LRD Watch DR1 · catalog object
LRDW J175359.35+651315.8
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. No coverage in F090W, F410M.
Spectral energy distribution
- NIRCam wide
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER main class
- Found by
- colour lane
- Redshift
- 6.697 DJA grade 3, PRISM
- Spectral shape
- inconclusive de Graaff+25 criteria
- F444W
- 26.09 AB S/N 24, 0.16″ aperture
- F277W − F444W
- 1.29 mag strict redness
- BH* share
- not in the BH* channel
- Compactness
- FWHM 0.149″
- Balmer break
- 3.53 ± 0.50 F356W/F200W, red:Hb+OIII+blue:far-uv
- Image vetting
- half-stack pass; no flags raised
- Literature
- 0 catalogue(s), 1 AGN paper(s) within 0.013″
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 | 6.6974 | nexus-obs7-v4_prism-clear_5105_21303.spec.fits |
z_vet | Adopted by vetting | 6.6974 | zspec:dja_specz_grade3.csv:21303 |
z_phot | Photometric (P(z) peak) | 7.584 | 68%: 3.099–8.083 |
z_bhs | BH* channel fit | — | — |
z_agn | Colour-lane fit | 7.58 | AGN-inclusive templates |
Spectral checks
- V-shape (spectrum)
- inconclusive
- Star (spectrum)
- no
- V-shape (photometry)
- fails βUV −0.16, βopt −1.29 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.
- Pan+2026 (NEXUS NIRSpec LRDs) broad-line AGN
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. |
|---|---|---|---|---|---|---|---|
| F115W | NIRCam wide | 1.154 | 10.86 | 14.02 | 28.81 | 0.8 | 1.12 |
| F150W | NIRCam wide | 1.501 | 19.26 | 8.66 | 28.19 | 2.2 | 1.11 |
| F200W | NIRCam wide | 1.989 | 32.39 | 4.45 | 27.62 | 7.3 | 1.09 |
| F277W | NIRCam wide | 2.762 | 40.85 | 2.77 | 27.37 | 14.8 | 1.19 |
| F356W | NIRCam wide | 3.568 | 114.70 | 4.23 | 26.25 | 27.1 | 1.23 |
| F444W | NIRCam wide | 4.404 | 133.56 | 5.65 | 26.09 | 23.6 | 1.27–1.28 |
Provenance
- Field
- NEXUS (
nexuscenter) - Programmes
05105, 09263behind every mosaic the field measured- Pipeline rows merged
- 2 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | jw09263-o001_t001_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw09263-o001_t001_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw09263-o001_t001_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw09263-o005_t004_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw09263-o001_t001_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F444W | jw09263-o002_t001_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 J175359.35+651315.8.
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.