---
OA_place: publisher
OA_type: hybrid
PlanS_conform: '1'
_id: '21484'
abstract:
- lang: eng
text: An individual's phenotype reflects a complex interplay of the direct effects
of their DNA, epigenetic modifications of their DNA induced by their parents,
and indirect effects of their parents' DNA. Here, we derive how the genetic variance
within a population is changed under the influence of indirect maternal, paternal
and parent-of-origin effects under random mating. We also consider indirect effects
of a sibling, in particular how the genetic variance is altered when looking at
the phenotypic difference between two siblings. The calculations are then extended
to include assortative mating (AM), which alters the variance by inducing increased
homozygosity and correlations within and across loci. AM likely leads to covariance
of parental genetic effects, a measure of the similarity of parents in the indirect
effects they have on their children. We propose that this assortment for parental
characteristics, where biological parents create similar environments for their
children, can create shared parental effects across traits and the appearance
of cross-trait AM. Our theory shows how the resemblance among relatives increases
under both AM, indirect and parent-of-origin effects. When our model is used to
predict correlations among relatives in human height, we find that explaining
the patterns observed in real data requires both indirect genetic effects and
assortative mating. The degree to which direct, indirect and epigenetic effects
shape the phenotypic variance of complex traits remains an open question that
requires large-scale family data to be resolved.
acknowledgement: We thank members of the Medical Genomics group at ISTA for their
comments, which improved this manuscript. This work was funded by an SNSF Eccellenza
Grant to MRR (PCEGP3-181181), and by core funding from the Institute of Science
and Technology Austria.
article_number: iyag042
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Ilse
full_name: Krätschmer, Ilse
id: 30d4014e-7753-11eb-b44b-db6d61112e73
last_name: Krätschmer
orcid: 0000-0002-5636-9259
- first_name: Matthew Richard
full_name: Robinson, Matthew Richard
id: E5D42276-F5DA-11E9-8E24-6303E6697425
last_name: Robinson
orcid: 0000-0001-8982-8813
citation:
ama: Krätschmer I, Robinson MR. A quantitative genetic model for indirect genetic
effects and genomic imprinting under random and assortative mating. Genetics.
2026. doi:10.1093/genetics/iyag042
apa: Krätschmer, I., & Robinson, M. R. (2026). A quantitative genetic model
for indirect genetic effects and genomic imprinting under random and assortative
mating. Genetics. Oxford University Press. https://doi.org/10.1093/genetics/iyag042
chicago: Krätschmer, Ilse, and Matthew Richard Robinson. “A Quantitative Genetic
Model for Indirect Genetic Effects and Genomic Imprinting under Random and Assortative
Mating.” Genetics. Oxford University Press, 2026. https://doi.org/10.1093/genetics/iyag042.
ieee: I. Krätschmer and M. R. Robinson, “A quantitative genetic model for indirect
genetic effects and genomic imprinting under random and assortative mating,” Genetics.
Oxford University Press, 2026.
ista: Krätschmer I, Robinson MR. 2026. A quantitative genetic model for indirect
genetic effects and genomic imprinting under random and assortative mating. Genetics.,
iyag042.
mla: Krätschmer, Ilse, and Matthew Richard Robinson. “A Quantitative Genetic Model
for Indirect Genetic Effects and Genomic Imprinting under Random and Assortative
Mating.” Genetics, iyag042, Oxford University Press, 2026, doi:10.1093/genetics/iyag042.
short: I. Krätschmer, M.R. Robinson, Genetics (2026).
corr_author: '1'
date_created: 2026-03-23T15:02:54Z
date_published: 2026-02-12T00:00:00Z
date_updated: 2026-06-18T08:31:14Z
day: '12'
ddc:
- '570'
department:
- _id: MaRo
doi: 10.1093/genetics/iyag042
external_id:
pmid:
- '41677404'
has_accepted_license: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/genetics/iyag042
month: '02'
oa: 1
oa_version: Published Version
pmid: 1
publication: Genetics
publication_identifier:
issn:
- 1943-2631
publication_status: epub_ahead
publisher: Oxford University Press
quality_controlled: '1'
related_material:
link:
- relation: software
url: https://github.com/medical-genomics-group/familyMC
status: public
title: A quantitative genetic model for indirect genetic effects and genomic imprinting
under random and assortative mating
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '21502'
abstract:
- lang: eng
text: The mammalian brain stores glucose, the main circulating energy substrate,
as glycogen. In rodents, the cerebellum contains relatively high glycogen levels,
yet its cellular and subcellular distribution remains poorly defined. Using monoclonal
antibodies against glycogen, we examined its distribution in the mouse cerebellar
cortex. Glycogen was predominantly localized to Bergmann glia (BG) processes in
the molecular layer and was also detected in Purkinje cells (PCs), the principal
cerebellar neurons. To assess the functional significance of cerebellar glycogen,
we analyzed behavior in mice lacking glycogen synthase 1 (Gys1) in BG or PCs using
a floxed Gys1 line. Gys1 deficiency in either PCs or GFAP-positive cells reduced
anxiety-like behavior, whereas combined deletion caused PC degeneration and ataxia.
These findings reveal a critical role for glycogen metabolism in both astrocytes
and neurons in cerebellar function.
acknowledgement: This work was supported by the Novo Nordisk Foundation (NNFOC0058058,
H. Hirase), the Danmarks Frie Forskningsfond (0134-00107B and 5283-00069A, H.Hirase),
the Lundbeck Foundation, Japan Society for the Promotion of Science Grants-in-Aid
for Scientific Research (KAKENHI) program (22K06454/24H01221, A.K.; 23K27482, H.Hirai),
the Japan Agency for Medical Research and Development (AMED) Brain Mapping by Integrated
Neurotechnologies for Disease Studies (Brain/MINDS) (JP21dm0207111, H. Hirai), AMED
Brain/MINDS 2.0 (JP23wm0625001 and JP24wm0625103, H. Hirai), and grants from the
Spanish Ministerio de Ciencia e Innovación (MCIU/FEDER/AEI) (PID2020-118699 GB-100,
J.D.) and the Fundación Ramón Areces (J.D.). Sonam Akther has been supported by
the RIKEN IPA fellowship. We are thankful to Dr. Yuki Oe for his support in the
initial stage of this study and to Dan Xue for his help with the graphical abstract.
