---
_id: '9896'
abstract:
- lang: eng
text: Summary of the analysed genomes. (CSV 24 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 1 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808841.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 1 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808841.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 1 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808841.v1.
ieee: O. M. Sigalova et al., “Additional file 1 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 1 of Chlamydia pan-genomic analysis
reveals balance between host adaptation and selective pressure to genome reduction,
Springer Nature, 10.6084/m9.figshare.9808841.v1.
mla: Sigalova, Olga M., et al. Additional File 1 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808841.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T07:50:53Z
date_published: 2019-09-02T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '02'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808841.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808841.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808841.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 1 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '9897'
abstract:
- lang: eng
text: Frameshift and nonsense mutations near homopolymeric tracts of OG1 genes.
Only 374 genes with typical length and domain composition were considered. (CSV
6 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 20 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808850.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 20 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808850.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 20 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808850.v1.
ieee: O. M. Sigalova et al., “Additional file 20 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 20 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction, Springer Nature, 10.6084/m9.figshare.9808850.v1.
mla: Sigalova, Olga M., et al. Additional File 20 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808850.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T07:58:15Z
date_published: 2019-09-12T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '12'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808850.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808850.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808850.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 20 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '9898'
abstract:
- lang: eng
text: All polyN tracts of length 5 or more nucleotides in sequences of genes from
OG1. Sequences were extracted and scanned prior to automatic correction for frameshifts
implemented in the RAST pipeline. (CSV 133 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 21 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808859.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 21 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808859.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 21 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808859.v1.
ieee: O. M. Sigalova et al., “Additional file 21 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 21 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction, Springer Nature, 10.6084/m9.figshare.9808859.v1.
mla: Sigalova, Olga M., et al. Additional File 21 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808859.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T08:10:23Z
date_published: 2019-09-12T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '12'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808859.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808859.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808859.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 21 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '9899'
abstract:
- lang: eng
text: Summary of orthologous groups (OGs) for 227 genomes of genus Chlamydia. (CSV
362 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 2 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808865.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 2 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808865.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 2 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808865.v1.
ieee: O. M. Sigalova et al., “Additional file 2 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 2 of Chlamydia pan-genomic analysis
reveals balance between host adaptation and selective pressure to genome reduction,
Springer Nature, 10.6084/m9.figshare.9808865.v1.
mla: Sigalova, Olga M., et al. Additional File 2 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808865.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T08:18:09Z
date_published: 2019-09-12T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '12'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808865.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808865.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808865.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 2 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '9900'
abstract:
- lang: eng
text: Pan-genome statistics by species. (CSV 3 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 5 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808886.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 5 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808886.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 5 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808886.v1.
ieee: O. M. Sigalova et al., “Additional file 5 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 5 of Chlamydia pan-genomic analysis
reveals balance between host adaptation and selective pressure to genome reduction,
Springer Nature, 10.6084/m9.figshare.9808886.v1.
mla: Sigalova, Olga M., et al. Additional File 5 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808886.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T08:44:49Z
date_published: 2019-09-12T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '12'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808886.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808886.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808886.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 5 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '9901'
abstract:
- lang: eng
text: Clusters of Orthologous Genes (COGs) and corresponding functional categories
assigned to OGs. (CSV 117 kb)
article_processing_charge: No
author:
- first_name: Olga M.
full_name: Sigalova, Olga M.
last_name: Sigalova
- first_name: Andrei V.
full_name: Chaplin, Andrei V.
last_name: Chaplin
- first_name: Olga
full_name: Bochkareva, Olga
id: C4558D3C-6102-11E9-A62E-F418E6697425
last_name: Bochkareva
orcid: 0000-0003-1006-6639
- first_name: Pavel V.
full_name: Shelyakin, Pavel V.
last_name: Shelyakin
- first_name: Vsevolod A.
full_name: Filaretov, Vsevolod A.
last_name: Filaretov
- first_name: Evgeny E.
full_name: Akkuratov, Evgeny E.
last_name: Akkuratov
- first_name: Valentina
full_name: Burskaia, Valentina
last_name: Burskaia
- first_name: Mikhail S.
full_name: Gelfand, Mikhail S.
last_name: Gelfand
citation:
ama: Sigalova OM, Chaplin AV, Bochkareva O, et al. Additional file 9 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. 2019. doi:10.6084/m9.figshare.9808907.v1
apa: Sigalova, O. M., Chaplin, A. V., Bochkareva, O., Shelyakin, P. V., Filaretov,
V. A., Akkuratov, E. E., … Gelfand, M. S. (2019). Additional file 9 of Chlamydia
pan-genomic analysis reveals balance between host adaptation and selective pressure
to genome reduction. Springer Nature. https://doi.org/10.6084/m9.figshare.9808907.v1
chicago: Sigalova, Olga M., Andrei V. Chaplin, Olga Bochkareva, Pavel V. Shelyakin,
Vsevolod A. Filaretov, Evgeny E. Akkuratov, Valentina Burskaia, and Mikhail S.
Gelfand. “Additional File 9 of Chlamydia Pan-Genomic Analysis Reveals Balance
between Host Adaptation and Selective Pressure to Genome Reduction.” Springer
Nature, 2019. https://doi.org/10.6084/m9.figshare.9808907.v1.
ieee: O. M. Sigalova et al., “Additional file 9 of Chlamydia pan-genomic
analysis reveals balance between host adaptation and selective pressure to genome
reduction.” Springer Nature, 2019.
ista: Sigalova OM, Chaplin AV, Bochkareva O, Shelyakin PV, Filaretov VA, Akkuratov
EE, Burskaia V, Gelfand MS. 2019. Additional file 9 of Chlamydia pan-genomic analysis
reveals balance between host adaptation and selective pressure to genome reduction,
Springer Nature, 10.6084/m9.figshare.9808907.v1.
mla: Sigalova, Olga M., et al. Additional File 9 of Chlamydia Pan-Genomic Analysis
Reveals Balance between Host Adaptation and Selective Pressure to Genome Reduction.
Springer Nature, 2019, doi:10.6084/m9.figshare.9808907.v1.
short: O.M. Sigalova, A.V. Chaplin, O. Bochkareva, P.V. Shelyakin, V.A. Filaretov,
E.E. Akkuratov, V. Burskaia, M.S. Gelfand, (2019).
date_created: 2021-08-12T10:54:03Z
date_published: 2019-09-12T00:00:00Z
date_updated: 2026-04-03T09:39:41Z
day: '12'
department:
- _id: FyKo
doi: 10.6084/m9.figshare.9808907.v1
fulldoi: https://doi.org/10.6084/m9.figshare.9808907.v1
main_file_link:
- open_access: '1'
url: https://doi.org/10.6084/m9.figshare.9808907.v1
month: '09'
oa: 1
oa_version: Published Version
publisher: Springer Nature
related_material:
record:
- id: '6898'
relation: used_in_publication
status: public
status: public
title: Additional file 9 of Chlamydia pan-genomic analysis reveals balance between
host adaptation and selective pressure to genome reduction
type: research_data_reference
user_id: 6785fbc1-c503-11eb-8a32-93094b40e1cf
year: '2019'
...
---
_id: '319'
abstract:
- lang: eng
text: We study spaces of modelled distributions with singular behaviour near the
boundary of a domain that, in the context of the theory of regularity structures,
allow one to give robust solution theories for singular stochastic PDEs with boundary
conditions. The calculus of modelled distributions established in Hairer (Invent
Math 198(2):269–504, 2014. https://doi.org/10.1007/s00222-014-0505-4) is extended
to this setting. We formulate and solve fixed point problems in these spaces with
a class of kernels that is sufficiently large to cover in particular the Dirichlet
and Neumann heat kernels. These results are then used to provide solution theories
for the KPZ equation with Dirichlet and Neumann boundary conditions and for the
2D generalised parabolic Anderson model with Dirichlet boundary conditions. In
the case of the KPZ equation with Neumann boundary conditions, we show that, depending
on the class of mollifiers one considers, a “boundary renormalisation” takes place.
