LRD Watch DR1 · catalog object
LRDW J100017.27+021750.1
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
- MIRI
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- TENTATIVE
- Found by
- BH* channel
- Redshift
- 4.384 DJA grade 3, PRISM
- Spectral shape
- inconclusive de Graaff+25 criteria
- F444W
- 25.92 AB S/N 45, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.64 bhs_bb4800_b8; Δχ² galaxy 5.7, dwarf 66.6
- Compactness
- growth ratio 2.463 stars 2.250
- Balmer break
- 2.92 ± 0.26 F277W/F150W, red:Hb+OIII+blue:far-uv
- Image vetting
- half-stack pass; 1 flag(s)
- Literature
- 2 catalogue(s), 0 AGN paper(s) within 0.041″
Vetting
- Image vettingnot applicable
- Half-stack testpass
- Artifact risknone
- Neighbourflagged
- Extendedno
- BH* channelevidence dchi2_gal=5.7 dchi2_bd=66.6
- BH* channelBH* share 0.64 below 0.8 (composite)
- BH* channelneighbor-contam footprint-overlap id 5928 at 1.25" (npix=1534, r_eq=1.39") + bright-neighbor id 5928 m=19.0 at 1.25" (< excl 2.24")
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 | 4.3837 | mom-cos04-v4_prism-clear_5224_292585.spec.fits |
z_vet | Adopted by vetting | 4.3837 | zspec:dja_specz_grade3.csv:292585 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 4.488 | bhs_bb4800_b8 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- inconclusive
- Star (spectrum)
- no
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured 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.
- de Graaff et al. (2025)
- Kokorev 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 | 40.75 | 6.11 | 27.38 | 6.7 | 1.15 |
| F115W | NIRCam wide | 1.154 | 64.99 | 5.90 | 26.87 | 11.0 | 1.12 |
| F150W | NIRCam wide | 1.501 | 54.00 | 4.76 | 27.07 | 11.3 | 1.11 |
| F200W | NIRCam wide | 1.989 | 64.96 | 2.09 | 26.87 | 31.1 | 1.09–1.11 |
| F212N | NIRCam wide | 2.121 | 93.90 | 22.20 | 26.47 | 4.2 | 1.14 |
| F277W | NIRCam wide | 2.762 | 157.77 | 3.01 | 25.91 | 52.4 | 1.20 |
| F300M | NIRCam medium | 2.990 | 92.46 | 5.75 | 26.48 | 16.1 | 1.22 |
| F356W | NIRCam wide | 3.568 | 226.37 | 3.02 | 25.51 | 74.9 | 1.24 |
| F360M | NIRCam medium | 3.624 | 331.65 | 6.25 | 25.10 | 53.1 | 1.24 |
| F410M | NIRCam medium | 4.082 | 146.03 | 4.71 | 25.99 | 31.0 | 1.26 |
| F444W | NIRCam wide | 4.404 | 155.67 | 3.43 | 25.92 | 45.5 | 1.27 |
| F1500W | MIRI | 15.048 | 45.96 | 39.28 | 27.24 | 1.2 | 4.24 |
Provenance
- Field
- COSMOS (PRIMER) (
cosmos) - Programmes
01837, 02321, 07814behind 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 |
|---|---|---|---|
| F090W | jw01837-o003_t003_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw01837-o003_t003_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw01837-o003_t003_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw02321-o002_t001_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F277W | jw01837-o003_t003_nircam_clear-f277w_i2d.fits | 0.063″ | 1.00 |
| F356W | jw01837-o003_t003_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F410M | jw01837-o003_t003_nircam_clear-f410m_i2d.fits | 0.063″ | 1.00 |
| F444W | jw01837-o003_t003_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 J100017.27+021750.1.
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.