We thank Dr. Pia Weikop for providing CTN research infrastructure. The authors declare
no competing financial interests.
article_number: '115192'
article_processing_charge: Yes
article_type: original
author:
- first_name: Sonam
full_name: Akther, Sonam
last_name: Akther
- first_name: Ashley Bomin
full_name: Lee, Ashley Bomin
last_name: Lee
- first_name: Ayumu
full_name: Konno, Ayumu
last_name: Konno
- first_name: Antonis
full_name: Asiminas, Antonis
last_name: Asiminas
- first_name: Marta
full_name: Vittani, Marta
last_name: Vittani
- first_name: Tsuneko
full_name: Mishima, Tsuneko
last_name: Mishima
- first_name: Hirokazu
full_name: Hirai, Hirokazu
last_name: Hirai
- first_name: Claire Francesca
full_name: Meehan, Claire Francesca
last_name: Meehan
- first_name: Jordi
full_name: Duran, Jordi
last_name: Duran
- first_name: Joan
full_name: Guinovart, Joan
last_name: Guinovart
- first_name: Hitoshi
full_name: Ashida, Hitoshi
last_name: Ashida
- first_name: Tsuyoshi
full_name: Morita, Tsuyoshi
last_name: Morita
- first_name: Otto
full_name: Baba, Otto
last_name: Baba
- first_name: Ryuichi
full_name: Shigemoto, Ryuichi
id: 499F3ABC-F248-11E8-B48F-1D18A9856A87
last_name: Shigemoto
orcid: 0000-0001-8761-9444
- first_name: Maiken
full_name: Nedergaard, Maiken
last_name: Nedergaard
- first_name: Hajime
full_name: Hirase, Hajime
last_name: Hirase
citation:
ama: Akther S, Lee AB, Konno A, et al. Distribution and functional significance
of rodent cerebellar glycogen. iScience. 2026;29(4). doi:10.1016/j.isci.2026.115192
apa: Akther, S., Lee, A. B., Konno, A., Asiminas, A., Vittani, M., Mishima, T.,
… Hirase, H. (2026). Distribution and functional significance of rodent cerebellar
glycogen. IScience. Elsevier. https://doi.org/10.1016/j.isci.2026.115192
chicago: Akther, Sonam, Ashley Bomin Lee, Ayumu Konno, Antonis Asiminas, Marta Vittani,
Tsuneko Mishima, Hirokazu Hirai, et al. “Distribution and Functional Significance
of Rodent Cerebellar Glycogen.” IScience. Elsevier, 2026. https://doi.org/10.1016/j.isci.2026.115192.
ieee: S. Akther et al., “Distribution and functional significance of rodent
cerebellar glycogen,” iScience, vol. 29, no. 4. Elsevier, 2026.
ista: Akther S, Lee AB, Konno A, Asiminas A, Vittani M, Mishima T, Hirai H, Meehan
CF, Duran J, Guinovart J, Ashida H, Morita T, Baba O, Shigemoto R, Nedergaard
M, Hirase H. 2026. Distribution and functional significance of rodent cerebellar
glycogen. iScience. 29(4), 115192.
mla: Akther, Sonam, et al. “Distribution and Functional Significance of Rodent Cerebellar
Glycogen.” IScience, vol. 29, no. 4, 115192, Elsevier, 2026, doi:10.1016/j.isci.2026.115192.
short: S. Akther, A.B. Lee, A. Konno, A. Asiminas, M. Vittani, T. Mishima, H. Hirai,
C.F. Meehan, J. Duran, J. Guinovart, H. Ashida, T. Morita, O. Baba, R. Shigemoto,
M. Nedergaard, H. Hirase, IScience 29 (2026).
date_created: 2026-03-29T22:07:07Z
date_published: 2026-03-17T00:00:00Z
date_updated: 2026-06-18T08:32:22Z
day: '17'
ddc:
- '570'
department:
- _id: RySh
doi: 10.1016/j.isci.2026.115192
external_id:
pmid:
- '41890976'
intvolume: ' 29'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1016/j.isci.2026.115192
month: '03'
oa: 1
oa_version: Published Version
pmid: 1
publication: iScience
publication_identifier:
eissn:
- 2589-0042
publication_status: epub_ahead
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Distribution and functional significance of rodent cerebellar glycogen
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 29
year: '2026'
...
---
OA_place: publisher
OA_type: gold
_id: '21436'
abstract:
- lang: eng
text: 'The cobalt-intercalated transition metal dichalcogenide CoxTaS2 hosts a rich
landscape of magnetic phases that depend sensitively on x. While the stoichiometric
compound with x = 1/3 exhibits a single magnetic transition, samples with x≤0.325
display two transitions with an anomalous Hall effect (AHE) emerging in the lower
temperature phase. Here, we resolve the spin structure in each phase by employing
a suite of magneto-optical probes that include the discovery of anomalous magneto-birefringence:
a spontaneous time-reversal sensitive rotation of the principal optic axes. A
symmetry-based analysis identifies the AHE-active phase as an anisotropic (2+1)Q
state, in which magnetic modulation at one wavevector (Q) differs in symmetry
from that at the remaining two. The (2+1)Q state naturally exhibits scalar spin
chirality as a mechanism for the AHE and expands the classification of multi-Q
magnetic phases.'
acknowledgement: 'We thank Linda Ye and Yue Sun for helpful discussion. Experimental
and theoretical work at LBNL and UC Berkeley was funded by the Quantum Materials
(KC2202) program under the U.S. Department of Energy, Office of Science, Office
of Basic Energy Sciences, Materials Sciences and Engineering Division under Contract
No. DE-AC02-05CH11231. V.S. and J.O. received support from the Gordon and Betty
Moore Foundation’s EPiQS Initiative through Grant GBMF4537 to J.O. at UC Berkeley.