In other words, there are situations in which a certain boundary condition is
applied to an approximation to the KPZ equation, but the limiting process is the
Hopf–Cole solution to the KPZ equation with a different boundary condition.
acknowledgement: "MG thanks the support of the LMS Postdoctoral Mobility Grant.\r\n\r\n"
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Mate
full_name: Gerencser, Mate
id: 44ECEDF2-F248-11E8-B48F-1D18A9856A87
last_name: Gerencser
- first_name: Martin
full_name: Hairer, Martin
last_name: Hairer
citation:
ama: Gerencser M, Hairer M. Singular SPDEs in domains with boundaries. Probability
Theory and Related Fields. 2019;173(3-4):697–758. doi:10.1007/s00440-018-0841-1
apa: Gerencser, M., & Hairer, M. (2019). Singular SPDEs in domains with boundaries.
Probability Theory and Related Fields. Springer. https://doi.org/10.1007/s00440-018-0841-1
chicago: Gerencser, Mate, and Martin Hairer. “Singular SPDEs in Domains with Boundaries.”
Probability Theory and Related Fields. Springer, 2019. https://doi.org/10.1007/s00440-018-0841-1.
ieee: M. Gerencser and M. Hairer, “Singular SPDEs in domains with boundaries,” Probability
Theory and Related Fields, vol. 173, no. 3–4. Springer, pp. 697–758, 2019.
ista: Gerencser M, Hairer M. 2019. Singular SPDEs in domains with boundaries. Probability
Theory and Related Fields. 173(3–4), 697–758.
mla: Gerencser, Mate, and Martin Hairer. “Singular SPDEs in Domains with Boundaries.”
Probability Theory and Related Fields, vol. 173, no. 3–4, Springer, 2019,
pp. 697–758, doi:10.1007/s00440-018-0841-1.
short: M. Gerencser, M. Hairer, Probability Theory and Related Fields 173 (2019)
697–758.
corr_author: '1'
date_created: 2018-12-11T11:45:48Z
date_published: 2019-04-01T00:00:00Z
date_updated: 2026-04-03T09:45:34Z
day: '01'
ddc:
- '510'
department:
- _id: JaMa
doi: 10.1007/s00440-018-0841-1
external_id:
isi:
- '000463613800001'
file:
- access_level: open_access
checksum: 288d16ef7291242f485a9660979486e3
content_type: application/pdf
creator: dernst
date_created: 2018-12-17T16:25:24Z
date_updated: 2020-07-14T12:46:03Z
file_id: '5722'
file_name: 2018_ProbTheory_Gerencser.pdf
file_size: 893182
relation: main_file
file_date_updated: 2020-07-14T12:46:03Z
fulldoi: https://doi.org/10.1007/s00440-018-0841-1
has_accepted_license: '1'
intvolume: ' 173'
isi: 1
issue: 3-4
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
page: 697–758
project:
- _id: B67AFEDC-15C9-11EA-A837-991A96BB2854
name: IST Austria Open Access Fund
publication: Probability Theory and Related Fields
publication_identifier:
eissn:
- 1432-2064
issn:
- 0178-8051
publication_status: published
publisher: Springer
publist_id: '7546'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Singular SPDEs in domains with boundaries
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: ba8df636-2132-11f1-aed0-ed93e2281fdd
volume: 173
year: '2019'
...
---
_id: '405'
abstract:
- lang: eng
text: We investigate the quantum Jensen divergences from the viewpoint of joint
convexity. It turns out that the set of the functions which generate jointly convex
quantum Jensen divergences on positive matrices coincides with the Matrix Entropy
Class which has been introduced by Chen and Tropp quite recently.
acknowledgement: The author was supported by the ISTFELLOW program of the Institute
of Science and Technology Austria (project code IC1027FELL01) and partially supported
by the Hungarian National Research, Development and Innovation Office – NKFIH (grant
no. K124152)
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Daniel
full_name: Virosztek, Daniel
id: 48DB45DA-F248-11E8-B48F-1D18A9856A87
last_name: Virosztek
orcid: 0000-0003-1109-5511
citation:
ama: Virosztek D. Jointly convex quantum Jensen divergences. Linear Algebra and
Its Applications. 2019;576:67-78. doi:10.1016/j.laa.2018.03.002
apa: Virosztek, D. (2019). Jointly convex quantum Jensen divergences. Linear
Algebra and Its Applications. Elsevier. https://doi.org/10.1016/j.laa.2018.03.002
chicago: Virosztek, Daniel. “Jointly Convex Quantum Jensen Divergences.” Linear
Algebra and Its Applications. Elsevier, 2019. https://doi.org/10.1016/j.laa.2018.03.002.
ieee: D. Virosztek, “Jointly convex quantum Jensen divergences,” Linear Algebra
and Its Applications, vol. 576. Elsevier, pp. 67–78, 2019.
ista: Virosztek D. 2019. Jointly convex quantum Jensen divergences. Linear Algebra
and Its Applications. 576, 67–78.
mla: Virosztek, Daniel. “Jointly Convex Quantum Jensen Divergences.” Linear Algebra
and Its Applications, vol. 576, Elsevier, 2019, pp. 67–78, doi:10.1016/j.laa.2018.03.002.
short: D. Virosztek, Linear Algebra and Its Applications 576 (2019) 67–78.
corr_author: '1'
date_created: 2018-12-11T11:46:17Z
date_published: 2019-09-01T00:00:00Z
date_updated: 2025-04-15T06:50:00Z
day: '01'
department:
- _id: LaEr
doi: 10.1016/j.laa.2018.03.002
ec_funded: 1
external_id:
arxiv:
- '1712.05324'
isi:
- '000470955300005'
fulldoi: https://doi.org/10.1016/j.laa.2018.03.002
intvolume: ' 576'
isi: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1712.05324
month: '09'
oa: 1
oa_version: Preprint
page: 67-78
project:
- _id: 25681D80-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '291734'
name: International IST Postdoc Fellowship Programme
publication: Linear Algebra and Its Applications
publication_status: published
publisher: Elsevier
publist_id: '7424'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Jointly convex quantum Jensen divergences
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 576
year: '2019'
...
---
_id: '429'
abstract:
- lang: eng
text: We consider real symmetric or complex hermitian random matrices with correlated
entries. We prove local laws for the resolvent and universality of the local eigenvalue
statistics in the bulk of the spectrum. The correlations have fast decay but are
otherwise of general form. The key novelty is the detailed stability analysis
of the corresponding matrix valued Dyson equation whose solution is the deterministic
limit of the resolvent.
acknowledgement: "Open access funding provided by Institute of Science and Technology
(IST Austria).\r\n"
article_processing_charge: Yes (via OA deal)
article_type: original
author:
- first_name: Oskari H
full_name: Ajanki, Oskari H
id: 36F2FB7E-F248-11E8-B48F-1D18A9856A87
last_name: Ajanki
- first_name: László
full_name: Erdös, László
id: 4DBD5372-F248-11E8-B48F-1D18A9856A87
last_name: Erdös
orcid: 0000-0001-5366-9603
- first_name: Torben H
full_name: Krüger, Torben H
id: 3020C786-F248-11E8-B48F-1D18A9856A87
last_name: Krüger
orcid: 0000-0002-4821-3297
citation:
ama: Ajanki OH, Erdös L, Krüger TH. Stability of the matrix Dyson equation and random
matrices with correlations. Probability Theory and Related Fields. 2019;173(1-2):293–373.
doi:10.1007/s00440-018-0835-z
apa: Ajanki, O. H., Erdös, L., & Krüger, T. H. (2019). Stability of the matrix
Dyson equation and random matrices with correlations. Probability Theory and
Related Fields. Springer. https://doi.org/10.1007/s00440-018-0835-z
chicago: Ajanki, Oskari H, László Erdös, and Torben H Krüger. “Stability of the
Matrix Dyson Equation and Random Matrices with Correlations.” Probability Theory
and Related Fields. Springer, 2019. https://doi.org/10.1007/s00440-018-0835-z.
ieee: O. H. Ajanki, L. Erdös, and T. H. Krüger, “Stability of the matrix Dyson equation
and random matrices with correlations,” Probability Theory and Related Fields,
vol. 173, no. 1–2. Springer, pp. 293–373, 2019.
ista: Ajanki OH, Erdös L, Krüger TH. 2019. Stability of the matrix Dyson equation
and random matrices with correlations. Probability Theory and Related Fields.
