---
_id: '17558'
abstract:
- lang: eng
text: The detection of starlight from the host galaxies of quasars during the reionization
epoch (z > 6) has been elusive, even with deep Hubble Space Telescope observations1,2.
The current highest redshift quasar host detected3, at z = 4.5, required the magnifying
effect of a foreground lensing galaxy. Low-luminosity quasars4,5,6 from the Hyper
Suprime-Cam Subaru Strategic Program (HSC-SSP)7 mitigate the challenge of detecting
their underlying, previously undetected host galaxies. Here we report rest-frame
optical images and spectroscopy of two HSC-SSP quasars at z > 6 with the JWST.
Using near-infrared camera imaging at 3.6 and 1.5 μm and subtracting the light
from the unresolved quasars, we find that the host galaxies are massive (stellar
masses of 13 × and 3.4 × 1010 M☉, respectively), compact and disc-like. Near-infrared
spectroscopy at medium resolution shows stellar absorption lines in the more massive
quasar, confirming the detection of the host. Velocity-broadened gas in the vicinity
of these quasars enables measurements of their black hole masses (1.4 × 109 and
2.0 × 108 M☉, respectively). Their location in the black hole mass–stellar mass
plane is consistent with the distribution at low redshift, suggesting that the
relation between black holes and their host galaxies was already in place less
than a billion years after the Big Bang.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Xuheng
full_name: Ding, Xuheng
last_name: Ding
- first_name: Masafusa
full_name: Onoue, Masafusa
last_name: Onoue
- first_name: John D.
full_name: Silverman, John D.
last_name: Silverman
- first_name: Yoshiki
full_name: Matsuoka, Yoshiki
last_name: Matsuoka
- first_name: Takuma
full_name: Izumi, Takuma
last_name: Izumi
- first_name: Michael A.
full_name: Strauss, Michael A.
last_name: Strauss
- first_name: Knud
full_name: Jahnke, Knud
last_name: Jahnke
- first_name: Camryn L.
full_name: Phillips, Camryn L.
last_name: Phillips
- first_name: Junyao
full_name: Li, Junyao
last_name: Li
- first_name: Marta
full_name: Volonteri, Marta
last_name: Volonteri
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Irham Taufik
full_name: Andika, Irham Taufik
last_name: Andika
- first_name: Kentaro
full_name: Aoki, Kentaro
last_name: Aoki
- first_name: Shunsuke
full_name: Baba, Shunsuke
last_name: Baba
- first_name: Rebekka
full_name: Bieri, Rebekka
last_name: Bieri
- first_name: Sarah E. I.
full_name: Bosman, Sarah E. I.
last_name: Bosman
- first_name: Connor
full_name: Bottrell, Connor
last_name: Bottrell
- first_name: Anna-Christina
full_name: Eilers, Anna-Christina
last_name: Eilers
- first_name: Seiji
full_name: Fujimoto, Seiji
last_name: Fujimoto
- first_name: Melanie
full_name: Habouzit, Melanie
last_name: Habouzit
- first_name: Masatoshi
full_name: Imanishi, Masatoshi
last_name: Imanishi
- first_name: Kohei
full_name: Inayoshi, Kohei
last_name: Inayoshi
- first_name: Kazushi
full_name: Iwasawa, Kazushi
last_name: Iwasawa
- first_name: Nobunari
full_name: Kashikawa, Nobunari
last_name: Kashikawa
- first_name: Toshihiro
full_name: Kawaguchi, Toshihiro
last_name: Kawaguchi
- first_name: Kotaro
full_name: Kohno, Kotaro
last_name: Kohno
- first_name: Chien-Hsiu
full_name: Lee, Chien-Hsiu
last_name: Lee
- first_name: Alessandro
full_name: Lupi, Alessandro
last_name: Lupi
- first_name: Jianwei
full_name: Lyu, Jianwei
last_name: Lyu
- first_name: Tohru
full_name: Nagao, Tohru
last_name: Nagao
- first_name: Roderik
full_name: Overzier, Roderik
last_name: Overzier
- first_name: Jan-Torge
full_name: Schindler, Jan-Torge
last_name: Schindler
- first_name: Malte
full_name: Schramm, Malte
last_name: Schramm
- first_name: Kazuhiro
full_name: Shimasaku, Kazuhiro
last_name: Shimasaku
- first_name: Yoshiki
full_name: Toba, Yoshiki
last_name: Toba
- first_name: Benny
full_name: Trakhtenbrot, Benny
last_name: Trakhtenbrot
- first_name: Maxime
full_name: Trebitsch, Maxime
last_name: Trebitsch
- first_name: Tommaso
full_name: Treu, Tommaso
last_name: Treu
- first_name: Hideki
full_name: Umehata, Hideki
last_name: Umehata
- first_name: Bram P.