J.K. received support from the National Science Foundation Graduate Research Fellowship
Program under Grant No. 2146752. Any opinions, findings, and conclusions or recommendations
expressed in this material are those of the author(s) and do not necessarily reflect
the views of the National Science Foundation. During the preparation of this manuscript,
we became aware of the following related work: refs. 56,57,58.'
article_number: '2507.12588'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Jonathon
full_name: Kruppe, Jonathon
last_name: Kruppe
- first_name: Josue
full_name: Rodriguez, Josue
last_name: Rodriguez
- first_name: Catherine
full_name: Xu, Catherine
last_name: Xu
- first_name: James
full_name: Analytis, James
last_name: Analytis
- first_name: Joseph
full_name: Orenstein, Joseph
last_name: Orenstein
- first_name: Veronika
full_name: Sunko, Veronika
id: 23cb1cf6-2c7a-11ef-91a4-f72fc19f20b3
last_name: Sunko
orcid: 0000-0003-2724-3523
citation:
ama: Kruppe J, Rodriguez J, Xu C, Analytis J, Orenstein J, Sunko V. Anisotropic
multi-Q order in CoxTaS2. npj Quantum Materials. 2026. doi:10.1038/s41535-026-00856-w
apa: Kruppe, J., Rodriguez, J., Xu, C., Analytis, J., Orenstein, J., & Sunko,
V. (2026). Anisotropic multi-Q order in CoxTaS2. Npj Quantum Materials.
Springer Nature. https://doi.org/10.1038/s41535-026-00856-w
chicago: Kruppe, Jonathon, Josue Rodriguez, Catherine Xu, James Analytis, Joseph
Orenstein, and Veronika Sunko. “Anisotropic Multi-Q Order in CoxTaS2.” Npj
Quantum Materials. Springer Nature, 2026. https://doi.org/10.1038/s41535-026-00856-w.
ieee: J. Kruppe, J. Rodriguez, C. Xu, J. Analytis, J. Orenstein, and V. Sunko, “Anisotropic
multi-Q order in CoxTaS2,” npj Quantum Materials. Springer Nature, 2026.
ista: Kruppe J, Rodriguez J, Xu C, Analytis J, Orenstein J, Sunko V. 2026. Anisotropic
multi-Q order in CoxTaS2. npj Quantum Materials., 2507.12588.
mla: Kruppe, Jonathon, et al. “Anisotropic Multi-Q Order in CoxTaS2.” Npj Quantum
Materials, 2507.12588, Springer Nature, 2026, doi:10.1038/s41535-026-00856-w.
short: J. Kruppe, J. Rodriguez, C. Xu, J. Analytis, J. Orenstein, V. Sunko, Npj
Quantum Materials (2026).
corr_author: '1'
date_created: 2026-03-11T10:39:55Z
date_published: 2026-04-09T00:00:00Z
date_updated: 2026-06-18T08:32:52Z
day: '09'
ddc:
- '530'
department:
- _id: VeSu
doi: 10.1038/s41535-026-00856-w
external_id:
arxiv:
- '2507.12588'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1038/s41535-026-00856-w
month: '04'
oa: 1
oa_version: Published Version
publication: npj Quantum Materials
publication_identifier:
eissn:
- 2397-4648
publication_status: epub_ahead
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Anisotropic multi-Q order in CoxTaS2
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21986'
abstract:
- lang: eng
text: Over the past two decades, molecular electronics has made significant progress
toward discovering nanoscale analogues of conventional electronic components,
largely enabled by the development of the scanning tunneling microscope-based
break-junction (STM-BJ) technique. The STM-BJ technique enables precise and highly
reproducible measurement of a molecule’s electronic transport properties, making
it a powerful technique to explore physiochemical and electrochemical phenomena
that are otherwise difficult to access. It has gained substantial popularity in
the past 20 years, with experiments becoming increasingly diverse and sophisticated.
Despite the wealth of literature, an accessible, practical guide to performing
STM-BJ experiments and interpreting the data is largely absent. This tutorial
includes a brief background into the development of STM-BJ measurements, followed
by detailed explanations of instrumentation, data collection, statistical analysis,
variations on standard experiments, and some troubleshooting methods. It is aimed
at researchers looking to begin or improve STM-BJ studies in their laboratories,
graduate students and postdoctoral researchers learning the technique, and readers
seeking to critically evaluate the growing body of STM-BJ literature.
acknowledgement: We thank Michael Inkpen, Timothy Su, Masha Kamenetska, and Wanzhuo
Shi for comments and Jyotisman Hazarika for data collection. This work was supported
in part by the National Science Foundation (NSF-DMR 2241180) and by the Institute
of Science and Technology Austria.
article_processing_charge: Yes
article_type: original
author:
- first_name: Emma
full_name: York, Emma
id: 08dde91e-8e0a-11f0-9d7d-9e8d80864f16
last_name: York
- first_name: Latha
full_name: Venkataraman, Latha
id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf
last_name: Venkataraman
orcid: 0000-0002-6957-6089
citation:
ama: York E, Venkataraman L. Scanning tunneling microscope-based break-junction
technique - A tutorial. ACS Physical Chemistry Au. 2026;6(3):408-424. doi:10.1021/acsphyschemau.6c00026
apa: York, E., & Venkataraman, L. (2026). Scanning tunneling microscope-based
break-junction technique - A tutorial. ACS Physical Chemistry Au. American
Chemical Society. https://doi.org/10.1021/acsphyschemau.6c00026
chicago: York, Emma, and Latha Venkataraman. “Scanning Tunneling Microscope-Based
Break-Junction Technique - A Tutorial.” ACS Physical Chemistry Au. American
Chemical Society, 2026. https://doi.org/10.1021/acsphyschemau.6c00026.
ieee: E. York and L. Venkataraman, “Scanning tunneling microscope-based break-junction
technique - A tutorial,” ACS Physical Chemistry Au, vol. 6, no. 3. American
Chemical Society, pp. 408–424, 2026.
ista: York E, Venkataraman L. 2026. Scanning tunneling microscope-based break-junction
technique - A tutorial. ACS Physical Chemistry Au. 6(3), 408–424.