173(1–2), 293–373.
mla: Ajanki, Oskari H., et al. “Stability of the Matrix Dyson Equation and Random
Matrices with Correlations.” Probability Theory and Related Fields, vol.
173, no. 1–2, Springer, 2019, pp. 293–373, doi:10.1007/s00440-018-0835-z.
short: O.H. Ajanki, L. Erdös, T.H. Krüger, Probability Theory and Related Fields
173 (2019) 293–373.
corr_author: '1'
date_created: 2018-12-11T11:46:25Z
date_published: 2019-02-01T00:00:00Z
date_updated: 2026-04-03T09:46:51Z
day: '01'
ddc:
- '510'
department:
- _id: LaEr
doi: 10.1007/s00440-018-0835-z
ec_funded: 1
external_id:
isi:
- '000459396500007'
file:
- access_level: open_access
checksum: f9354fa5c71f9edd17132588f0dc7d01
content_type: application/pdf
creator: dernst
date_created: 2018-12-17T16:12:08Z
date_updated: 2020-07-14T12:46:26Z
file_id: '5720'
file_name: 2018_ProbTheory_Ajanki.pdf
file_size: 1201840
relation: main_file
file_date_updated: 2020-07-14T12:46:26Z
fulldoi: https://doi.org/10.1007/s00440-018-0835-z
has_accepted_license: '1'
intvolume: ' 173'
isi: 1
issue: 1-2
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: 293–373
project:
- _id: 258DCDE6-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '338804'
name: Random matrices, universality and disordered quantum systems
- _id: B67AFEDC-15C9-11EA-A837-991A96BB2854
name: IST Austria Open Access Fund
publication: Probability Theory and Related Fields
publication_identifier:
eissn:
- 1432-2064
issn:
- 0178-8051
publication_status: published
publisher: Springer
publist_id: '7394'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Stability of the matrix Dyson equation and random matrices with correlations
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: ba8df636-2132-11f1-aed0-ed93e2281fdd
volume: 173
year: '2019'
...
---
_id: '17506'
abstract:
- lang: eng
text: Sandboxing is a common technique that allows low-level, untrusted components
to safely interact with trusted code. However, previous work has only investigated
the low-level memory isolation guarantees of sandboxing, leaving open the question
of the end-to-end guarantees that sandboxing affords programmers. In this paper,
we fill this gap by showing that sandboxing enables reasoning about the known
concept of robust safety, i.e., safety of the trusted code even in the presence
of arbitrary untrusted code. To do this, we first present an idealized operational
semantics for a language that combines trusted code with untrusted code. Sandboxing
is built into our semantics. Then, we prove that safety properties of the trusted
code (as enforced through a rich type system) are upheld in the presence of arbitrary
untrusted code, so long as all interactions with untrusted code occur at the “any”
type (a type inhabited by all values). Finally, to alleviate the burden of having
to interact with untrusted code at only the “any” type, we formalize and prove
safe several wrappers, which automatically convert values between the “any” type
and much richer types. All our results are mechanized in the Coq proof assistant.
article_processing_charge: No
article_type: original
author:
- first_name: Michael Joachim
full_name: Sammler, Michael Joachim
id: 510d3901-2a03-11ee-914d-d9ae9011f0a7
last_name: Sammler
- first_name: Deepak
full_name: Garg, Deepak
last_name: Garg
- first_name: Derek
full_name: Dreyer, Derek
last_name: Dreyer
- first_name: Tadeusz
full_name: Litak, Tadeusz
last_name: Litak
citation:
ama: Sammler MJ, Garg D, Dreyer D, Litak T. The high-level benefits of low-level
sandboxing. Proceedings of the ACM on Programming Languages. 2019;4(POPL):1-32.
doi:10.1145/3371100
apa: Sammler, M. J., Garg, D., Dreyer, D., & Litak, T. (2019). The high-level
benefits of low-level sandboxing. Proceedings of the ACM on Programming Languages.
Association for Computing Machinery. https://doi.org/10.1145/3371100
chicago: Sammler, Michael Joachim, Deepak Garg, Derek Dreyer, and Tadeusz Litak.
“The High-Level Benefits of Low-Level Sandboxing.” Proceedings of the ACM on
Programming Languages. Association for Computing Machinery, 2019. https://doi.org/10.1145/3371100.
ieee: M. J. Sammler, D. Garg, D. Dreyer, and T. Litak, “The high-level benefits
of low-level sandboxing,” Proceedings of the ACM on Programming Languages,
vol. 4, no. POPL. Association for Computing Machinery, pp. 1–32, 2019.
ista: Sammler MJ, Garg D, Dreyer D, Litak T. 2019. The high-level benefits of low-level
sandboxing. Proceedings of the ACM on Programming Languages. 4(POPL), 1–32.
mla: Sammler, Michael Joachim, et al. “The High-Level Benefits of Low-Level Sandboxing.”
Proceedings of the ACM on Programming Languages, vol. 4, no. POPL, Association
for Computing Machinery, 2019, pp. 1–32, doi:10.1145/3371100.
short: M.J. Sammler, D. Garg, D. Dreyer, T. Litak, Proceedings of the ACM on Programming
Languages 4 (2019) 1–32.
date_created: 2024-09-05T08:36:52Z
date_published: 2019-12-20T00:00:00Z
date_updated: 2024-09-10T09:58:57Z
day: '20'
doi: 10.1145/3371100
extern: '1'
fulldoi: https://doi.org/10.1145/3371100
intvolume: ' 4'
issue: POPL
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1145/3371100
month: '12'
oa: 1
oa_version: Published Version
page: 1-32
publication: Proceedings of the ACM on Programming Languages
publication_identifier:
issn:
- 2475-1421
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: The high-level benefits of low-level sandboxing
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 4
year: '2019'
...
---
_id: '17510'
abstract:
- lang: eng
text: Weak lensing surveys are reaching sensitivities at which uncertainties in
the galaxy redshift distributions n(z) from photo-z errors degrade cosmological
constraints. We use ray-tracing simulations and a simple treatment of photo-z
errors to assess cosmological parameter biases from uncertainties in n(z) in an
LSST-like survey. We use lensing peak counts and the power spectrum to infer cosmological
parameters, and find that the latter is somewhat more resilient to photo-z errors.
We place conservative lower limits on the survey size at which different types
of photo-z errors significantly degrade (${\sim }50{{\ \rm per\ cent}}$) ΛCDM
(cold dark matter, wCDM) parameter constraints. A residual constant photo-z bias
of |δz| < 0.003(1 + z), the current LSST requirement, does not significantly
degrade surveys smaller than ≈1300 (≈490) deg2 using peaks and ≈6500 (≈4900) deg2
using the power spectrum. Surveys smaller than ≈920 (≈450) deg2 and ≈4600 (≈4000)
deg2 avoid 25 per cent degradation. Adopting a recent prediction for LSST’s full
photo-z probability distribution function (PDF), we find that simply approximating
n(z) with the photo-z galaxy distribution computed from this PDF significantly
degrades surveys as small as ≈60 (≈65) deg2 using peaks or the power spectrum.