full_name: Venemans, Bram P.
last_name: Venemans
- first_name: Marianne
full_name: Vestergaard, Marianne
last_name: Vestergaard
- first_name: Fabian
full_name: Walter, Fabian
last_name: Walter
- first_name: Feige
full_name: Wang, Feige
last_name: Wang
- first_name: Jinyi
full_name: Yang, Jinyi
last_name: Yang
citation:
ama: Ding X, Onoue M, Silverman JD, et al. Detection of stellar light from quasar
host galaxies at redshifts above 6. Nature. 2023;621(7977):51-55. doi:10.1038/s41586-023-06345-5
apa: Ding, X., Onoue, M., Silverman, J. D., Matsuoka, Y., Izumi, T., Strauss, M.
A., … Yang, J. (2023). Detection of stellar light from quasar host galaxies at
redshifts above 6. Nature. Springer Science and Business Media LLC. https://doi.org/10.1038/s41586-023-06345-5
chicago: Ding, Xuheng, Masafusa Onoue, John D. Silverman, Yoshiki Matsuoka, Takuma
Izumi, Michael A. Strauss, Knud Jahnke, et al. “Detection of Stellar Light from
Quasar Host Galaxies at Redshifts above 6.” Nature. Springer Science and
Business Media LLC, 2023. https://doi.org/10.1038/s41586-023-06345-5.
ieee: X. Ding et al., “Detection of stellar light from quasar host galaxies
at redshifts above 6,” Nature, vol. 621, no. 7977. Springer Science and
Business Media LLC, pp. 51–55, 2023.
ista: Ding X, Onoue M, Silverman JD, Matsuoka Y, Izumi T, Strauss MA, Jahnke K,
Phillips CL, Li J, Volonteri M, Haiman Z, Andika IT, Aoki K, Baba S, Bieri R,
Bosman SEI, Bottrell C, Eilers A-C, Fujimoto S, Habouzit M, Imanishi M, Inayoshi
K, Iwasawa K, Kashikawa N, Kawaguchi T, Kohno K, Lee C-H, Lupi A, Lyu J, Nagao
T, Overzier R, Schindler J-T, Schramm M, Shimasaku K, Toba Y, Trakhtenbrot B,
Trebitsch M, Treu T, Umehata H, Venemans BP, Vestergaard M, Walter F, Wang F,
Yang J. 2023. Detection of stellar light from quasar host galaxies at redshifts
above 6. Nature. 621(7977), 51–55.
mla: Ding, Xuheng, et al. “Detection of Stellar Light from Quasar Host Galaxies
at Redshifts above 6.” Nature, vol. 621, no. 7977, Springer Science and
Business Media LLC, 2023, pp. 51–55, doi:10.1038/s41586-023-06345-5.
short: X. Ding, M. Onoue, J.D. Silverman, Y. Matsuoka, T. Izumi, M.A. Strauss, K.
Jahnke, C.L. Phillips, J. Li, M. Volonteri, Z. Haiman, I.T. Andika, K. Aoki, S.