mla: York, Emma, and Latha Venkataraman. “Scanning Tunneling Microscope-Based Break-Junction
Technique - A Tutorial.” ACS Physical Chemistry Au, vol. 6, no. 3, American
Chemical Society, 2026, pp. 408–24, doi:10.1021/acsphyschemau.6c00026.
short: E. York, L. Venkataraman, ACS Physical Chemistry Au 6 (2026) 408–424.
corr_author: '1'
date_created: 2026-06-10T07:38:41Z
date_published: 2026-05-04T00:00:00Z
date_updated: 2026-06-19T06:35:58Z
day: '04'
ddc:
- '540'
department:
- _id: LaVe
doi: 10.1021/acsphyschemau.6c00026
external_id:
pmid:
- '42221941'
file:
- access_level: open_access
checksum: 1dc16bdfb1c1cd3acde802f4350cb42a
content_type: application/pdf
creator: dernst
date_created: 2026-06-19T06:31:16Z
date_updated: 2026-06-19T06:31:16Z
file_id: '22020'
file_name: 2026_ACSPhysChem_York.pdf
file_size: 11251172
relation: main_file
success: 1
file_date_updated: 2026-06-19T06:31:16Z
has_accepted_license: '1'
intvolume: ' 6'
issue: '3'
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
page: 408-424
pmid: 1
publication: ACS Physical Chemistry Au
publication_identifier:
eissn:
- 2694-2445
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Scanning tunneling microscope-based break-junction technique - A tutorial
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 6
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '21987'
abstract:
- lang: eng
text: 'We introduce JODIE, a genetic joint modeling approach that estimates how
DNA loci influence human traits by partitioning genetic effects into four components:
direct effects (from a child’s alleles), indirect maternal and paternal effects
(from parents’ alleles), and parent-of-origin (PofO) effects (dependent on parental
transmission of alleles), while uniquely accounting for assortative mating. We
analyze 30,000 child-mother-father trios from the Estonian Biobank and the Norwegian
Mother, Father, and Child Cohort, focusing on height, body mass index, and childhood
educational test scores. We find direct effects to be the largest contributor
to trait variation, but combined, indirect parental and PofO effects are similarly
substantial. We support our results by within-family genome-wide association testing
and identify 276 independently associated DNA regions with a complex interplay
between direct, indirect, and PofO effects. By joint modeling, we show that direct,
indirect, and PofO effects collectively shape human phenotypic variation across
loci genome-wide.'
acknowledged_ssus:
- _id: ScienComp
acknowledgement: "We thank Zoltan Kutalik, Peter Visscher, and members of the Robinson
group at ISTA for their comments, which improved this manuscript. This work was
funded by an SNSF Eccellenza Grant to M.R.R. (PCEGP3-181181) and by core funding
from the Institute of Science and Technology Austria.\r\nThe Norwegian Mother, Father,
and Child Cohort Study is supported by the Norwegian Ministry of Health and Care
Services and the Ministry of Education and Research. We are grateful to all the
participating families in Norway who take part in this on-going cohort study. We
thank the Norwegian Institute of Public Health (NIPH) for generating high-quality
genomic data. The research is part of the HARVEST collaboration, supported by the
Research Council of Norway (#229624). We also thank the NORMENT Center for providing
genotype data, funded by the Research Council of Norway (#223273), South East Norway
Health Authorities, and Stiftelsen Kristian Gerhard Jebsen, and in collaboration
with deCODE Genetics. We further thank the Center for Diabetes Research, the University
of Bergen for providing genotype data funded by the ERC AdG project SELECTionPREDISPOSED,
Stiftelsen Kristian Gerhard Jebsen, Trond Mohn Foundation, the Research Council
of Norway, the Novo Nordisk Foundation, the University of Bergen, and the Western
Norway Health Authorities. The MoBa work was performed on the TSD (Tjeneste for
Sensitive Data) facilities, owned by the University of Oslo, operated and developed
by the TSD service group at the University of Oslo, IT Department (USIT, tsd-drift@usit.uio.no).
E.Y. is supported by the European Union (grant numbers 101045526 and 101073237)
and the Research Council of Norway (grant numbers 336078, 288083, and 331640).\r\nWe
would like to acknowledge the participants and investigators of the Generation Scotland
Cohort study. Generation Scotland received core support from the Chief Scientist
Office of the Scottish Government Health Directorates (CZD/16/6) and the Scottish
Funding Council (HR03006). Genotyping and methylation typing of the GS:SFHS samples
was carried out by the Genetics Core Laboratory at the Wellcome Trust Clinical Research
Facility, Edinburgh, Scotland and was funded by the Medical Research Council UK
and the Wellcome Trust (Wellcome Trust Strategic Award “STratifying Resilience and
Depression Longitudinally” [STRADL] ref. 104036/Z/14/Z).\r\nWe would like to thank
and acknowledge the participants and investigators of the Estonian Biobank (EstBB)
study. The research was conducted using the Estonian Center of Genomics/Roadmap
II funded by the Estonian Research Council (project number TT17).\r\nNorwegian analyses
were performed on resources provided by Sigma2 - the National Infrastructure for
High-Performance Computing and Data Storage in Norway. Estonian Data analysis was
carried out in the High-Performance Computing Center cloud provided by University
of Tartu. Analysis of the Generation Scotland data and the summary statistics obtained
from the other analyses was conducted at IST Austria and is supported by the Scientific
Service Units (SSU) of IST Austria through resources provided by Scientific Computing
(SciComp)."
article_number: '101277'
article_processing_charge: Yes
article_type: original
author:
- first_name: Ilse
full_name: Krätschmer, Ilse
id: 30d4014e-7753-11eb-b44b-db6d61112e73
last_name: Krätschmer
orcid: 0000-0002-5636-9259
- first_name: Laura
full_name: Hegemann, Laura
last_name: Hegemann
- first_name: Robin J.
full_name: Hofmeister, Robin J.
last_name: Hofmeister
- first_name: Elizabeth C.
full_name: Corfield, Elizabeth C.
