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Researcher Evidence Record

Octavio M. Guilera

This bounded record lists 19 Pith paper rows and 0 imported work rows attributed to this corpus identity. The enumerated, non-disputed paper rows include astro-ph.EP, astro-ph.HE work dated 2010 to 2026. The record describes sources and coverage; it makes no judgment about the person.

Compiled coverage vector

Measured lane counts only. Not a trust score or person verdict.

Enumerated paper scope: 2 fields (astro-ph.EP, astro-ph.HE) · 2010-2026 sources: authors, author_identifiers · paper_authors · author_works · current_verdicts · cited_works

A sourced case file for attributed work. It is neither a profile score nor a verdict about this researcher.

Attributed works

A bounded ledger from the Pith paper and imported-work queries. Counts and source confidence stay with each work.

  1. 2026 Pith paper

    A formation pathway for giant planets in S-type discs of {\gamma}-Cephei-like compact binaries

    astro-ph.EP provisional current review present

    Sources and evidence
    Authorship source
    backfill
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: a current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  2. 2025 Pith paper

    Ionized envelopes around protoplanets and the role of radiative feedback in gas accretion

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    8
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  3. 2025 Pith paper

    From Streaming Instability to the Onset of Pebble Accretion I. Investigating the Growth Modes in Planetesimal Rings

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  4. 2025 Pith paper

    Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets II: The Role of Pebble Accretion in Planet Growth within a Global Planet Formation Model

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    1
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  5. 2025 Pith paper

    The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Complete Size Distributions for the 100 Brightest Disks Across Multiplicity and SED Classes

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    12
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  6. 2024 Pith paper

    A fading radius valley towards M-dwarfs, a persistent density valley across stellar types

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    3
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  7. 2023 Pith paper

    Planet formation around Intermediate-mass stars I: Different disc evolutionary pathways as a function of stellar mass

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    4
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  8. 2023 Pith paper

    Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    1
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  9. 2022 Pith paper

    Constraining mass, radius and tidal deformability of compact stars with axial wI modes: new universal relations including slow stable hybrid stars

    astro-ph.HE provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    4
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  10. 2022 Pith paper

    Breaking of universal relationships of axial wI-modes in hybrid stars: rapid and slow hadron-quark conversion scenarios

    astro-ph.HE provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  11. 2021 Pith paper

    Long live the disk: lifetimes of protoplanetary disks in hierarchical triple star systems and a possible explanation for HD 98800 B

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  12. 2020 Pith paper

    The Nature of the Radius Valley: Hints from Formation and Evolution Models

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  13. 2020 Pith paper

    Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  14. 2020 Pith paper

    How Jupiters save or destroy inner Neptunes around evolved stars

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    6
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 1 pith inbound references from cited_work_pith_inbound_counts
  15. 2020 Pith paper

    Setting the Stage: Planet formation and Volatile Delivery

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    3
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  16. 2019 Pith paper

    Hybrid magnetized stars within the Field Correlator Method

    astro-ph.HE provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    4
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  17. 2018 Pith paper

    Oscillation modes of hybrid stars within the relativistic Cowling approximation

    astro-ph.HE provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    • 2 pith inbound references from cited_work_pith_inbound_counts
  18. 2011 Pith paper

    The Diversity of Planetary Systems Architectures: Contrasting Theory with Observations

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.
  19. 2010 Pith paper

    The role of the initial surface density profiles of the disc on giant planet formation: comparing with observations

    astro-ph.EP provisional measured, no current review

    Sources and evidence
    Authorship source
    arxiv_oai
    Printed name
    Octavio M. Guilera
    Author position
    2
    Identity state
    provisional
    Source confidence
    0.7
    Review coverage
    Measured: no current Pith review exists.
    Citation counts
    No source count is attached to this work row.

Evidence apparatus

The machinery behind this record. Every lane states whether Pith measured it, did not query it, could not reach it, or withheld it.

LaneStateObservedBoundary and source
identity Measured 2 Canonical identity row plus public typed identifiers.
source=authors, author_identifiers
papers Measured 19 of 19 bounded rows Rows attributed to this author UUID in the Pith corpus.
source=paper_authors
works Measured zero 0 of 0 bounded rows Imported works not duplicated by the paper ledger.
source=author_works
reviews Measured 1 of 19 bounded rows Coverage count only. No review outcome is projected onto the person.
source=current_verdicts
citations Measured 7 of 19 bounded rows Counts remain itemized by work and source.
source=cited_works
coauthors Measured 49 of 19 bounded rows Shared-work edges from admitted paper rows.
source=paper_authors
account Unavailable No public count of 1 bounded rows Account metadata is separate from corpus evidence.
source=users.author_id
Public identity sources
  • name variant
    Octavio M. Guilera
    backfill
    confidence 0.6
Enumerated research scope

Fields and dates come only from enumerated, non-disputed Pith paper rows. They do not claim career completeness.

  • astro-ph.EP15 rows
  • astro-ph.HE4 rows
  • 20101 rows
  • 20111 rows
  • 20181 rows
  • 20191 rows
  • 20204 rows
  • 20211 rows
  • 20222 rows
  • 20232 rows
  • 20241 rows
  • 20254 rows
  • 20261 rows
Shared-work index
Record scope

The work queries are bounded. Missing rows may mean measured zero, an unavailable source, a query that did not run, or private data that Pith withheld. The lane table keeps those cases separate.

Paper findings remain attached to papers. They do not become findings about this researcher.