Baba, R. Bieri, S.E.I. Bosman, C. Bottrell, A.-C. Eilers, S. Fujimoto, M. Habouzit,
M. Imanishi, K. Inayoshi, K. Iwasawa, N. Kashikawa, T. Kawaguchi, K. Kohno, C.-H.
Lee, A. Lupi, J. Lyu, T. Nagao, R. Overzier, J.-T. Schindler, M. Schramm, K. Shimasaku,
Y. Toba, B. Trakhtenbrot, M. Trebitsch, T. Treu, H. Umehata, B.P. Venemans, M.
Vestergaard, F. Walter, F. Wang, J. Yang, Nature 621 (2023) 51–55.
date_created: 2024-09-05T11:28:21Z
date_published: 2023-06-28T00:00:00Z
date_updated: 2024-09-18T12:19:50Z
day: '28'
doi: 10.1038/s41586-023-06345-5
extern: '1'
external_id:
arxiv:
- '2211.14329'
intvolume: ' 621'
issue: '7977'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.2211.14329'
month: '06'
oa: 1
oa_version: Preprint
page: 51-55
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: Detection of stellar light from quasar host galaxies at redshifts above 6
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 621
year: '2023'
...
---
_id: '17536'
abstract:
- lang: eng
text: There is some weak evidence that the black hole merger named GW190521 had
a non-zero eccentricity. In addition, the component black holes' masses exceeded
the limit predicted by stellar evolution. The large masses can be explained by
successive mergers, which may be efficient in gas disks surrounding active galactic
nuclei (AGN), but it is difficult to maintain an eccentric orbit all the way to
the merger, as basic physics would argue for circularization. Here we show that
AGN-disk environments can lead to an excess of eccentric mergers, if the interactions
between single and binary black holes are frequent, and occur with mutual inclinations
of less than a few degrees. We further illustrate that this eccentric population
has a different distribution of the inclination between the spin vectors of the
black holes and their orbital angular momentum at merger, referred to as the spin-orbit
tilt, compared to the remaining circular mergers.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: J.
full_name: Samsing, J.
last_name: Samsing
- first_name: I.
full_name: Bartos, I.
last_name: Bartos
- first_name: D. J.
full_name: D’Orazio, D. J.
last_name: D’Orazio
- 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: N. W. C.
full_name: Leigh, N. W. C.
last_name: Leigh
- first_name: B.
full_name: Liu, B.
last_name: Liu
- first_name: M. E.
full_name: Pessah, M. E.
last_name: Pessah
- first_name: H.
full_name: Tagawa, H.
last_name: Tagawa
citation:
ama: Samsing J, Bartos I, D’Orazio DJ, et al. AGN as potential factories for eccentric
black hole mergers. Nature. 2022;603(7900):237-240. doi:10.1038/s41586-021-04333-1
apa: Samsing, J., Bartos, I., D’Orazio, D. J., Haiman, Z., Kocsis, B., Leigh, N.
W. C., … Tagawa, H. (2022). AGN as potential factories for eccentric black hole
mergers. Nature. Springer Science and Business Media LLC. https://doi.org/10.1038/s41586-021-04333-1
chicago: Samsing, J., I. Bartos, D. J. D’Orazio, Zoltán Haiman, B. Kocsis, N. W.
C. Leigh, B. Liu, M. E. Pessah, and H. Tagawa. “AGN as Potential Factories for
Eccentric Black Hole Mergers.” Nature. Springer Science and Business Media
LLC, 2022. https://doi.org/10.1038/s41586-021-04333-1.
ieee: J. Samsing et al., “AGN as potential factories for eccentric black
hole mergers,” Nature, vol. 603, no. 7900. Springer Science and Business
Media LLC, pp. 237–240, 2022.
ista: Samsing J, Bartos I, D’Orazio DJ, Haiman Z, Kocsis B, Leigh NWC, Liu B, Pessah
ME, Tagawa H. 2022. AGN as potential factories for eccentric black hole mergers.
Nature. 603(7900), 237–240.
mla: Samsing, J., et al. “AGN as Potential Factories for Eccentric Black Hole Mergers.”
Nature, vol. 603, no. 7900, Springer Science and Business Media LLC, 2022,
pp. 237–40, doi:10.1038/s41586-021-04333-1.
short: J. Samsing, I. Bartos, D.J. D’Orazio, Z. Haiman, B. Kocsis, N.W.C. Leigh,
B. Liu, M.E. Pessah, H. Tagawa, Nature 603 (2022) 237–240.
date_created: 2024-09-05T09:45:31Z
date_published: 2022-05-09T00:00:00Z
date_updated: 2024-09-12T09:24:50Z
day: '09'
doi: 10.1038/s41586-021-04333-1
extern: '1'
external_id:
arxiv:
- '2010.09765'
intvolume: ' 603'
issue: '7900'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.2010.09765'
month: '05'
oa: 1
oa_version: Preprint
page: 237-240
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: AGN as potential factories for eccentric black hole mergers
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 603
year: '2022'
...