last_name: Corfield
- first_name: Mahdi
full_name: Mahmoudi, Mahdi
last_name: Mahmoudi
- first_name: Olivier
full_name: Delaneau, Olivier
last_name: Delaneau
- first_name: Ole A.
full_name: Andreassen, Ole A.
last_name: Andreassen
- first_name: Archie
full_name: Campbell, Archie
last_name: Campbell
- first_name: Caroline
full_name: Hayward, Caroline
last_name: Hayward
- first_name: Riccardo E.
full_name: Marioni, Riccardo E.
last_name: Marioni
- first_name: Eivind
full_name: Ystrom, Eivind
last_name: Ystrom
- first_name: Alexandra
full_name: Havdahl, Alexandra
last_name: Havdahl
- first_name: Matthew Richard
full_name: Robinson, Matthew Richard
id: E5D42276-F5DA-11E9-8E24-6303E6697425
last_name: Robinson
orcid: 0000-0001-8982-8813
citation:
ama: Krätschmer I, Hegemann L, Hofmeister RJ, et al. Separating direct, indirect,
and parent-of-origin genetic effects in the human population. Cell Genomics.
doi:10.1016/j.xgen.2026.101277
apa: Krätschmer, I., Hegemann, L., Hofmeister, R. J., Corfield, E. C., Mahmoudi,
M., Delaneau, O., … Robinson, M. R. (n.d.). Separating direct, indirect, and parent-of-origin
genetic effects in the human population. Cell Genomics. Elsevier. https://doi.org/10.1016/j.xgen.2026.101277
chicago: Krätschmer, Ilse, Laura Hegemann, Robin J. Hofmeister, Elizabeth C. Corfield,
Mahdi Mahmoudi, Olivier Delaneau, Ole A. Andreassen, et al. “Separating Direct,
Indirect, and Parent-of-Origin Genetic Effects in the Human Population.” Cell
Genomics. Elsevier, n.d. https://doi.org/10.1016/j.xgen.2026.101277.
ieee: I. Krätschmer et al., “Separating direct, indirect, and parent-of-origin
genetic effects in the human population,” Cell Genomics. Elsevier.
ista: Krätschmer I, Hegemann L, Hofmeister RJ, Corfield EC, Mahmoudi M, Delaneau
O, Andreassen OA, Campbell A, Hayward C, Marioni RE, Ystrom E, Havdahl A, Robinson
MR. Separating direct, indirect, and parent-of-origin genetic effects in the human
population. Cell Genomics., 101277.
mla: Krätschmer, Ilse, et al. “Separating Direct, Indirect, and Parent-of-Origin
Genetic Effects in the Human Population.” Cell Genomics, 101277, Elsevier,
doi:10.1016/j.xgen.2026.101277.
short: I. Krätschmer, L. Hegemann, R.J. Hofmeister, E.C. Corfield, M. Mahmoudi,
O. Delaneau, O.A. Andreassen, A. Campbell, C. Hayward, R.E. Marioni, E. Ystrom,
A. Havdahl, M.R. Robinson, Cell Genomics (n.d.).
corr_author: '1'
date_created: 2026-06-10T07:39:08Z
date_published: 2026-06-09T00:00:00Z
date_updated: 2026-06-19T07:00:47Z
day: '09'
department:
- _id: MaRo
doi: 10.1016/j.xgen.2026.101277
external_id:
pmid:
- '40909755'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1016/j.xgen.2026.101277
month: '06'
oa: 1
oa_version: Published Version
pmid: 1
project:
- _id: 9B8D11D6-BA93-11EA-9121-9846C619BF3A
grant_number: PCEGP3_181181
name: Improving estimation and prediction of common complex disease risk
publication: Cell Genomics
publication_identifier:
eissn:
- 2666-979X
publication_status: inpress
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Separating direct, indirect, and parent-of-origin genetic effects in the human
population
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
OA_place: repository
OA_type: green
_id: '21994'
abstract:
- lang: eng
text: Adaptive plant development is orchestrated, among others, by directional,
intercellular transport of the phytohormone auxin. Self-organizing development,
such as flexible vasculature formation, depends on so-called auxin canalization,
manifested by the gradual formation of auxin transport channels through feedback
between auxin signalling and transport. Herein, we identify MAKR6 as an important,
novel component in this feedback. MAKR6 expression accumulates strongly in vascular
cells and is tightly regulated by auxin via the Aux/IAA-ARF-WRKY23 transcriptional
network. MAKR6 is required for auxin canalization-dependent processes, including
leaf venation, vasculature regeneration, and de novo auxin channel formation from
local auxin sources. Mechanistically, MAKR6 interacts with the PIN1 auxin transporter,
modulating its trafficking and polarization. MAKR6 also associates with and integrates
two key receptor-like kinase complexes involved in canalization, TMK1/4 and the
CAMEL-CANAR. Together, our study establishes MAKR6 as a multifaceted regulator
that couples transcriptional auxin signalling to PIN1 repolarization and coordinates
multiple RLK-mediated signalling pathways during canalization. This provides mechanistic
insights into auxin canalization and exemplifies a framework for exploring similar
regulatory nodes in other developmental contexts.
acknowledgement: 'We would like to thank Dr. Yvon Jaillais (ENS, Lyon) for sharing
MAKR2 materials. This research was supported by the Scientific Service Units (SSU)
of ISTA through resources provided by the Imaging & Optics Facility (IOF) and the
Lab Support Facility (LSF). The research in the Friml group leading to these results
was funded by the European Research Council (ERC): 101142681 CYNIPS; and the Austrian
Science Fund (FWF): I 6123-B and P 37051-B. Ewa Mazur was supported by the National
Science Centre (NCN), Poland, under the OPUS call in the WEAVE programme: 2021/43/I/NZ1/01835.'
