Pith Number

pith:AWKWIFZX

pith:2013:AWKWIFZX4YES7PANCBGYF772CG

not attested not anchored not stored refs pending

Studying Galactic interstellar turbulence through fluctuations in synchrotron emission: First LOFAR Galactic foreground detection

A. Alexov, A. Asgekar, A. Bonafede, A. G. Polatidis, A. Horneffer, A. Karastergiou, A. Scaife, A. W. Gunst, A. Zensus, B. Ciardi, B. W. Stappers, C. Ferrari, C. Horellou, C. Sobey, C. Sotomayor-Beltran, C. Tasse, C. Toribio, C. Vocks, C. Vogt, D. D. Mulcahy, D. Engels, D. Schwarz, E. de Geus, E. Orr\'u, F. Breitling, F. De Gasperin, G. Bernardi, G. Heald, G. Kuper, G. Macario, G. Mann, H. Falcke, H. Junklewitz, H. Munk, H. R. Butcher, H. R\"ottgering, I. M. Avruch, I. van Bemmel, J. Anderson, J. Broderick, J. E. Conway, J. Eisloffel, J. Griessmeier, J. Horandel, J. P. Hamaker, J. P. McKean, J. Sluman, J. van Leeuwen, J. W. T. Hessels, K. Chyzy, L. Birzan, L. V. E. Koopmans, M. A. Garrett, M. Bruggen, M. E. Bell, M. Haverkorn, M. Hoeft, M. Iacobelli, M. J. Bentum, M. Kramer, M. Kuniyoshi, M. Pandey-Pommier, M. R. Bell, M. Steinmetz, M. Tagger, M. W. Wise, O. Smirnov, O. Wucknitz, P. Best, P. Zarka, R. A. Fallows, R. Beck, R. F. Pizzo, R.-J. Dettmar, R. J. van Weeren, R. Paladino, R. Vermeulen, S. Duscha, S. Yatawatta, T.A. En{\ss}lin, T. E. Hassall, V. I. Kondratiev, V. Jelic, W. Frieswijk, W. Jurusik, W. N. Brouw, W. Reich, Y. Tang

arxiv:1308.2804 v2 · 2013-08-13 · astro-ph.GA

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{AWKWIFZX4YES7PANCBGYF772CG}

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

1 paper in Pith

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz

Receipt and verification

First computed	2026-05-18T03:15:42.825823Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

0595641737e6092fbc0d104d82fffa11b55a225fff67b62cb941f054ecc64253

Aliases

arxiv: 1308.2804 · arxiv_version: 1308.2804v2 · doi: 10.48550/arxiv.1308.2804 · pith_short_12: AWKWIFZX4YES · pith_short_16: AWKWIFZX4YES7PAN · pith_short_8: AWKWIFZX

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/AWKWIFZX4YES7PANCBGYF772CG \
  | 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: 0595641737e6092fbc0d104d82fffa11b55a225fff67b62cb941f054ecc64253

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "f543117dc5f5c96ac3fea3db573fccc60b9d56d138c10d8f07cb565772b8f9cb",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2013-08-13T09:52:20Z",
    "title_canon_sha256": "4699c9459a3b3a008c4e80fb6a991c5cb8b44e431c993dfb72a0bcb60cdcd8e2"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1308.2804",
    "kind": "arxiv",
    "version": 2
  }
}