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Pith Number

pith:UGXGTYAG

pith:2026:UGXGTYAGNXTR7Q6VAFRIJD34XI
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Tracking down the broadband polarimetric properties of PG 1553+113

Alan P. Marscher, Alberto Floris, Alessandro Maselli, Alexander Kraus, Alexey V. Zhovtan, Alfredo Sota, Alkmini Koukoutsi, Anastasia Glykopoulou, Andrea Gokus, Andrey A. Vasilyev, Aristeidis Polychronakis, A. Trindade Falc\~ao, Beatriz Ag\'is-Gonz\'alez, Dana Kirchner, Daria A. Morozova, Dawoon E. Kim, Dimitrios A. Langis, Dimitrios Rompogiannakis, D. \L. Kr\'ol, Dmitry Blinov, Ekaterina V. Shishkina, Elena G. Larionova, Elina Lindfors, Emanuele Nardini, Emmanouil Angelakis, Evgenia N. Kopatskaya, Florian Eppel, Florian R\"osch, Francisco Jos\'e Aceituno, Gabriel Emery, Garrett Keating, George A. Borman, Georgios F. Paraschos, Hiroshi Akitaya, Ioannis Liodakis, Ioannis Myserlis, Iv\'an Agudo, Ivan S. Troitskiy, John A. Kypriotakis, Jonas He{\ss}d\"orfer, Jorge Otero-Santos, Juan Escudero Pedrosa, Julia Eich, Kari Nilsson, Koji S. Kawabata, Laura Di Gesu, Lena Debbrecht, Lucio A. Antonelli, Mahito Sasada, Makoto Uemura, Mark Gurwell, Matteo Perri, Matthias Kadler, Orestis Zoumpoulakis, Panagiotis Fotis, Petra Benke, Pouya M. Kouch, Ramprasad Rao, Riccardo Middei, Ryo Imazawa, Sara Capecchiacci, Sergey S. Savchenko, Simonetta Puccetti, Stavros Vogiatzis, Stefano Ciprini, Steven H\"ammerich, Sumie Tochihara, Svetlana G. Jorstad, Takahiro Akai, Tapio Pursimo, Tatiana S. Grishina, Tatsuya Nakaoka, Tommaso Aniello, Tsunefumi Mizuno, Vasiliki Tsioupli, V\'ictor Casanova, Vilppu Piirola, Vladimir A. Hagen-Thorn, Wladislaw Schulga, Yasushi Fukazawa, Yulia V. Troitskaya

X-ray and optical emissions from the blazar PG 1553+113 arise from closely related but not identical regions in its jet.

arxiv:2605.12602 v1 · 2026-05-12 · astro-ph.HE · hep-ph

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\pithnumber{UGXGTYAGNXTR7Q6VAFRIJD34XI}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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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.

Claims

C1strongest claim

the data support a picture in which the X-ray and optical emissions arise from closely related but not strictly co-spatial regions within a dynamically evolving, magnetically structured jet.

C2weakest assumption

The assumption that the observed polarization variability and EVPA rotation directly trace magnetic field configurations in the jet plasma rather than propagation effects or unrelated components.

C3one line summary

New IXPE X-ray polarimetry and optical monitoring of PG 1553+113 reveal variable polarization and a large EVPA swing, supporting jet models with related but non-co-spatial X-ray and optical emission regions.

References

226 extracted · 226 resolved · 88 Pith anchors

[12] A., Tombesi , F., et al 2024 · doi:10.1051/0004-6361/202449515
[13] Arnaud , K. A. 1996, title XSPEC: The First Ten Years , in Astronomical Society of the Pacific Conference Series, Vol. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & J. Bar 1996
[23] Capecchiacci , S., Liodakis , I., Middei , R., et al. 2025, title Unveiling blazar synchrotron emission: A multiwavelength polarimetric study of high-synchrotron and low-synchrotron peaked populations 2025 · doi:10.1051/0004-6361/202555392
[26] J., Liodakis , I., Middei , R., et al 2024 · doi:10.3847/1538-4357/ad63a1
[35] Gabriel , C., Denby , M., Fyfe , D. J., et al. 2004, title The XMM-Newton SAS - Distributed Development and Maintenance of a Large Science Analysis System: A Critical Analysis , in Astronomical Societ 2004
Receipt and verification
First computed 2026-05-18T03:10:00.980259Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

a1ae69e0066de71fc3d50162848f7cba32e894fd7c6d78cd7fafd7134ff1bb74

Aliases

arxiv: 2605.12602 · arxiv_version: 2605.12602v1 · doi: 10.48550/arxiv.2605.12602 · pith_short_12: UGXGTYAGNXTR · pith_short_16: UGXGTYAGNXTR7Q6V · pith_short_8: UGXGTYAG
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UGXGTYAGNXTR7Q6VAFRIJD34XI \
  | 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: a1ae69e0066de71fc3d50162848f7cba32e894fd7c6d78cd7fafd7134ff1bb74
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "63bcb0783f13055e7437a296aafebbad37c4939e52e9286a379854605a5366a0",
    "cross_cats_sorted": [
      "hep-ph"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2026-05-12T18:00:05Z",
    "title_canon_sha256": "473669bd5b3d3ea693b00d2a756bbd647bb4b37b3fc9aaeeb5f51065bde84303"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.12602",
    "kind": "arxiv",
    "version": 1
  }
}