article_processing_charge: No
author:
- first_name: Zengxiang
full_name: Ge, Zengxiang
id: f43371a3-09ff-11eb-8013-bd0c6a2f6de8
last_name: Ge
orcid: 0000-0001-9381-3577
- first_name: Lilla
full_name: Koczka, Lilla
last_name: Koczka
- first_name: Ewa
full_name: Mazur, Ewa
last_name: Mazur
- first_name: Gergely
full_name: Molnar, Gergely
id: 34F1AF46-F248-11E8-B48F-1D18A9856A87
last_name: Molnar
- first_name: Dmitrii
full_name: Vladimirtsev, Dmitrii
id: 60466724-5355-11ee-ae5a-fa55e8f99c3d
last_name: Vladimirtsev
- first_name: Nada
full_name: Kassem, Nada
last_name: Kassem
- first_name: Sara
full_name: Ait Ikene, Sara
id: 6a0bb896-6bad-11f1-9bef-906e9eb76034
last_name: Ait Ikene
- first_name: Lukas
full_name: Fiedler, Lukas
id: 7c417475-8972-11ed-ae7b-8b674ca26986
last_name: Fiedler
- first_name: Jiří
full_name: Friml, Jiří
id: 4159519E-F248-11E8-B48F-1D18A9856A87
last_name: Friml
orcid: 0000-0002-8302-7596
citation:
ama: Ge Z, Koczka L, Mazur E, et al. MAKR6 integrates TMK and CAMEL/CANAR signalling
for auxin canalization in Arabidopsis. bioRxiv. doi:10.1101/2025.10.07.680881
apa: Ge, Z., Koczka, L., Mazur, E., Molnar, G., Vladimirtsev, D., Kassem, N., …
Friml, J. (n.d.). MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization
in Arabidopsis. bioRxiv. https://doi.org/10.1101/2025.10.07.680881
chicago: Ge, Zengxiang, Lilla Koczka, Ewa Mazur, Gergely Molnar, Dmitrii Vladimirtsev,
Nada Kassem, Sara Ait Ikene, Lukas Fiedler, and Jiří Friml. “MAKR6 Integrates
TMK and CAMEL/CANAR Signalling for Auxin Canalization in Arabidopsis.” BioRxiv,
n.d. https://doi.org/10.1101/2025.10.07.680881.
ieee: Z. Ge et al., “MAKR6 integrates TMK and CAMEL/CANAR signalling for
auxin canalization in Arabidopsis,” bioRxiv. .
ista: Ge Z, Koczka L, Mazur E, Molnar G, Vladimirtsev D, Kassem N, Ait Ikene S,
Fiedler L, Friml J. MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin
canalization in Arabidopsis. bioRxiv, 10.1101/2025.10.07.680881.
mla: Ge, Zengxiang, et al. “MAKR6 Integrates TMK and CAMEL/CANAR Signalling for
Auxin Canalization in Arabidopsis.” BioRxiv, doi:10.1101/2025.10.07.680881.
short: Z. Ge, L. Koczka, E. Mazur, G. Molnar, D. Vladimirtsev, N. Kassem, S. Ait
Ikene, L. Fiedler, J. Friml, BioRxiv (n.d.).
corr_author: '1'
date_created: 2026-06-13T16:57:07Z
date_published: 2026-05-30T00:00:00Z
date_updated: 2026-06-19T07:14:01Z
day: '30'
ddc:
- '580'
department:
- _id: GradSch
- _id: JiFr
doi: 10.1101/2025.10.07.680881
has_accepted_license: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1101/2025.10.07.680881
month: '05'
oa: 1
oa_version: Preprint
project:
- _id: 8f347782-16d5-11f0-9cad-8c19706ee739
grant_number: '101142681'
name: Cyclic nucleotides as second messengers in plants
- _id: bd76d395-d553-11ed-ba76-f678c14f9033
grant_number: I06123
name: Peptide receptors for auxin canalization in Arabidopsis
- _id: 7bcece63-9f16-11ee-852c-ae94e099eeb6
grant_number: P37051
name: Guanylate cyclase activity of TIR1/AFBs auxin receptors
publication: bioRxiv
publication_status: submitted
scopus_import: '1'
status: public
title: MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21998'
abstract:
- lang: eng
text: Little Red Dots (LRDs), among the most enigmatic high-redshift discoveries
by JWST, are commonly believed to be powered by accreting supermassive black holes.
Here, we explore the possibility that these sources are globular clusters in formation,
with rest-frame UV arising from a very young stellar population and rest-frame
optical from a short-lived supermassive (>104 M⊙) star. The spectral profiles
of LRDs are broadly consistent with this scenario, though the observed temperatures
and bolometric luminosities favor emission reprocessed by optically thick continuum-driven
winds not fully captured by current models. The LRD z ∼ 5−7 UV luminosity function
naturally evolves, under standard evolutionary and mass-loss prescriptions, into
a present-day mass function with a turnover at log10(M*/M⊙) = 5.3 and an exponential
cutoff at high masses, consistent with local globular cluster populations. We
estimate the total present-day number density of LRDs formed across all redshifts
to be ≈0.3 Mpc−3, similar within uncertainties to local globular clusters. The
observed LRD redshift range matches the age distribution of metal-poor globular
clusters, without current LRD counterparts to the metal-rich population. If LRDs
are globular clusters in formation, we predict chemical abundance patterns characteristic
of multiple stellar populations, including enhanced He and N, and potential Na–O
and Al–Mg anticorrelations. These results offer a local perspective to explore
this surprisingly abundant population of distant sources, and a potential new
window into extreme stellar astrophysics in the early Universe.
acknowledgement: "We thank the referees for detailed and highly constructive reports
that significantly improved the scope and breadth of the manuscript. J.C. thanks
Hollis Akins, Volker Bromm, Rui Chaves-Marques, Steve Finkelstein, Karl Gebhardt,
Keith Hawkins, Harley Katz, Stellar Offner, Daniel Schaerer, Grace Telford, and
Jorick Vink for conversations that improved the Letter. A.d.G. acknowledges support
from a Clay Fellowship awarded by the Smithsonian Astrophysical Observatory. M.B.K.
acknowledges support from NSF grants AST-2108962 and AST-2408247; NASA grant 80NSSC22K0827;
HST-GO-16686, HST-AR-17028, JWST-GO-03788, and JWST-AR-06278 from the Space Telescope
Science Institute, which is operated by AURA, Inc., under NASA contract NAS5-26555;
and from the Samuel T. and Fern Yanagisawa Regents Professorship in Astronomy at
UT Austin. A.A.C.S. acknowledges support by the Deutsche Forschungsgemeinschaft
(DFG, German Research Foundation) in the form of an Emmy Noether Research Group—Project-ID
445674056 (SA4064/1-1, PI Sander). A.A.C.S. further acknowledges support from the
Deutsches Zentrum für Luft und Raumfahrt (DLR) grant grants 50 OR 2509 (PI: A.A.C.
