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Axia — Chandra Source Catalog corpus
astromindinc/axia-csc-corpus — 51,450 X-ray sources from the
Chandra Source Catalog 2.1, each carrying:
- Per-photon event lists in two forms: an
event_listpruned to a single 8 h window in 0.5-8 keV (the input shape the Axia fine-tuned model trained on), and anoriginal_event_listcontaining the full unpruned observation (the input to the model-free spectrum-snapshot / light-curve pipeline). - A 64-d learned embedding (
pca_64d) suitable for nearest-neighbour / vector search. The values are cosine-similarity-ready. - A 2-d UMAP projection (
umap_2d) for visualisation. - The full CSC catalog metadata: hardness ratios, four-model spectral fits, photometry, variability indices, sky coordinates, etc.
This is the dataset that backs the Axia multi-agent X-ray source decoder.
Quick start
from datasets import load_dataset
ds = load_dataset("astromindinc/axia-csc-corpus", split="train")
print(ds)
# Dataset({
# features: [...],
# num_rows: 51,450
# })
src = ds[0]
print(src["source_name"], "@", (src["ra"], src["dec"]))
print(" pruned events:", len(src["event_list"]))
print(" full events: ", len(src["original_event_list"]))
print(" embedding: ", len(src["pca_64d"]), "dim")
Stratification
The 11 source-type categories present in the corpus (training-set distribution):
| Category | Count |
|---|---|
| Other | 15,849 |
| Large accretors | 12,604 |
| Young stars | 8,221 |
| Normal stars | 4,407 |
| Small accretors | 3,899 |
| Normal galaxies | 2,549 |
| Active / variable stars | 1,386 |
| Stellar systems & clusters | 1,207 |
| Stellar remnants | 555 |
| Massive stars | 461 |
| White Dwarf accretors | 312 |
Fields
| Field | Type | Notes |
|---|---|---|
obsid |
int | Chandra observation ID |
obi |
int | Observation interval |
region_id |
int | CSC region ID |
source_name |
string | CSC source designation (e.g. 2CXO J123456.7+001122) |
ra, dec |
float | ICRS / J2000, decimal degrees |
theta |
float | Off-axis angle, arcmin |
source_type |
string | CSC source_type (e.g. AGN, Seyfert1, XB, X, ...) |
source_type_category |
string | One of 11 broad categories used for stratification |
thermal_classification |
string | thermal / nonthermal |
event_list |
list[[t_s, energy_eV]] | Pruned event list — single 8 h window, filtered to 0.5–8 keV. This is what the Axia fine-tuned model trained on. |
original_event_list |
list[[t_s, energy_eV]] | Original event list — full observation, all energies. Used by the spectrum-snapshot / light-curve / dE-dt computations. |
pca_64d |
listfloat | 64-d embedding from the Axia XrayProcessor → PCA pipeline. Cosine-similarity-indexable. |
umap_2d |
listfloat | 2-d UMAP projection for visualisation |
hard_hs, hard_hm, hard_ms |
float | Hardness ratios in the standard CSC H/M/S bands |
flux_significance_b |
float | Broad-band detection significance |
flux_aper_b, flux_bb_aper_b |
float | Broad-band aperture fluxes |
src_cnts_aper_b |
float | Net source counts in the aperture |
var_index_b, var_prob_b |
float | Variability index / probability (CSC) |
gti_mjd_obs |
float | Observation start time in MJD |
powlaw_stat, powlaw_gamma, powlaw_nh, powlaw_ampl |
float | Power-law spectral fit |
powlaw_gamma_lolim, powlaw_gamma_hilim |
float | Power-law Γ confidence bounds |
powerlaw_gamma_low, powerlaw_gamma_high |
float | Alternate Γ bound spelling (kept verbatim from CSC) |
bb_stat, bb_kt, bb_nh, bb_ampl |
float | Black-body spectral fit |
brems_stat, brems_kt |
float | Bremsstrahlung spectral fit |
apec_stat, apec_kt, apec_nh, apec_norm, apec_abund, apec_z |
float | APEC plasma spectral fit (NaN→null when not fit) |
preferred_spectral_model |
list[string] | Catalog recommendation |
recommended_model |
string | Catalog recommendation |
match_type |
string | CSC master-source match type |
significance |
float | CSC source significance |
Floats that are
NaNin the underlying CSC catalog are stored as JSONnull. ObjectIds and datetimes have been converted to strings.
Provenance
The X-ray and catalog data are derived from the Chandra Source Catalog 2.1
(CSC 2.1), which is freely available from the Harvard CXC. The pca_64d
embedding and the umap_2d projection were computed using the Axia
fine-tuned model (DeepSeek-R1-Distill-Qwen-7B + XrayProcessor, LoRA r=8).
Source cluster of this dump: am-webapp.niojd.mongodb.net.
Produced: 2026-05-28T10:31:23.830768Z.
Auxiliary files in this repo
data/corpus.jsonl.gz— the main file. One JSON document per line.data/metadata_records.json— small dataset registry used by the Axia webapp's/api/datasetsendpoint.data/atlas_indexes/pca_64_vector_search.json— MongoDB Atlas Vector Search index definition for thepca_64dfield (cosine, 64 dims).manifest.json— original dump provenance (counts, SHA-256, source cluster identifier).
Loading into MongoDB
The companion script data/ingest/load_from_huggingface.py in the
Axia repo downloads this dataset
and loads it into a MongoDB instance (local or Atlas), creating the
vector-search index if the target is Atlas.
# In the axia/ repo:
make load-from-hf # default: astromindinc/axia-csc-corpus
make load-from-hf DATASET=... # custom HF repo id
License
This packaged dataset is released under CC-BY-4.0. The underlying Chandra Source Catalog data is in the public domain; see the CSC homepage for the original data use policy. Please cite both the Axia paper and the CSC if you use this dataset in published work.
Citation
@misc{axia2026,
title = {Axia: a multi-agent decoder for Chandra X-ray sources},
author = {AstroMind Authors},
year = {2026},
note = {TBA — paper in preparation}
}
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