If the centroid bias in each tomographic bin is removed from the photo-z galaxy
distribution, using peaks or the power spectrum still significantly degrades surveys
larger than ≈200 (≈255) or ≈248 (≈315) deg2; 25 per cent degradations occur at
survey sizes of ≈140 (≈180) deg2 or ≈165 (≈210) deg2. These results imply that
the expected broad photo-z PDF significantly biases parameters, which must be
further mitigated using more sophisticated photo-z treatments.
article_processing_charge: No
article_type: original
author:
- first_name: Matthew W
full_name: Abruzzo, Matthew W
last_name: Abruzzo
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Abruzzo MW, Haiman Z. The impact of photometric redshift errors on lensing
statistics in ray-tracing simulations. Monthly Notices of the Royal Astronomical
Society. 2019;486(2):2730-2753. doi:10.1093/mnras/stz1016
apa: Abruzzo, M. W., & Haiman, Z. (2019). The impact of photometric redshift
errors on lensing statistics in ray-tracing simulations. Monthly Notices of
the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stz1016
chicago: Abruzzo, Matthew W, and Zoltán Haiman. “The Impact of Photometric Redshift
Errors on Lensing Statistics in Ray-Tracing Simulations.” Monthly Notices of
the Royal Astronomical Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz1016.
ieee: M. W. Abruzzo and Z. Haiman, “The impact of photometric redshift errors on
lensing statistics in ray-tracing simulations,” Monthly Notices of the Royal
Astronomical Society, vol. 486, no. 2. Oxford University Press, pp. 2730–2753,
2019.
ista: Abruzzo MW, Haiman Z. 2019. The impact of photometric redshift errors on lensing
statistics in ray-tracing simulations. Monthly Notices of the Royal Astronomical
Society. 486(2), 2730–2753.
mla: Abruzzo, Matthew W., and Zoltán Haiman. “The Impact of Photometric Redshift
Errors on Lensing Statistics in Ray-Tracing Simulations.” Monthly Notices of
the Royal Astronomical Society, vol. 486, no. 2, Oxford University Press,
2019, pp. 2730–53, doi:10.1093/mnras/stz1016.
short: M.W. Abruzzo, Z. Haiman, Monthly Notices of the Royal Astronomical Society
486 (2019) 2730–2753.
date_created: 2024-09-05T08:49:24Z
date_published: 2019-04-18T00:00:00Z
date_updated: 2024-09-10T12:49:04Z
day: '18'
doi: 10.1093/mnras/stz1016
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/stz1016
intvolume: ' 486'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stz1016
month: '04'
oa: 1
oa_version: Published Version
page: 2730-2753
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: The impact of photometric redshift errors on lensing statistics in ray-tracing
simulations
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 486
year: '2019'
...
---
_id: '17511'
article_number: '019'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Gabriela A.
full_name: Marques, Gabriela A.
last_name: Marques
- first_name: Jia
full_name: Liu, Jia
last_name: Liu
- first_name: José Manuel Zorrilla
full_name: Matilla, José Manuel Zorrilla
last_name: Matilla
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Armando
full_name: Bernui, Armando
last_name: Bernui
- first_name: Camila P.
full_name: Novaes, Camila P.
last_name: Novaes
citation:
ama: Marques GA, Liu J, Matilla JMZ, Haiman Z, Bernui A, Novaes CP. Constraining
neutrino mass with weak lensing Minkowski Functionals. Journal of Cosmology
and Astroparticle Physics. 2019;2019(06). doi:10.1088/1475-7516/2019/06/019
apa: Marques, G. A., Liu, J., Matilla, J. M. Z., Haiman, Z., Bernui, A., & Novaes,
C. P. (2019). Constraining neutrino mass with weak lensing Minkowski Functionals.
Journal of Cosmology and Astroparticle Physics. IOP Publishing. https://doi.org/10.1088/1475-7516/2019/06/019
chicago: Marques, Gabriela A., Jia Liu, José Manuel Zorrilla Matilla, Zoltán Haiman,
Armando Bernui, and Camila P. Novaes. “Constraining Neutrino Mass with Weak Lensing
Minkowski Functionals.” Journal of Cosmology and Astroparticle Physics.
IOP Publishing, 2019. https://doi.org/10.1088/1475-7516/2019/06/019.
ieee: G. A. Marques, J. Liu, J. M. Z. Matilla, Z. Haiman, A. Bernui, and C. P. Novaes,
“Constraining neutrino mass with weak lensing Minkowski Functionals,” Journal
of Cosmology and Astroparticle Physics, vol. 2019, no. 06. IOP Publishing,
2019.
ista: Marques GA, Liu J, Matilla JMZ, Haiman Z, Bernui A, Novaes CP. 2019. Constraining
neutrino mass with weak lensing Minkowski Functionals. Journal of Cosmology and
Astroparticle Physics. 2019(06), 019.
mla: Marques, Gabriela A., et al. “Constraining Neutrino Mass with Weak Lensing
Minkowski Functionals.” Journal of Cosmology and Astroparticle Physics,
vol. 2019, no. 06, 019, IOP Publishing, 2019, doi:10.1088/1475-7516/2019/06/019.
short: G.A. Marques, J. Liu, J.M.Z. Matilla, Z. Haiman, A. Bernui, C.P. Novaes,
Journal of Cosmology and Astroparticle Physics 2019 (2019).
date_created: 2024-09-05T08:50:20Z
date_published: 2019-06-07T00:00:00Z
date_updated: 2024-09-10T13:10:34Z
day: '07'
doi: 10.1088/1475-7516/2019/06/019
extern: '1'
external_id:
arxiv:
- '1812.08206'
fulldoi: https://doi.org/10.1088/1475-7516/2019/06/019
intvolume: ' 2019'
issue: '06'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1812.08206'
month: '06'
oa: 1
oa_version: Preprint
publication: Journal of Cosmology and Astroparticle Physics
publication_identifier:
issn:
- 1475-7516
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Constraining neutrino mass with weak lensing Minkowski Functionals
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 2019
year: '2019'
...
---
_id: '17512'
abstract:
- lang: eng
text: 'The localization of stellar-mass binary black hole mergers using gravitational
waves is critical in understanding the properties of the binaries’ host galaxies,
observing possible electromagnetic emission from the mergers, or using them as
a cosmological distance ladder. The precision of this localization can be substantially
increased with prior astrophysical information about the binary system. In particular,
constraining the inclination of the binary can reduce the distance uncertainty
of the source. Here, we present the first realistic set of localizations for binary
black hole mergers, including different prior constraints on the binaries’ inclinations.
We find that prior information on the inclination can reduce the localization
volume by a factor of 3. We discuss two astrophysical scenarios of interest: (i)
follow-up searches for beamed electromagnetic/neutrino counterparts and (ii) mergers
in the accretion discs of active galactic nuclei.'
article_processing_charge: No
article_type: original
author:
- first_name: K Rainer
full_name: Corley, K Rainer
last_name: Corley
- first_name: Imre
full_name: Bartos, Imre
last_name: Bartos
- first_name: Leo P
full_name: Singer, Leo P
last_name: Singer
- first_name: Andrew R
full_name: Williamson, Andrew R
last_name: Williamson
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Bence
full_name: Kocsis, Bence
last_name: Kocsis
- first_name: Samaya
full_name: Nissanke, Samaya
last_name: Nissanke
- first_name: Zsuzsa
full_name: Márka, Zsuzsa
last_name: Márka
- first_name: Szabolcs
full_name: Márka, Szabolcs
last_name: Márka
citation:
ama: Corley KR, Bartos I, Singer LP, et al. Localization of binary black hole mergers
with known inclination. Monthly Notices of the Royal Astronomical Society.
2019;488(3):4459-4463. doi:10.1093/mnras/stz2072
apa: Corley, K. R., Bartos, I., Singer, L. P., Williamson, A. R., Haiman, Z., Kocsis,
B., … Márka, S. (2019). Localization of binary black hole mergers with known inclination.