Sander) and 50 OR 2306 (PI: V. Ramachandran/A.A.C. Sander) as well as from the Federal
Ministry of Research, Technology, and Space (BMFTR) and the Baden-Württemberg Ministry
of Science as part of the Excellence Strategy of the German Federal and State Governments.
This project was cofunded by the European Union (Project 101183150—OCEANS).\r\n\r\nThis
work is based in part on observations made with the NASA/ESA/CSA James Webb Space
Telescope. The data were obtained from the Mikulski Archive for Space Telescopes
at the Space Telescope Science Institute, which is operated by the Association of
Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for
JWST. These observations are associated with programs 1180, 1181, 1208, 1212, 1213,
1215, 1286, 1345, 1433, 2198, 2561, 2750, 2767, 4106, 4233, 5105, 5224, 6368, and
6585."
article_number: L4
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: John
full_name: Chisholm, John
last_name: Chisholm
- first_name: Danielle A.
full_name: Berg, Danielle A.
last_name: Berg
- first_name: Michael
full_name: Boylan-Kolchin, Michael
last_name: Boylan-Kolchin
- first_name: Anna
full_name: De Graaff, Anna
last_name: De Graaff
- first_name: Lukas J.
full_name: Furtak, Lukas J.
last_name: Furtak
- first_name: Vasily
full_name: Kokorev, Vasily
last_name: Kokorev
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Julian B.
full_name: Muñoz, Julian B.
last_name: Muñoz
- first_name: Rohan P.
full_name: Naidu, Rohan P.
last_name: Naidu
- first_name: Andreas A.C.
full_name: Sander, Andreas A.C.
last_name: Sander
citation:
ama: Chisholm J, Berg DA, Boylan-Kolchin M, et al. Little Red Dots as globular clusters
in formation. The Astrophysical Journal Letters. 2026;1004(1). doi:10.3847/2041-8213/ae6dae
apa: Chisholm, J., Berg, D. A., Boylan-Kolchin, M., De Graaff, A., Furtak, L. J.,
Kokorev, V., … Sander, A. A. C. (2026). Little Red Dots as globular clusters in
formation. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae6dae
chicago: Chisholm, John, Danielle A. Berg, Michael Boylan-Kolchin, Anna De Graaff,
Lukas J. Furtak, Vasily Kokorev, Jorryt J Matthee, Julian B. Muñoz, Rohan P. Naidu,
and Andreas A.C. Sander. “Little Red Dots as Globular Clusters in Formation.”
The Astrophysical Journal Letters. IOP Publishing, 2026. https://doi.org/10.3847/2041-8213/ae6dae.
ieee: J. Chisholm et al., “Little Red Dots as globular clusters in formation,”
The Astrophysical Journal Letters, vol. 1004, no. 1. IOP Publishing, 2026.
ista: Chisholm J, Berg DA, Boylan-Kolchin M, De Graaff A, Furtak LJ, Kokorev V,
Matthee JJ, Muñoz JB, Naidu RP, Sander AAC. 2026. Little Red Dots as globular
clusters in formation. The Astrophysical Journal Letters. 1004(1), L4.
mla: Chisholm, John, et al. “Little Red Dots as Globular Clusters in Formation.”
The Astrophysical Journal Letters, vol. 1004, no. 1, L4, IOP Publishing,
2026, doi:10.3847/2041-8213/ae6dae.
short: J. Chisholm, D.A. Berg, M. Boylan-Kolchin, A. De Graaff, L.J. Furtak, V.
Kokorev, J.J. Matthee, J.B. Muñoz, R.P. Naidu, A.A.C. Sander, The Astrophysical
Journal Letters 1004 (2026).
date_created: 2026-06-14T22:01:42Z
date_published: 2026-06-10T00:00:00Z
date_updated: 2026-06-19T09:50:33Z
day: '10'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/2041-8213/ae6dae
external_id:
arxiv:
- '2602.15935'
file:
- access_level: open_access
checksum: 66949af6e620c8ef37de42688829a3e3
content_type: application/pdf
creator: dernst
date_created: 2026-06-19T09:45:21Z
date_updated: 2026-06-19T09:45:21Z
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file_name: 2026_AstrophysicalJourLetters_Chisholm.pdf
file_size: 919919
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success: 1
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intvolume: ' 1004'
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language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal Letters
publication_identifier:
eissn:
- 2041-8213
issn:
- 2041-8205
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Little Red Dots as globular clusters in formation
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 1004
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21997'
abstract:
- lang: eng
text: 'The massive binary common envelope (CE) phase plays a pivotal role in the
formation of close black hole (BH)/neutron star binaries, yet significant uncertainties
remain in our understanding of this process. In this study, we aim to constrain
the massive binary CE phase by systematically reconstructing three observed BH
X-ray binaries (BHXBs): GRO J1655-40, SAX J1819.3-2525, and 4U 1543-47. Through
comprehensive binary evolution simulations and parametric supernova modeling,
we establish lower limits for the CE efficiency parameters under different energy
considerations within the standard energy formalism. Specifically, we derive minimum
values for three cases: α0.5U and αU, representing CE efficiencies with half and
all of the internal energy contributing to the envelope ejection, respectively,
and αH, accounting for the envelope’s enthalpy. Our analysis reveals that the
self-consistent formation of these three BHXBs requires CE efficiency parameters
satisfying α0.5U ≳ 6.7, αU ≳ 4.2, and αH ≳ 1.7. Notably, we find no viable solutions
with CE efficiency values below unity, even when considering the most extreme
scenarios, in which the envelope binding energy is significantly reduced through
enthalpy inclusion. Our results strongly imply that either additional energy sources
are required or the formalism itself must be revised. Furthermore, we quantitatively
assess the impact of BH natal kicks on our results. A key finding is that 4U 1543-47’s
formation requires substantial natal kicks (≳50 km s−1), as lower kick velocities
are incompatible with isolated binary evolution.'
