Pith Number

pith:WJOIBRSF

pith:2024:WJOIBRSFNVGWTT5ZEBSOABXMSL

not attested not anchored not stored refs pending

WST -- Widefield Spectroscopic Telescope: Motivation, science drivers and top-level requirements for a new dedicated facility

Adriano Fontana, Andrea Cimatti, Angel Otarola, Ben Montet, Bianca Garilli, Bodo Ziegler, Christophe Yeche, Cyrielle Opitom, David Lee, Eline Tolstoi, Ian Bryson, Jarle Brinchmann, Jean-Paul Kneib, Joel Vernet, Julia Bryant, Laura Magrini, Laurence Tresse, Luca Pasquini, Marc Casali, Martin Roth, Matthew Colless, Matthew Lehnert, Matthias Steinmetz, Oscar Gonzalez, Paula Sanchez Saez, Philippe Dierickx, Pietro Schipani, Richard Anderson, Richard Ellis, Rodolfo Smiljanic, Roelof de Jong, Roland Bacon, Ruben Sanchez-Janssen, Simon Driver, Sofia Randich, Steffen Mieske, Tony Travouillon, Vanessa Hill, Vincenzo Maineiri, Warrick Couch

arxiv:2405.12518 v2 · 2024-05-21 · astro-ph.IM · astro-ph.CO · astro-ph.GA · astro-ph.SR

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{WJOIBRSFNVGWTT5ZEBSOABXMSL}

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

7 papers in Pith

Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints

Quality Assessment of Spectroscopic Data Reduction Pipelines Using Artificial Intelligence: Scrutinizing Data Release 2 from the DESI Survey

Characterizing robotic positioners under the influence of changing gravity vectors for future spectroscopic surveys

Unlocking the Full Potential of SKAO Extra-galactic Science with High-multiplex Optical Spectroscopy

Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology

Receipt and verification

First computed	2026-07-05T08:29:00.781175Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

b25c80c6456d4d69cfb92064e006ec92f48edb8213c7d620769fd0b855fe8de9

Aliases

arxiv: 2405.12518 · arxiv_version: 2405.12518v2 · doi: 10.48550/arxiv.2405.12518 · pith_short_12: WJOIBRSFNVGW · pith_short_16: WJOIBRSFNVGWTT5Z · pith_short_8: WJOIBRSF

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/WJOIBRSFNVGWTT5ZEBSOABXMSL \
  | 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: b25c80c6456d4d69cfb92064e006ec92f48edb8213c7d620769fd0b855fe8de9

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "696a7b1b18ded2dbf1d7a125d05b50784f3b6f66ed0d9365c595a136c885ab68",
    "cross_cats_sorted": [
      "astro-ph.CO",
      "astro-ph.GA",
      "astro-ph.SR"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.IM",
    "submitted_at": "2024-05-21T06:08:59Z",
    "title_canon_sha256": "7d070b003ad351ed7c196da4561e80a89e10f688ff306e265455d43ece63e57c"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2405.12518",
    "kind": "arxiv",
    "version": 2
  }
}