---
_id: '18199'
abstract:
- lang: eng
text: 'The concept of a supersolid state combines the crystallization of a many-body
system with dissipationless flow of the atoms from which it is built. This quantum
phase requires the breaking of two continuous symmetries: the phase invariance
of a superfluid and the continuous translational invariance to form the crystal1,2.
Despite having been proposed for helium almost 50 years ago3,4, experimental verification
of supersolidity remains elusive5,6. A variant with only discrete translational
symmetry breaking on a preimposed lattice structure—the ‘lattice supersolid’7—has
been realized, based on self-organization of a Bose–Einstein condensate8,9. However,
lattice supersolids do not feature the continuous ground-state degeneracy that
characterizes the supersolid state as originally proposed. Here we report the
realization of a supersolid with continuous translational symmetry breaking along
one direction in a quantum gas. The continuous symmetry that is broken emerges
from two discrete spatial symmetries by symmetrically coupling a Bose–Einstein
condensate to the modes of two optical cavities. We establish the phase coherence
of the supersolid and find a high ground-state degeneracy by measuring the crystal
position over many realizations through the light fields that leak from the cavities.
These light fields are also used to monitor the position fluctuations in real
time. Our concept provides a route to creating and studying glassy many-body systems
with controllably lifted ground-state degeneracies, such as supersolids in the
presence of disorder.'
article_processing_charge: No
article_type: letter_note
author:
- first_name: Julian
full_name: Leonard, Julian
id: b75b3f45-7995-11ef-9bfd-9a9cd02c3577
last_name: Leonard
- first_name: Andrea
full_name: Morales, Andrea
last_name: Morales
- first_name: Philip
full_name: Zupancic, Philip
last_name: Zupancic
- first_name: Tilman
full_name: Esslinger, Tilman
last_name: Esslinger
- first_name: Tobias
full_name: Donner, Tobias
last_name: Donner
citation:
ama: Leonard J, Morales A, Zupancic P, Esslinger T, Donner T. Supersolid formation
in a quantum gas breaking a continuous translational symmetry. Nature.
2017;543(7643):87-90. doi:10.1038/nature21067
apa: Leonard, J., Morales, A., Zupancic, P., Esslinger, T., & Donner, T. (2017).
Supersolid formation in a quantum gas breaking a continuous translational symmetry.
Nature. Springer Science and Business Media LLC. https://doi.org/10.1038/nature21067
chicago: Leonard, Julian, Andrea Morales, Philip Zupancic, Tilman Esslinger, and
Tobias Donner. “Supersolid Formation in a Quantum Gas Breaking a Continuous Translational
Symmetry.” Nature. Springer Science and Business Media LLC, 2017. https://doi.org/10.1038/nature21067.
ieee: J. Leonard, A. Morales, P. Zupancic, T. Esslinger, and T. Donner, “Supersolid
formation in a quantum gas breaking a continuous translational symmetry,” Nature,
vol. 543, no. 7643. Springer Science and Business Media LLC, pp. 87–90, 2017.
ista: Leonard J, Morales A, Zupancic P, Esslinger T, Donner T. 2017. Supersolid
formation in a quantum gas breaking a continuous translational symmetry. Nature.
543(7643), 87–90.
mla: Leonard, Julian, et al. “Supersolid Formation in a Quantum Gas Breaking a Continuous
Translational Symmetry.” Nature, vol. 543, no. 7643, Springer Science and
Business Media LLC, 2017, pp. 87–90, doi:10.1038/nature21067.
short: J. Leonard, A. Morales, P. Zupancic, T. Esslinger, T. Donner, Nature 543
(2017) 87–90.
date_created: 2024-10-07T11:49:44Z
date_published: 2017-03-02T00:00:00Z
date_updated: 2024-10-07T12:09:33Z
day: '02'
doi: 10.1038/nature21067
extern: '1'
intvolume: ' 543'
issue: '7643'
language:
- iso: eng
month: '03'
oa_version: None
page: 87-90
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: Supersolid formation in a quantum gas breaking a continuous translational symmetry
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 543
year: '2017'
...