acknowledgement: We deeply thank the referee for a very careful reading and constructive
comments that have led to the improvement of the manuscript. The authors are grateful
to Poshak Gandhi for his valuable suggestions and feedback on this work. This work
is supported by the Natural Science Foundation of China (grant Nos. 12125303, 12525304,
12288102, 12473034, 12103028, 12333008, 12422305, 12090040/3, 12273105, 11703081,
11422324, 12073070, and 12173081), the CAS Project for Young Scientists in Basic
Research (YSBR-148), the Strategic Priority Research Program of the Chinese Academy
of Sciences (grant Nos. XDB1160303, XDB1160201, and XDB1160000), the National Key
R&D Program of China (grant Nos. 2021YFA1600403 and 2021YFA1600400), the Key Research
Program of Frontier Sciences of CAS (No. ZDBS-LY-7005), the “CAS Light of West China”,
the Yunnan Revitalization Talent Support Program-Science & Technology Champion Project
(No. 202305AB350003) and Young Talent Project, the International Centre of Supernovae
(ICESUN), Yunnan Key Laboratory of Supernova Research (Nos. 202302AN360001 and 202201BC070003),
Yunnan Fundamental Research Projects (No. 202401AT070139), and the Natural Science
Foundation of Henan Province (No. 242300420944). X.C. acknowledges the New Cornerstone
Science Foundation through the XPLORER PRIZE. The authors gratefully acknowledge
the “PHOENIX Supercomputing Platform” jointly operated by the Binary Population
Synthesis Group and the Stellar Astrophysics Group at Yunnan Observatories, Chinese
Academy of Sciences.
article_number: '31'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Zhenwei
full_name: Li, Zhenwei
last_name: Li
- first_name: Dandan
full_name: Wei, Dandan
id: 5dd129bd-0601-11ef-b325-833284687b76
last_name: Wei
- first_name: Shi
full_name: Jia, Shi
last_name: Jia
- first_name: Hailiang
full_name: Chen, Hailiang
last_name: Chen
- first_name: Hongwei
full_name: Ge, Hongwei
last_name: Ge
- first_name: Zhuo
full_name: Chen, Zhuo
last_name: Chen
- first_name: Yangyang
full_name: Zhang, Yangyang
last_name: Zhang
- first_name: Xuefei
full_name: Chen, Xuefei
last_name: Chen
- first_name: Zhanwen
full_name: Han, Zhanwen
last_name: Han
citation:
ama: 'Li Z, Wei D, Jia S, et al. A path to constraints on common envelope ejection
in massive binaries: Full evolutionary reconstruction of three Black Hole X-ray
binaries. The Astrophysical Journal. 2026;1004(1). doi:10.3847/1538-4357/ae66fd'
apa: 'Li, Z., Wei, D., Jia, S., Chen, H., Ge, H., Chen, Z., … Han, Z. (2026). A
path to constraints on common envelope ejection in massive binaries: Full evolutionary
reconstruction of three Black Hole X-ray binaries. The Astrophysical Journal.
IOP Publishing. https://doi.org/10.3847/1538-4357/ae66fd'
chicago: 'Li, Zhenwei, Dandan Wei, Shi Jia, Hailiang Chen, Hongwei Ge, Zhuo Chen,
Yangyang Zhang, Xuefei Chen, and Zhanwen Han. “A Path to Constraints on Common
Envelope Ejection in Massive Binaries: Full Evolutionary Reconstruction of Three
Black Hole X-Ray Binaries.” The Astrophysical Journal. IOP Publishing,
2026. https://doi.org/10.3847/1538-4357/ae66fd.'
ieee: 'Z. Li et al., “A path to constraints on common envelope ejection in
massive binaries: Full evolutionary reconstruction of three Black Hole X-ray binaries,”
The Astrophysical Journal, vol. 1004, no. 1. IOP Publishing, 2026.'
ista: 'Li Z, Wei D, Jia S, Chen H, Ge H, Chen Z, Zhang Y, Chen X, Han Z. 2026. A
path to constraints on common envelope ejection in massive binaries: Full evolutionary
reconstruction of three Black Hole X-ray binaries. The Astrophysical Journal.
1004(1), 31.'
mla: 'Li, Zhenwei, et al. “A Path to Constraints on Common Envelope Ejection in
Massive Binaries: Full Evolutionary Reconstruction of Three Black Hole X-Ray Binaries.”
The Astrophysical Journal, vol. 1004, no. 1, 31, IOP Publishing, 2026,
doi:10.3847/1538-4357/ae66fd.'
short: Z. Li, D. Wei, S. Jia, H. Chen, H. Ge, Z. Chen, Y. Zhang, X. Chen, Z. Han,
The Astrophysical Journal 1004 (2026).
date_created: 2026-06-14T22:01:42Z
date_published: 2026-06-10T00:00:00Z
date_updated: 2026-06-19T09:58:52Z
day: '10'
ddc:
- '520'
department:
- _id: YlGo
doi: 10.3847/1538-4357/ae66fd
external_id:
arxiv:
- '2604.10440'
file:
- access_level: open_access
checksum: bb76fbb51f8d2834cb79f19e7932e3bd
content_type: application/pdf
creator: dernst
date_created: 2026-06-19T09:56:29Z
date_updated: 2026-06-19T09:56:29Z
file_id: '22099'
file_name: 2026_AstrophysicalJour_Li.pdf
file_size: 3386217
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success: 1
file_date_updated: 2026-06-19T09:56:29Z
has_accepted_license: '1'
intvolume: ' 1004'
issue: '1'
language:
- iso: eng
month: '06'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'A path to constraints on common envelope ejection in massive binaries: Full
evolutionary reconstruction of three Black Hole X-ray binaries'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 1004
year: '2026'
...