Monthly Notices of the Royal Astronomical Society. Oxford University Press.
https://doi.org/10.1093/mnras/stz2072
chicago: Corley, K Rainer, Imre Bartos, Leo P Singer, Andrew R Williamson, Zoltán
Haiman, Bence Kocsis, Samaya Nissanke, Zsuzsa Márka, and Szabolcs Márka. “Localization
of Binary Black Hole Mergers with Known Inclination.” Monthly Notices of the
Royal Astronomical Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz2072.
ieee: K. R. Corley et al., “Localization of binary black hole mergers with
known inclination,” Monthly Notices of the Royal Astronomical Society,
vol. 488, no. 3. Oxford University Press, pp. 4459–4463, 2019.
ista: Corley KR, Bartos I, Singer LP, Williamson AR, Haiman Z, Kocsis B, Nissanke
S, Márka Z, Márka S. 2019. Localization of binary black hole mergers with known
inclination. Monthly Notices of the Royal Astronomical Society. 488(3), 4459–4463.
mla: Corley, K. Rainer, et al. “Localization of Binary Black Hole Mergers with Known
Inclination.” Monthly Notices of the Royal Astronomical Society, vol. 488,
no. 3, Oxford University Press, 2019, pp. 4459–63, doi:10.1093/mnras/stz2072.
short: K.R. Corley, I. Bartos, L.P. Singer, A.R. Williamson, Z. Haiman, B. Kocsis,
S. Nissanke, Z. Márka, S. Márka, Monthly Notices of the Royal Astronomical Society
488 (2019) 4459–4463.
date_created: 2024-09-05T08:51:22Z
date_published: 2019-07-30T00:00:00Z
date_updated: 2024-09-10T13:26:28Z
day: '30'
doi: 10.1093/mnras/stz2072
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/stz2072
intvolume: ' 488'
issue: '3'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stz2072
month: '07'
oa: 1
oa_version: Published Version
page: 4459-4463
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Localization of binary black hole mergers with known inclination
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 488
year: '2019'
...
---
_id: '17530'
abstract:
- lang: eng
text: Based on the cosmic shear data from the Canada-France-Hawaii Telescope Lensing
Survey (CFHTLenS), Kilbinger et al. (2013) obtained a constraint on the amplitude
of matter fluctuations of σ8(Ωm/0.27)0.6=0.79±0.03 from the two-point correlation
function (2PCF). This is ≈3σ lower than the value 0.89±0.01 derived from Planck
data on cosmic microwave background (CMB) anisotropies. On the other hand, based
on the same CFHTLenS data, but using the power spectrum, and performing a different
analysis, Liu et al. (2015) obtained the higher value of σ8(Ωm/0.27)0.64=0.87+0.05−0.06.
We here investigate the origin of this difference, by performing a fair side-by-side
comparison of the 2PCF and power spectrum analyses on CFHTLenS data. We find that
these two statistics indeed deliver different results, even when applied to the
same data in an otherwise identical procedure. We identify excess power in the
data on small scales (ℓ>5,000) driving the larger values inferred from the power
spectrum. We speculate on the possible origin of this excess small-scale power.
More generally, our results highlight the utility of analysing the 2PCF and the
power spectrum in tandem, to discover (and to help control) systematic errors.
article_processing_charge: No
article_type: original
author:
- first_name: Tianhuan
full_name: Lu, Tianhuan
last_name: Lu
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Lu T, Haiman Z. The matter fluctuation amplitude inferred from the weak lensing
power spectrum and correlation function in CFHTLenS data. Monthly Notices of
the Royal Astronomical Society. 2019;490(4):5033-5042. doi:10.1093/mnras/stz2931
apa: Lu, T., & Haiman, Z. (2019). The matter fluctuation amplitude inferred
from the weak lensing power spectrum and correlation function in CFHTLenS data.
Monthly Notices of the Royal Astronomical Society. Oxford University Press.
https://doi.org/10.1093/mnras/stz2931
chicago: Lu, Tianhuan, and Zoltán Haiman. “The Matter Fluctuation Amplitude Inferred
from the Weak Lensing Power Spectrum and Correlation Function in CFHTLenS Data.”
Monthly Notices of the Royal Astronomical Society. Oxford University Press,
2019. https://doi.org/10.1093/mnras/stz2931.
ieee: T. Lu and Z. Haiman, “The matter fluctuation amplitude inferred from the weak
lensing power spectrum and correlation function in CFHTLenS data,” Monthly
Notices of the Royal Astronomical Society, vol. 490, no. 4. Oxford University
Press, pp. 5033–5042, 2019.
ista: Lu T, Haiman Z. 2019. The matter fluctuation amplitude inferred from the weak
lensing power spectrum and correlation function in CFHTLenS data. Monthly Notices
of the Royal Astronomical Society. 490(4), 5033–5042.
mla: Lu, Tianhuan, and Zoltán Haiman. “The Matter Fluctuation Amplitude Inferred
from the Weak Lensing Power Spectrum and Correlation Function in CFHTLenS Data.”
Monthly Notices of the Royal Astronomical Society, vol. 490, no. 4, Oxford
University Press, 2019, pp. 5033–42, doi:10.1093/mnras/stz2931.
short: T. Lu, Z. Haiman, Monthly Notices of the Royal Astronomical Society 490 (2019)
5033–5042.
date_created: 2024-09-05T09:37:20Z
date_published: 2019-10-18T00:00:00Z
date_updated: 2024-09-11T08:01:58Z
day: '18'
doi: 10.1093/mnras/stz2931
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/stz2931
intvolume: ' 490'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stz2931
month: '10'
oa: 1
oa_version: Published Version
page: 5033-5042
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1093/mnras/stad1748
scopus_import: '1'
status: public
title: The matter fluctuation amplitude inferred from the weak lensing power spectrum
and correlation function in CFHTLenS data
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 490
year: '2019'
...
---
_id: '17533'
abstract:
- lang: eng
text: "The origins of the stellar-mass black hole mergers discovered by LIGO/Virgo
are still unknown. Here we show that if migration traps develop in the accretion
disks of active galactic nuclei (AGNs) and promote the mergers of their captive
black holes, the majority of black holes within disks will undergo hierarchical
mergers—with one of the black holes being the remnant of a previous merger. 40%
of AGN-assisted mergers detected by LIGO/Virgo will include a black hole with
mass ≳50\U0001D440⊙, the mass limit from stellar core collapse. Hierarchical
mergers at traps in AGNs will exhibit black hole spins (anti)aligned with the
binary’s orbital axis, a distinct property from other hierarchical channels. Our
results suggest, although not definitively (with odds ratio of ∼1), that LIGO’s
heaviest merger so far, GW170729, could have originated from this channel."
article_number: '181101'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Y.
full_name: Yang, Y.
last_name: Yang
- first_name: I.
full_name: Bartos, I.
last_name: Bartos
- first_name: V.
full_name: Gayathri, V.
last_name: Gayathri
- first_name: K. E. S.
full_name: Ford, K. E. S.
last_name: Ford
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: S.
full_name: Klimenko, S.
last_name: Klimenko
- first_name: B.
full_name: Kocsis, B.
last_name: Kocsis
- first_name: S.
full_name: Márka, S.
last_name: Márka
- first_name: Z.
full_name: Márka, Z.
last_name: Márka
- first_name: B.
full_name: McKernan, B.
last_name: McKernan
- first_name: R.
full_name: O’Shaughnessy, R.
last_name: O’Shaughnessy
citation:
ama: Yang Y, Bartos I, Gayathri V, et al. Hierarchical black hole mergers in active
galactic nuclei. Physical Review Letters. 2019;123(18). doi:10.1103/physrevlett.123.181101
apa: Yang, Y., Bartos, I., Gayathri, V., Ford, K. E. S., Haiman, Z., Klimenko, S.,
… O’Shaughnessy, R. (2019). Hierarchical black hole mergers in active galactic
nuclei. Physical Review Letters. American Physical Society. https://doi.org/10.1103/physrevlett.123.181101
chicago: Yang, Y., I. Bartos, V. Gayathri, K. E. S. Ford, Zoltán Haiman, S. Klimenko,
B. Kocsis, et al. “Hierarchical Black Hole Mergers in Active Galactic Nuclei.”
Physical Review Letters. American Physical Society, 2019. https://doi.org/10.1103/physrevlett.123.181101.
ieee: Y. Yang et al., “Hierarchical black hole mergers in active galactic
nuclei,” Physical Review Letters, vol. 123, no. 18. American Physical Society,
2019.
ista: Yang Y, Bartos I, Gayathri V, Ford KES, Haiman Z, Klimenko S, Kocsis B, Márka
S, Márka Z, McKernan B, O’Shaughnessy R. 2019. Hierarchical black hole mergers
in active galactic nuclei. Physical Review Letters. 123(18), 181101.
mla: Yang, Y., et al. “Hierarchical Black Hole Mergers in Active Galactic Nuclei.”
Physical Review Letters, vol. 123, no. 18, 181101, American Physical Society,
2019, doi:10.1103/physrevlett.123.181101.
short: Y. Yang, I. Bartos, V. Gayathri, K.E.S. Ford, Z. Haiman, S. Klimenko, B.
