 0.82 | 29.40 | 7.7 | 1.30–1.41 |
| F162M | NIRCam medium | 1.627 | 9.00 | 1.03 | 29.02 | 8.7 | 1.37–1.38 |
| F182M | NIRCam medium | 1.845 | 8.61 | 0.64 | 29.06 | 13.5 | 1.36–1.37 |
| F200W | NIRCam wide | 1.989 | 7.39 | 0.84 | 29.23 | 8.8 | 1.34–1.39 |
| F210M | NIRCam medium | 2.095 | 7.95 | 0.80 | 29.15 | 9.9 | 1.39–1.40 |
| F250M | NIRCam medium | 2.504 | 8.68 | 0.81 | 29.05 | 10.7 | 1.46–1.47 |
| F277W | NIRCam wide | 2.762 | 11.58 | 0.49 | 28.74 | 23.4 | 1.46–1.50 |
| F300M | NIRCam medium | 2.990 | 13.64 | 0.56 | 28.56 | 24.3 | 1.50–1.51 |
| F335M | NIRCam medium | 3.362 | 17.80 | 0.53 | 28.27 | 33.7 | 1.50–1.55 |
| F356W | NIRCam wide | 3.568 | 18.59 | 0.51 | 28.23 | 36.3 | 1.52–1.56 |
| F410M | NIRCam medium | 4.082 | 60.46 | 0.83 | 26.95 | 73.0 | 1.52–1.59 |
| F444W | NIRCam wide | 4.404 | 38.64 | 0.77 | 27.43 | 50.0 | 1.55–1.62 |
| F1800W | MIRI | 17.970 | −22.20 | 101.82 | — | −0.2 | — |
| F2100W | MIRI | 20.801 | 119.04 | 189.13 | 26.21 | 0.6 | — |
| F2550W | MIRI | 25.230 | −352.13 | 960.13 | — | −0.4 | — |
Provenance
- Field
- GOODS-S (JADES Origins Field); GOODS-S (JADES Medium/HST F2); GOODS-S (JADES Medium/HST F3) (
deep,jw01180o026,jw01180o027) - Programmes
01180, 01207, 01210, 03215, 04540behind every mosaic the field measured- Pipeline rows merged
- 6 largest separation 0.024″
- 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 J033223.13-275111.0.
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.