LRD Watch DR1 · catalog object
LRDW J033223.10-275404.1
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
- SILVER main class
- Found by
- colour lane
- Redshift
- 7.93 photometric
- Spectral shape
- no labelled spectrum
- F444W
- 27.97 AB S/N 19, 0.16″ aperture
- F277W − F444W
- 1.06 mag strict redness
- BH* share
- not in the BH* channel
- Compactness
- FWHM 0.169″
- Balmer break
- 1.38 ± 0.30 F410M/F277W, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.015″
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 | 7.9350 | pz:z_map |
z_phot | Photometric (P(z) peak) | 7.935 | 68%: 7.792–8.549 |
z_bhs | BH* channel fit | — | — |
z_agn | Colour-lane fit | 7.93 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- passes βUV −2.04, βopt 6.50 at z_agn
- Line in F410M
- none 1 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.
- 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. |
|---|---|---|---|---|---|---|---|
| F090W | NIRCam wide | 0.902 | −2.15 | 3.19 | — | −0.7 | 1.31–1.39 |
| F115W | NIRCam wide | 1.154 | 7.68 | 2.62 | 29.19 | 2.9 | 1.37–1.40 |
| F150W | NIRCam wide | 1.501 | 11.02 | 2.58 | 28.80 | 4.3 | 1.36–1.36 |
| F200W | NIRCam wide | 1.989 | 10.90 | 2.17 | 28.81 | 5.0 | 1.37–1.38 |
| F277W | NIRCam wide | 2.762 | 8.88 | 1.23 | 29.03 | 7.2 | 1.38–1.50 |
| F356W | NIRCam wide | 3.568 | 12.04 | 1.07 | 28.70 | 11.3 | 1.50–1.55 |
| F410M | NIRCam medium | 4.082 | 12.25 | 2.02 | 28.68 | 6.1 | 1.50–1.57 |
| F444W | NIRCam wide | 4.404 | 23.64 | 1.24 | 27.97 | 19.0 | 1.58–1.59 |
Provenance
- Field
- GOODS-S (JADES Medium/HST F5); GOODS-S (JADES Medium/HST F6) (
jw01180o029,jw01180o030) - Programmes
01180, 01207behind every mosaic the field measured- Pipeline rows merged
- 4 largest separation 0.026″
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F090W | jw01180-o029_t028_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01180-o029_t028_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01180-o029_t028_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01180-o029_t028_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01180-o029_t028_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01180-o029_t028_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01180-o029_t028_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01180-o029_t028_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 J033223.10-275404.1.
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.