---
_id: '6117'
abstract:
- lang: eng
text: 'Interleukin-17 (IL-17) is a major pro-inflammatory cytokine: it mediates
responses to pathogens or tissue damage, and drives autoimmune diseases. Little
is known about its role in the nervous system. Here we show that IL-17 has neuromodulator-like
properties in Caenorhabditis elegans. IL-17 can act directly on neurons to alter
their response properties and contribution to behaviour. Using unbiased genetic
screens, we delineate an IL-17 signalling pathway and show that it acts in the
RMG hub interneurons. Disrupting IL-17 signalling reduces RMG responsiveness to
input from oxygen sensors, and renders sustained escape from 21% oxygen transient
and contingent on additional stimuli. Over-activating IL-17 receptors abnormally
heightens responses to 21% oxygen in RMG neurons and whole animals. IL-17 deficiency
can be bypassed by optogenetic stimulation of RMG. Inducing IL-17 expression in
adults can rescue mutant defects within 6 h. These findings reveal a non-immunological
role of IL-17 modulating circuit function and behaviour.'
author:
- first_name: Changchun
full_name: Chen, Changchun
last_name: Chen
- first_name: Eisuke
full_name: Itakura, Eisuke
last_name: Itakura
- first_name: Geoffrey M.
full_name: Nelson, Geoffrey M.
last_name: Nelson
- first_name: Ming
full_name: Sheng, Ming
last_name: Sheng
- first_name: Patrick
full_name: Laurent, Patrick
last_name: Laurent
- first_name: Lorenz A.
full_name: Fenk, Lorenz A.
last_name: Fenk
- first_name: Rebecca A.
full_name: Butcher, Rebecca A.
last_name: Butcher
- first_name: Ramanujan S.
full_name: Hegde, Ramanujan S.
last_name: Hegde
- first_name: Mario
full_name: de Bono, Mario
id: 4E3FF80E-F248-11E8-B48F-1D18A9856A87
last_name: de Bono
orcid: 0000-0001-8347-0443
citation:
ama: Chen C, Itakura E, Nelson GM, et al. IL-17 is a neuromodulator of Caenorhabditis
elegans sensory responses. Nature. 2017;542(7639):43-48. doi:10.1038/nature20818
apa: Chen, C., Itakura, E., Nelson, G. M., Sheng, M., Laurent, P., Fenk, L. A.,
… de Bono, M. (2017). IL-17 is a neuromodulator of Caenorhabditis elegans sensory
responses. Nature. Springer Nature. https://doi.org/10.1038/nature20818
chicago: Chen, Changchun, Eisuke Itakura, Geoffrey M. Nelson, Ming Sheng, Patrick
Laurent, Lorenz A. Fenk, Rebecca A. Butcher, Ramanujan S. Hegde, and Mario de
Bono. “IL-17 Is a Neuromodulator of Caenorhabditis Elegans Sensory Responses.”
Nature. Springer Nature, 2017. https://doi.org/10.1038/nature20818.
ieee: C. Chen et al., “IL-17 is a neuromodulator of Caenorhabditis elegans
sensory responses,” Nature, vol. 542, no. 7639. Springer Nature, pp. 43–48,
2017.
ista: Chen C, Itakura E, Nelson GM, Sheng M, Laurent P, Fenk LA, Butcher RA, Hegde
RS, de Bono M. 2017. IL-17 is a neuromodulator of Caenorhabditis elegans sensory
responses. Nature. 542(7639), 43–48.
mla: Chen, Changchun, et al. “IL-17 Is a Neuromodulator of Caenorhabditis Elegans
Sensory Responses.” Nature, vol. 542, no. 7639, Springer Nature, 2017,
pp. 43–48, doi:10.1038/nature20818.
short: C. Chen, E. Itakura, G.M. Nelson, M. Sheng, P. Laurent, L.A. Fenk, R.A. Butcher,
R.S. Hegde, M. de Bono, Nature 542 (2017) 43–48.
