LRD Watch DR1 · catalog object
LRDW J100025.85+020701.7
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
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 7.57 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 24.84 AB S/N 174, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.66 bhs_bb4200_b4; Δχ² galaxy 5.9, dwarf 13.7
- Compactness
- growth ratio 1.734 stars 2.036
- Balmer break
- 3.14 ± 0.13 F356W/F277W, clean
- Image vetting
- half-stack no-coverage; 1 flag(s)
- Literature
- 1 catalogue(s), 0 AGN paper(s) within 0.043″
Vetting
- Image vettingnot applicable
- Half-stack testno-coverage
- Artifact risknone
- Neighbourflagged
- Extendedno
- BH* channelevidence dchi2_gal=5.9 dchi2_bd=13.7
- BH* channelBH* share 0.66 below 0.8 (composite)
- BH* channelneighbor-contam footprint-overlap id 20621 at 0.46" (npix=319, r_eq=0.40")
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 | 7.5710 | bhstar:bhs_bb4200_b4 (zpub 0.8523 noted) |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 7.571 | bhs_bb4200_b4 |
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
- Hb, OIII 1 line-free optical band(s)
- Line-ambiguous
- yes
- Settling verdict
- not evaluated
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- Akins 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. |
|---|---|---|---|---|---|---|---|
| F115W | NIRCam wide | 1.154 | 22.08 | 11.53 | 28.04 | 1.9 | 1.31 |
| F150W | NIRCam wide | 1.501 | 33.32 | 12.37 | 27.59 | 2.7 | 1.33 |
| F277W | NIRCam wide | 2.762 | 64.53 | 2.49 | 26.88 | 25.9 | 1.43 |
| F356W | NIRCam wide | 3.568 | 202.36 | 2.47 | 25.64 | 81.8 | 1.49 |
| F444W | NIRCam wide | 4.404 | 420.44 | 2.42 | 24.84 | 173.9 | 1.52 |
Provenance
- Field
- PANORAMIC J100024+0208 (
panoramicj100024p0208) - Programmes
02514behind every mosaic the field measured- Pipeline rows merged
- 1 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F115W | panoramic-j100024p0208-grizli-v7.2-f115w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F150W | panoramic-j100024p0208-grizli-v7.2-f150w-clear_drc_sci.fits | 0.020″ | 1.00 |
| F200W | panoramic-j100024p0208-grizli-v7.2-f200w-clear_drc_sci.fits | 0.020″ | 0.52 |
| F277W | panoramic-j100024p0208-grizli-v7.2-f277w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F356W | panoramic-j100024p0208-grizli-v7.2-f356w-clear_drc_sci.fits | 0.040″ | 1.00 |
| F444W | panoramic-j100024p0208-grizli-v7.2-f444w-clear_drc_sci.fits | 0.040″ | 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 J100025.85+020701.7.
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.