Kocsis, S. Márka, Z. Márka, B. McKernan, R. O’Shaughnessy, Physical Review Letters
123 (2019).
date_created: 2024-09-05T09:39:53Z
date_published: 2019-11-01T00:00:00Z
date_updated: 2024-09-11T14:39:29Z
day: '1'
doi: 10.1103/physrevlett.123.181101
extern: '1'
external_id:
arxiv:
- '1906.09281'
fulldoi: https://doi.org/10.1103/physrevlett.123.181101
intvolume: ' 123'
issue: '18'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1906.09281'
month: '11'
oa: 1
oa_version: Preprint
publication: Physical Review Letters
publication_identifier:
issn:
- 0031-9007
- 1079-7114
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Hierarchical black hole mergers in active galactic nuclei
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 123
year: '2019'
...
---
_id: '17541'
abstract:
- lang: eng
text: 'In recent years, the discovery of massive quasars at z~7 has provided a striking
challenge to our understanding of the origin and growth of supermassive black
holes in the early Universe. Mounting observational and theoretical evidence indicates
the viability of massive seeds, formed by the collapse of supermassive stars,
as a progenitor model for such early, massive accreting black holes. Although
considerable progress has been made in our theoretical understanding, many questions
remain regarding how (and how often) such objects may form, how they live and
die, and how next generation observatories may yield new insight into the origin
of these primordial titans. This review focusses on our present understanding
of this remarkable formation scenario, based on discussions held at the Monash
Prato Centre from November 20--24, 2017, during the workshop "Titans of the Early
Universe: The Origin of the First Supermassive Black Holes."'
article_number: e027
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Tyrone E.
full_name: Woods, Tyrone E.
last_name: Woods
- first_name: Bhaskar
full_name: Agarwal, Bhaskar
last_name: Agarwal
- first_name: Volker
full_name: Bromm, Volker
last_name: Bromm
- first_name: Andrew
full_name: Bunker, Andrew
last_name: Bunker
- first_name: Ke-Jung
full_name: Chen, Ke-Jung
last_name: Chen
- first_name: Sunmyon
full_name: Chon, Sunmyon
last_name: Chon
- first_name: Andrea
full_name: Ferrara, Andrea
last_name: Ferrara
- first_name: Simon C. O.
full_name: Glover, Simon C. O.
last_name: Glover
- first_name: Lionel
full_name: Haemmerlé, Lionel
last_name: Haemmerlé
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Tilman
full_name: Hartwig, Tilman
last_name: Hartwig
- first_name: Alexander
full_name: Heger, Alexander
last_name: Heger
- first_name: Shingo
full_name: Hirano, Shingo
last_name: Hirano
- first_name: Takashi
full_name: Hosokawa, Takashi
last_name: Hosokawa
- first_name: Kohei
full_name: Inayoshi, Kohei
last_name: Inayoshi
- first_name: Ralf S.
full_name: Klessen, Ralf S.
last_name: Klessen
- first_name: Chiaki
full_name: Kobayashi, Chiaki
last_name: Kobayashi
- first_name: Filippos
full_name: Koliopanos, Filippos
last_name: Koliopanos
- first_name: Muhammad A.
full_name: Latif, Muhammad A.
last_name: Latif
- first_name: Yuexing
full_name: Li, Yuexing
last_name: Li
- first_name: Lucio
full_name: Mayer, Lucio
last_name: Mayer
- first_name: Mar
full_name: Mezcua, Mar
last_name: Mezcua
- first_name: Priyamvada
full_name: Natarajan, Priyamvada
last_name: Natarajan
- first_name: Fabio
full_name: Pacucci, Fabio
last_name: Pacucci
- first_name: Martin J.
full_name: Rees, Martin J.
last_name: Rees
- first_name: John A.
full_name: Regan, John A.
last_name: Regan
- first_name: Yuya
full_name: Sakurai, Yuya
last_name: Sakurai
- first_name: Stefania
full_name: Salvadori, Stefania
last_name: Salvadori
- first_name: Raffaella
full_name: Schneider, Raffaella
last_name: Schneider
- first_name: Marco
full_name: Surace, Marco
last_name: Surace
- first_name: Takamitsu L.
full_name: Tanaka, Takamitsu L.
last_name: Tanaka
- first_name: Daniel J.
full_name: Whalen, Daniel J.
last_name: Whalen
- first_name: Naoki
full_name: Yoshida, Naoki
last_name: Yoshida
citation:
ama: 'Woods TE, Agarwal B, Bromm V, et al. Titans of the early universe: The prato
statement on the origin of the first supermassive black holes. Publications
of the Astronomical Society of Australia. 2019;36. doi:10.1017/pasa.2019.14'
apa: 'Woods, T. E., Agarwal, B., Bromm, V., Bunker, A., Chen, K.-J., Chon, S., …
Yoshida, N. (2019). Titans of the early universe: The prato statement on the origin
of the first supermassive black holes. Publications of the Astronomical Society
of Australia. Cambridge University Press. https://doi.org/10.1017/pasa.2019.14'
chicago: 'Woods, Tyrone E., Bhaskar Agarwal, Volker Bromm, Andrew Bunker, Ke-Jung
Chen, Sunmyon Chon, Andrea Ferrara, et al. “Titans of the Early Universe: The
Prato Statement on the Origin of the First Supermassive Black Holes.” Publications
of the Astronomical Society of Australia. Cambridge University Press, 2019.
https://doi.org/10.1017/pasa.2019.14.'
ieee: 'T. E. Woods et al., “Titans of the early universe: The prato statement
on the origin of the first supermassive black holes,” Publications of the Astronomical
Society of Australia, vol. 36. Cambridge University Press, 2019.'
ista: 'Woods TE, Agarwal B, Bromm V, Bunker A, Chen K-J, Chon S, Ferrara A, Glover
SCO, Haemmerlé L, Haiman Z, Hartwig T, Heger A, Hirano S, Hosokawa T, Inayoshi
K, Klessen RS, Kobayashi C, Koliopanos F, Latif MA, Li Y, Mayer L, Mezcua M, Natarajan
P, Pacucci F, Rees MJ, Regan JA, Sakurai Y, Salvadori S, Schneider R, Surace M,
Tanaka TL, Whalen DJ, Yoshida N. 2019. Titans of the early universe: The prato
statement on the origin of the first supermassive black holes. Publications of
the Astronomical Society of Australia. 36, e027.'
mla: 'Woods, Tyrone E., et al. “Titans of the Early Universe: The Prato Statement
on the Origin of the First Supermassive Black Holes.” Publications of the Astronomical
Society of Australia, vol. 36, e027, Cambridge University Press, 2019, doi:10.1017/pasa.2019.14.'
short: T.E. Woods, B. Agarwal, V. Bromm, A. Bunker, K.-J. Chen, S. Chon, A. Ferrara,
S.C.O. Glover, L. Haemmerlé, Z. Haiman, T. Hartwig, A. Heger, S. Hirano, T. Hosokawa,
K. Inayoshi, R.S. Klessen, C. Kobayashi, F. Koliopanos, M.A. Latif, Y. Li, L.
Mayer, M. Mezcua, P. Natarajan, F. Pacucci, M.J. Rees, J.A. Regan, Y. Sakurai,
S. Salvadori, R. Schneider, M. Surace, T.L. Tanaka, D.J. Whalen, N. Yoshida, Publications
of the Astronomical Society of Australia 36 (2019).
date_created: 2024-09-05T09:57:20Z
date_published: 2019-08-06T00:00:00Z
date_updated: 2024-09-12T13:20:41Z
day: '06'
doi: 10.1017/pasa.2019.14
extern: '1'
external_id:
arxiv:
- '1810.12310'
fulldoi: https://doi.org/10.1017/pasa.2019.14
intvolume: ' 36'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1810.12310'
month: '08'
oa: 1
oa_version: Preprint
publication: Publications of the Astronomical Society of Australia
publication_identifier:
issn:
- 1323-3580
- 1448-6083
publication_status: published
publisher: Cambridge University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Titans of the early universe: The prato statement on the origin of the first
supermassive black holes'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 36
year: '2019'
...
