LRD Watch DR1 · catalog object
LRDW J033208.97-275156.1
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
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 4.95 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 24.82 AB S/N 582, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.78 cliff_degraaff25; Δχ² galaxy 11.3, dwarf 303.3
- Compactness
- growth ratio 1.879 stars 2.414
- Balmer break
- 1.94 ± 0.03 F250M/F210M, 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 0.78 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 | 4.9475 | bhstar:cliff_degraaff25 (zpub 5.35 noted) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 4.947 | 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
- Ha 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.
- Rinaldi 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. |
|---|---|---|---|---|---|---|---|
| F070W | NIRCam wide | 0.704 | 16.89 | 1.94 | 28.33 | 8.7 | 1.36–1.43 |
| F090W | NIRCam wide | 0.902 | 57.65 | 1.44 | 27.00 | 40.0 | 1.34–1.41 |
| F115W | NIRCam wide | 1.154 | 42.07 | 0.91 | 27.34 | 46.4 | 1.34–1.38 |
| F150W | NIRCam wide | 1.501 | 49.03 | 0.88 | 27.17 | 55.6 | 1.30–1.38 |
| F162M | NIRCam medium | 1.627 | 51.01 | 1.14 | 27.13 | 44.9 | 1.37–1.38 |
| F182M | NIRCam medium | 1.845 | 51.70 | 0.69 | 27.12 | 75.0 | 1.36–1.37 |
| F200W | NIRCam wide | 1.989 | 56.06 | 0.85 | 27.03 | 65.7 | 1.34–1.37 |
| F210M | NIRCam medium | 2.095 | 57.21 | 0.87 | 27.01 | 65.8 | 1.39–1.40 |
| F250M | NIRCam medium | 2.504 | 111.22 | 0.96 | 26.29 | 115.9 | 1.46–1.47 |
| F277W | NIRCam wide | 2.762 | 200.62 | 0.64 | 25.64 | 315.8 | 1.46–1.49 |
| F300M | NIRCam medium | 2.990 | 317.03 | 0.87 | 25.15 | 364.2 | 1.50–1.51 |
| F335M | NIRCam medium | 3.362 | 232.09 | 0.82 | 25.49 | 281.9 | 1.50–1.55 |
| F356W | NIRCam wide | 3.568 | 432.67 | 0.86 | 24.81 | 504.6 | 1.52–1.56 |
| F410M | NIRCam medium | 4.082 | 425.51 | 1.19 | 24.83 | 356.2 | 1.52–1.59 |
| F444W | NIRCam wide | 4.404 | 429.47 | 0.74 | 24.82 | 581.9 | 1.55–1.62 |
Provenance
- Field
- GOODS-S (JADES Origins Field); GOODS-S (JADES Medium/HST F1); GOODS-S (JADES Medium/HST F2); GOODS-S (JADES Medium/HST F1, GO 4549 pointing 2) (
deep,gs,jw01180o026,pointingx) - Programmes
01180, 01207, 01210, 01963, 03215, 04540, 04549behind every mosaic the field measured- Pipeline rows merged
- 4 largest separation 0.061″
- 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″ | 0.94 |
| F356W | jw01210-o001_t002_nircam_clear-f356w_i2d.fits | 0.063″ | 0.94 |
| F410M | jw01210-o001_t002_nircam_clear-f410m_i2d.fits | 0.063″ | 0.94 |
| F444W | jw01210-o001_t002_nircam_clear-f444w_i2d.fits | 0.063″ | 0.94 |
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 J033208.97-275156.1.
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.