Pith Number

pith:WLTDUBAX

pith:2016:WLTDUBAXQMPTKR7AZYHDSSSTYX

not attested not anchored not stored refs pending

Pan-STARRS Photometric and Astrometric Calibration

(10) Harvard-Smithsonian Center for Astrophysics), (2) Lawrence Berkeley National Laboratory, 3), (3) Hubble Fellow, (4) ITC Harvard-Smithsonian Center for Astrophysics, 5), (5) Department of Physics Harvard University, (6) Max Planck Institute for Astronomy, (7) Astronomisches Rechen-Institut Zentrum f\"ur Astronomie der Universit\"at Heidelberg, (8) Department of Astrophysical Sciences Princeton University, (9) Department of Physics Durham University, B. Goldman (6), C. W. Stubbs (10), C. Z. Waters (1), Douglas P. Finkbeiner (4, Edward. F. Schlafly (2, E. Schilbach (7), Eugene. A. Magnier (1), H. A. Flewelling (1), J. L. Tonry (1), K. C. Chambers (1), K. W. Hodapp (1), L. Denneau (1), M. E. Huber (1), N. Metcalfe (9), P. A. Price (8), P. Draper (9), R. Jedicke (1), R. J. Wainscoast (1) ((1) UH Institute for Astronomy, R.-P. Kudritzki (1), S. R\"oser (7), W. E. Sweeney (1)

arxiv:1612.05242 v3 · 2016-12-15 · astro-ph.IM

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{WLTDUBAXQMPTKR7AZYHDSSSTYX}

Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge

Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Cited by

5 papers in Pith

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star

Transient and Variable Ultra-luminous X-ray Sources in NGC 4552

Decadal pre-explosion activity and circumstellar interaction in a supernova

A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS

The Pan-STARRS1 Surveys

Receipt and verification

First computed	2026-07-05T01:52:13.332924Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

b2e63a0417831f3547e0ce0e394a53c5f555652474db9348d7f4d53b63d0ece4

Aliases

arxiv: 1612.05242 · arxiv_version: 1612.05242v3 · doi: 10.48550/arxiv.1612.05242 · pith_short_12: WLTDUBAXQMPT · pith_short_16: WLTDUBAXQMPTKR7A · pith_short_8: WLTDUBAX

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/WLTDUBAXQMPTKR7AZYHDSSSTYX \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: b2e63a0417831f3547e0ce0e394a53c5f555652474db9348d7f4d53b63d0ece4

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "3cf777cf4b45f9beb8e2eb760337485a979f42cba63347c4dbd372e273073b1f",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.IM",
    "submitted_at": "2016-12-15T20:50:21Z",
    "title_canon_sha256": "5118bd1304e06bfceae3e64e7a97579b5e4270fed69ad7a17d0ea020a718a465"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1612.05242",
    "kind": "arxiv",
    "version": 3
  }
}