---
_id: '17543'
abstract:
- lang: eng
text: 'Massive black-hole (MBH) binaries, which are expected to form following the
merger of their parent galaxies, produce gravitational waves which will be detectable
by Pulsar Timing Arrays at nanohertz frequencies (year periods). While no confirmed,
compact MBH binary systems have been seen in electromagnetic observations, a large
number of candidates have recently been identified in optical surveys of AGN variability.
Using a combination of cosmological, hydrodynamic simulations; comprehensive,
semi-analytic binary merger models; and analytic AGN spectra and variability prescriptions;
we calculate the expected electromagnetic detection rates of MBH binaries as periodically
variable AGN. In particular, we consider two independent variability models: (i)
Doppler boosting due to large orbital velocities, and (ii) hydrodynamic variability
in which the fueling of MBH accretion disks is periodically modulated by the companion.
Our models predict that numerous MBH binaries should be present and distinguishable
in the existing data. In particular, our fiducial models produce an expectation
value of 0.2 (Doppler) and 5 (hydrodynamic) binaries to be identifiable in CRTS,
while 20 and 100 are expected after five years of LSST observations. The brightness
variations in most systems are too small to be distinguishable, but almost 1%
of AGN at redshifts z≲0.6 could be in massive binaries. We analyze the predicted
binary parameters of observable systems and their selection biases, and include
an extensive discussion of our model parameters and uncertainties.'
article_processing_charge: No
article_type: original
author:
- first_name: Luke Zoltan
full_name: Kelley, Luke Zoltan
last_name: Kelley
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Alberto
full_name: Sesana, Alberto
last_name: Sesana
- first_name: Lars
full_name: Hernquist, Lars
last_name: Hernquist
citation:
ama: Kelley LZ, Haiman Z, Sesana A, Hernquist L. Massive BH binaries as periodically
variable AGN. Monthly Notices of the Royal Astronomical Society. 2019;485(2):1579-1594.
doi:10.1093/mnras/stz150
apa: Kelley, L. Z., Haiman, Z., Sesana, A., & Hernquist, L. (2019). Massive
BH binaries as periodically variable AGN. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stz150
chicago: Kelley, Luke Zoltan, Zoltán Haiman, Alberto Sesana, and Lars Hernquist.
“Massive BH Binaries as Periodically Variable AGN.” Monthly Notices of the
Royal Astronomical Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz150.
ieee: L. Z. Kelley, Z. Haiman, A. Sesana, and L. Hernquist, “Massive BH binaries
as periodically variable AGN,” Monthly Notices of the Royal Astronomical Society,
vol. 485, no. 2. Oxford University Press, pp. 1579–1594, 2019.
ista: Kelley LZ, Haiman Z, Sesana A, Hernquist L. 2019. Massive BH binaries as periodically
variable AGN. Monthly Notices of the Royal Astronomical Society. 485(2), 1579–1594.
mla: Kelley, Luke Zoltan, et al. “Massive BH Binaries as Periodically Variable AGN.”
Monthly Notices of the Royal Astronomical Society, vol. 485, no. 2, Oxford
University Press, 2019, pp. 1579–94, doi:10.1093/mnras/stz150.
short: L.Z. Kelley, Z. Haiman, A. Sesana, L. Hernquist, Monthly Notices of the Royal
Astronomical Society 485 (2019) 1579–1594.
date_created: 2024-09-05T09:59:54Z
date_published: 2019-01-30T00:00:00Z
date_updated: 2024-09-18T08:52:07Z
day: '30'
doi: 10.1093/mnras/stz150
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/stz150
intvolume: ' 485'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stz150
month: '01'
oa: 1
oa_version: Published Version
page: 1579-1594
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Massive BH binaries as periodically variable AGN
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 485
year: '2019'
...
---
_id: '17556'
abstract:
- lang: eng
text: The abundance of molecular hydrogen (H2), the primary coolant in primordial
gas, is critical for the thermodynamic evolution and star-formation histories
in early protogalaxies. Determining the photodissociation rate of H2 by an incident
Lyman-Werner (LW) flux is thus crucial, but prohibitively expensive to calculate
on the fly in simulations. The rate is sensitive to the H2 rovibrational distribution,
which in turn depends on the gas density, temperature, and incident LW radiation
field. We use the publicly available cloudy package to model primordial gas clouds
and compare exact photodissociation rate calculations to commonly-used fitting
formulae. We find the fit from Wolcott-Green et al. (2011) is most accurate for
moderate densities n~10^3 cm^{-3} and temperatures, T~10^3K, and we provide a
new fit, which captures the increase in the rate at higher densities and temperatures,
owing to the increased excited rovibrational populations in this regime. Our new
fit has typical errors of a few percent percent up to n =<10^7 cm^{-3}, T =< 8000K,
and H2 column density NH2 =<10^{17} cm^{-2}, and can be easily utilized in simulations.
We also show that pumping of the excited rovibrational states of H2 by a strong
LW flux further modifies the level populations when the gas density is low, and
noticeably decreases self-shielding for J_21 > 10^3 and n < 10^2 cm^{-3}. This
may lower the "critical flux" at which primordial gas remains H2-poor in some
protogalaxies, enabling massive black hole seed formation.
article_processing_charge: No
article_type: original
author:
- first_name: J
full_name: Wolcott-Green, J
last_name: Wolcott-Green
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: 'Wolcott-Green J, Haiman Z. H2 self-shielding with non-LTE rovibrational populations:
Implications for cooling in protogalaxies. Monthly Notices of the Royal Astronomical
Society. 2019;484(2):2467-2473. doi:10.1093/mnras/sty3280'
apa: 'Wolcott-Green, J., & Haiman, Z. (2019). H2 self-shielding with non-LTE
rovibrational populations: Implications for cooling in protogalaxies. Monthly
Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/sty3280'
chicago: 'Wolcott-Green, J, and Zoltán Haiman. “H2 Self-Shielding with Non-LTE Rovibrational
Populations: Implications for Cooling in Protogalaxies.” Monthly Notices of
the Royal Astronomical Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/sty3280.'
ieee: 'J. Wolcott-Green and Z. Haiman, “H2 self-shielding with non-LTE rovibrational
populations: Implications for cooling in protogalaxies,” Monthly Notices of
the Royal Astronomical Society, vol. 484, no. 2. Oxford University Press,
pp. 2467–2473, 2019.'
ista: 'Wolcott-Green J, Haiman Z. 2019. H2 self-shielding with non-LTE rovibrational
populations: Implications for cooling in protogalaxies. Monthly Notices of the
Royal Astronomical Society. 484(2), 2467–2473.'
mla: 'Wolcott-Green, J., and Zoltán Haiman. “H2 Self-Shielding with Non-LTE Rovibrational
Populations: Implications for Cooling in Protogalaxies.” Monthly Notices of
the Royal Astronomical Society, vol. 484, no. 2, Oxford University Press,
2019, pp. 2467–73, doi:10.1093/mnras/sty3280.'
short: J. Wolcott-Green, Z. Haiman, Monthly Notices of the Royal Astronomical Society
484 (2019) 2467–2473.
date_created: 2024-09-05T10:24:40Z
date_published: 2019-01-16T00:00:00Z
date_updated: 2024-09-18T12:00:29Z
day: '16'
doi: 10.1093/mnras/sty3280
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/sty3280
intvolume: ' 484'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/sty3280
month: '01'
oa: 1
oa_version: Published Version
page: 2467-2473
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'H2 self-shielding with non-LTE rovibrational populations: Implications for
cooling in protogalaxies'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 484
year: '2019'
...
---
_id: '17565'
abstract:
- lang: eng
text: 'The coalescence of a compact object with a 104−107M⊙ supermassive black hole
(SMBH) produces mHz gravitational waves (GWs) detectable by the future Laser Interferometer
Space Antenna (LISA). If such an inspiral occurs in the accretion disc of an active
galactic nucleus (AGN), the gas torques imprint a small deviation in the GW waveform.
