LRD Watch DR1 · catalog object
LRDW J021754.73-051007.3
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.
Spectral energy distribution
- NIRCam wide
- NIRCam medium
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER main class
- Found by
- BH* channel + colour lane
- Redshift
- 6.047 DJA grade 3, PRISM
- Spectral shape
- not V-shaped de Graaff+25 criteria
- F444W
- 27.12 AB S/N 16, 0.16″ aperture
- F277W − F444W
- 1.03 mag strict redness
- BH* share
- 0.61 bhs_bb4200_b4; Δχ² galaxy 1.6, dwarf 5.5
- Compactness
- growth ratio 1.635 stars 2.271
- Balmer break
- 2.03 ± 0.51 F356W/F200W, red:Hb+OIII
- Image vetting
- half-stack pass; no flags raised
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.100″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- BH* channelevidence dchi2_gal=1.6 dchi2_bd=5.5
- BH* channelBH* share 0.61 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 | 6.0467 | rubies-uds32-v4_prism-clear_4233_125917.spec.fits |
z_vet | Adopted by vetting | 6.0467 | zspec:dja_specz_grade3.csv:125917 |
z_phot | Photometric (P(z) peak) | 5.619 | 68%: 2.410–6.116 |
z_bhs | BH* channel fit | 5.878 | bhs_bb4200_b4 |
z_agn | Colour-lane fit | 5.62 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- not V-shaped
- Star (spectrum)
- no
- V-shape (photometry)
- fails βUV −1.83, βopt −0.29 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 | 16.65 | 7.07 | 28.35 | 2.4 | 1.15 |
| F115W | NIRCam wide | 1.154 | 16.74 | 6.49 | 28.34 | 2.6 | 1.12 |
| F150W | NIRCam wide | 1.501 | 17.52 | 5.23 | 28.29 | 3.4 | 1.11 |
| F200W | NIRCam wide | 1.989 | 17.97 | 4.42 | 28.26 | 4.1 | 1.09 |
| F277W | NIRCam wide | 2.762 | 20.02 | 2.51 | 28.15 | 8.0 | 1.20 |
| F356W | NIRCam wide | 3.568 | 36.54 | 2.51 | 27.49 | 14.6 | 1.23 |
| F410M | NIRCam medium | 4.082 | 30.88 | 4.42 | 27.68 | 7.0 | 1.26 |
| F444W | NIRCam wide | 4.404 | 51.69 | 3.15 | 27.12 | 16.4 | 1.27 |
Provenance
- Field
- UDS (PRIMER UDS-2) (
primeruds2) - Programmes
01837, 07814behind every mosaic the field measured- Pipeline rows merged
- 3 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F090W | jw01837-c1001_t000_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01837-c1001_t000_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01837-c1001_t000_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw01837-c1001_t000_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01837-c1001_t000_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01837-c1001_t000_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01837-c1001_t000_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01837-c1001_t000_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 J021754.73-051007.3.
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.