Pith Number

pith:YX3MZ75Y

pith:2011:YX3MZ75YQ6EYSRFMWLI52VSVER

not attested not anchored not stored refs pending

Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1

Amelie Saintonge, Antonio Cava, Anton M. Koekemoer, Arjen van der Wel, Benjamin Magnelli, Dale D. Kocevski, Dieter Lutz, Elizabeth J. McGrath, Emeric Le Floc'h, Francesca Pozzi, Giulia Rodighiero, Guillermo Barro, Herve Aussel, Javier Gracia-Carpio, Kuang-Han Huang, Kyoung-Soo Lee, Laurie Riguccini, Linda Tacconi, Natascha M. Forster Schreiber, Nimish P. Hathi, Paola Popesso, Raanan Nordon, Reinhard Genzel, Stefano Berta, Stijn Wuyts, Yicheng Guo

arxiv:1107.0317 v2 · 2011-07-01 · astro-ph.CO

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{YX3MZ75YQ6EYSRFMWLI52VSVER}

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

4 papers in Pith

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

Empirical estimates of how massive galaxies can be in {\Lambda}CDM

Receipt and verification

First computed	2026-05-18T02:01:25.703918Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

c5f6ccffb887898944acb2d1dd5655245dcce76e478976553c2d588a1d7a83a0

Aliases

arxiv: 1107.0317 · arxiv_version: 1107.0317v2 · doi: 10.48550/arxiv.1107.0317 · pith_short_12: YX3MZ75YQ6EY · pith_short_16: YX3MZ75YQ6EYSRFM · pith_short_8: YX3MZ75Y

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/YX3MZ75YQ6EYSRFMWLI52VSVER \
  | 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: c5f6ccffb887898944acb2d1dd5655245dcce76e478976553c2d588a1d7a83a0

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "53a078fb16cf8f108c7f61a90130a8f06504b57e1829ab3885628a2314d9d323",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2011-07-01T20:00:02Z",
    "title_canon_sha256": "92cd642b6ddf49772aab1d3855c833dc86bc7313dd070fe004e8d7094216090e"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1107.0317",
    "kind": "arxiv",
    "version": 2
  }
}