Here we present two-dimensional hydrodynamical simulations with the moving-mesh
code DISCO of a BH inspiraling at the GW rate in a binary system with a mass ratio
q=M2/M1=10−3, embedded in an accretion disc. We assume a locally isothermal equation
of state for the gas (with Mach number M=20) and implement a standard α-prescription
for its viscosity (with α=0.03). We find disc torques on the binary that are weaker
than in previous semi-analytic toy models, and are in the opposite direction:
the gas disc slows down, rather than speeds up the inspiral. We compute the resulting
deviations in the GW waveform, which scale linearly with the mass of the disc.
The SNR of these deviations accumulates mostly at high frequencies, and becomes
detectable in a 5-year LISA observation if the total phase shift exceeds a few
radians. We find that this occurs if the disc surface density exceeds Σ0≳102−3gcm−2,
as may be the case in thin discs with near-Eddington accretion rates. Since the
characteristic imprint on the GW signal is strongly dependent on disc parameters,
a LISA detection of an intermediate mass ratio inspiral would probe the physics
of AGN discs and migration.'
article_processing_charge: No
article_type: original
author:
- first_name: A M
full_name: Derdzinski, A M
last_name: Derdzinski
- first_name: D
full_name: D’Orazio, D
last_name: D’Orazio
- first_name: P
full_name: Duffell, P
last_name: Duffell
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: A
full_name: MacFadyen, A
last_name: MacFadyen
citation:
ama: 'Derdzinski AM, D’Orazio D, Duffell P, Haiman Z, MacFadyen A. Probing gas disc
physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion
disc. Monthly Notices of the Royal Astronomical Society. 2019;486(2):2754-2765.
doi:10.1093/mnras/stz1026'
apa: 'Derdzinski, A. M., D’Orazio, D., Duffell, P., Haiman, Z., & MacFadyen,
A. (2019). Probing gas disc physics with LISA: simulations of an intermediate
mass ratio inspiral in an accretion disc. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stz1026'
chicago: 'Derdzinski, A M, D D’Orazio, P Duffell, Zoltán Haiman, and A MacFadyen.
“Probing Gas Disc Physics with LISA: Simulations of an Intermediate Mass Ratio
Inspiral in an Accretion Disc.” Monthly Notices of the Royal Astronomical Society.
Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz1026.'
ieee: 'A. M. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, and A. MacFadyen, “Probing
gas disc physics with LISA: simulations of an intermediate mass ratio inspiral
in an accretion disc,” Monthly Notices of the Royal Astronomical Society,
vol. 486, no. 2. Oxford University Press, pp. 2754–2765, 2019.'
ista: 'Derdzinski AM, D’Orazio D, Duffell P, Haiman Z, MacFadyen A. 2019. Probing
gas disc physics with LISA: simulations of an intermediate mass ratio inspiral
in an accretion disc. Monthly Notices of the Royal Astronomical Society. 486(2),
2754–2765.'
mla: 'Derdzinski, A. M., et al. “Probing Gas Disc Physics with LISA: Simulations
of an Intermediate Mass Ratio Inspiral in an Accretion Disc.” Monthly Notices
of the Royal Astronomical Society, vol. 486, no. 2, Oxford University Press,
2019, pp. 2754–65, doi:10.1093/mnras/stz1026.'
short: A.M. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, A. MacFadyen, Monthly
Notices of the Royal Astronomical Society 486 (2019) 2754–2765.
date_created: 2024-09-05T12:05:43Z
date_published: 2019-09-05T00:00:00Z
date_updated: 2024-09-18T11:01:36Z
day: '05'
doi: 10.1093/mnras/stz1026
extern: '1'
fulldoi: https://doi.org/10.1093/mnras/stz1026
intvolume: ' 486'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/stz1026
month: '09'
oa: 1
oa_version: Published Version
page: 2754-2765
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
issn:
- 0035-8711
- 1365-2966
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1093/mnras/stz2435
scopus_import: '1'
status: public
title: 'Probing gas disc physics with LISA: simulations of an intermediate mass ratio
inspiral in an accretion disc'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 486
year: '2019'
...
---
_id: '17567'
abstract:
- lang: eng
text: The growing number of stellar-mass binary black hole mergers discovered by
Advanced LIGO and Advanced Virgo are starting to constrain the binaries' origin
and environment. However, we still lack sufficiently accurate modeling of binary
formation channels to obtain strong constraints, or to identify sub-populations.
One promising formation mechanism that could result in different black hole properties
is binaries merging within the accretion disks of Active Galactic Nuclei (AGN).
Here we show that the black holes' orbital alignment with the AGN disks preferentially
selects heavier black holes. We carry out Monte Carlo simulations of orbital alignment
with AGN disks, and find that AGNs harden the initial black hole mass function.
Assuming an initial power law mass distribution M−βbh, we find that the power
law index changes by Δβ∼1.3, resulting in a more top-heavy population of merging
black holes. This change is independent of the mass of, and accretion rate onto,
the supermassive black hole in the center of the AGN. Our simulations predict
an AGN-assisted merger rate of ∼4Gpc−3yr−1. With its hardened mass spectra, the
AGN channel could be responsible for 10−50% of gravitational-wave detections.
article_number: '122'
article_processing_charge: No
article_type: original
author:
- first_name: Y.
full_name: Yang, Y.
last_name: Yang
- first_name: I.
full_name: Bartos, I.
last_name: Bartos
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: B.
full_name: Kocsis, B.
last_name: Kocsis
- first_name: Z.
full_name: Márka, Z.
last_name: Márka
- first_name: N. C.
full_name: Stone, N. C.
last_name: Stone
- first_name: S.
full_name: Márka, S.
last_name: Márka
citation:
ama: Yang Y, Bartos I, Haiman Z, et al. AGN disks harden the mass distribution of
stellar-mass binary black hole mergers. The Astrophysical Journal. 2019;876(2).
doi:10.3847/1538-4357/ab16e3
apa: Yang, Y., Bartos, I., Haiman, Z., Kocsis, B., Márka, Z., Stone, N. C., &
Márka, S. (2019). AGN disks harden the mass distribution of stellar-mass binary
black hole mergers. The Astrophysical Journal. American Astronomical Society.
https://doi.org/10.3847/1538-4357/ab16e3
chicago: Yang, Y., I. Bartos, Zoltán Haiman, B. Kocsis, Z. Márka, N. C. Stone, and
S. Márka. “AGN Disks Harden the Mass Distribution of Stellar-Mass Binary Black
Hole Mergers.” The Astrophysical Journal. American Astronomical Society,
2019. https://doi.org/10.3847/1538-4357/ab16e3.
ieee: Y. Yang et al., “AGN disks harden the mass distribution of stellar-mass
binary black hole mergers,” The Astrophysical Journal, vol. 876, no. 2.
American Astronomical Society, 2019.
ista: Yang Y, Bartos I, Haiman Z, Kocsis B, Márka Z, Stone NC, Márka S. 2019. AGN
disks harden the mass distribution of stellar-mass binary black hole mergers.
The Astrophysical Journal. 876(2), 122.
mla: Yang, Y., et al. “AGN Disks Harden the Mass Distribution of Stellar-Mass Binary
Black Hole Mergers.” The Astrophysical Journal, vol. 876, no. 2, 122, American
Astronomical Society, 2019, doi:10.3847/1538-4357/ab16e3.
short: Y. Yang, I. Bartos, Z. Haiman, B. Kocsis, Z. Márka, N.C. Stone, S. Márka,
The Astrophysical Journal 876 (2019).
date_created: 2024-09-05T12:11:39Z
date_published: 2019-05-10T00:00:00Z
date_updated: 2024-09-18T13:26:34Z
day: '10'
doi: 10.3847/1538-4357/ab16e3
extern: '1'
fulldoi: https://doi.org/10.3847/1538-4357/ab16e3
intvolume: ' 876'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.3847/1538-4357/ab16e3
month: '05'
oa: 1
oa_version: Published Version
publication: The Astrophysical Journal
publication_identifier:
issn:
- 0004-637X
- 1538-4357
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: AGN disks harden the mass distribution of stellar-mass binary black hole mergers
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 876
year: '2019'
...