date_created: 2019-03-19T14:06:41Z
date_published: 2017-02-02T00:00:00Z
date_updated: 2021-01-12T08:06:12Z
day: '02'
doi: 10.1038/nature20818
extern: '1'
external_id:
pmid:
- ' 28099418'
intvolume: ' 542'
issue: '7639'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://www.ncbi.nlm.nih.gov/pubmed/28099418
month: '02'
oa: 1
oa_version: Submitted Version
page: 43-48
pmid: 1
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: IL-17 is a neuromodulator of Caenorhabditis elegans sensory responses
type: journal_article
user_id: 3E5EF7F0-F248-11E8-B48F-1D18A9856A87
volume: 542
year: '2017'
...
---
_id: '17652'
abstract:
- lang: eng
text: Because most large galaxies contain a central black hole, and galaxies often
merge, black-hole binaries are expected to be common in galactic nuclei. Although
they cannot be imaged, periodicities in the light curves of quasars have been
interpreted as evidence for binaries, most recently in PG~1302-102, with a short
rest-frame optical period of 4 years. If the orbital period matches this value,
then for the range of estimated black hole masses the components would be separated
by 0.007-0.017 pc, implying relativistic orbital speeds. There has been much debate
over whether black hole orbits could be smaller than 1 pc. Here we show that the
amplitude and the sinusoid-like shape of the variability of PG~1302-102 can be
fit by relativistic Doppler boosting of emission from a compact, steadily accreting,
unequal-mass binary. We predict that brightness variations in the ultraviolet
light curve track those in the optical, but with a 2-3 times larger amplitude.
This prediction is relatively insensitive to the details of the emission process,
and is consistent with archival UV data. Follow-up UV and optical observations
in the next few years can test this prediction and confirm the existence of a
binary black hole in the relativistic regime.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Daniel J.
full_name: D'Orazio, Daniel J.
last_name: D'Orazio
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: David
full_name: Schiminovich, David
last_name: Schiminovich
citation:
ama: D’Orazio DJ, Haiman Z, Schiminovich D. Relativistic boost as the cause of periodicity
in a massive black-hole binary candidate. Nature. 2015;525(7569):351-353.
doi:10.1038/nature15262
apa: D’Orazio, D. J., Haiman, Z., & Schiminovich, D. (2015). Relativistic boost
as the cause of periodicity in a massive black-hole binary candidate. Nature.
Springer Science and Business Media LLC. https://doi.org/10.1038/nature15262
chicago: D’Orazio, Daniel J., Zoltán Haiman, and David Schiminovich. “Relativistic
Boost as the Cause of Periodicity in a Massive Black-Hole Binary Candidate.” Nature.
Springer Science and Business Media LLC, 2015. https://doi.org/10.1038/nature15262.
ieee: D. J. D’Orazio, Z. Haiman, and D. Schiminovich, “Relativistic boost as the
cause of periodicity in a massive black-hole binary candidate,” Nature,
vol. 525, no. 7569. Springer Science and Business Media LLC, pp. 351–353, 2015.
ista: D’Orazio DJ, Haiman Z, Schiminovich D. 2015. Relativistic boost as the cause
of periodicity in a massive black-hole binary candidate. Nature. 525(7569), 351–353.
mla: D’Orazio, Daniel J., et al. “Relativistic Boost as the Cause of Periodicity
in a Massive Black-Hole Binary Candidate.” Nature, vol. 525, no. 7569,
Springer Science and Business Media LLC, 2015, pp. 351–53, doi:10.1038/nature15262.
short: D.J. D’Orazio, Z. Haiman, D. Schiminovich, Nature 525 (2015) 351–353.
date_created: 2024-09-06T07:30:45Z
date_published: 2015-09-16T00:00:00Z
date_updated: 2024-09-24T13:22:24Z
day: '16'
doi: 10.1038/nature15262
extern: '1'
external_id:
arxiv:
- '1509.04301'
intvolume: ' 525'
issue: '7569'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1509.04301'
month: '09'
oa: 1
oa_version: Preprint
page: 351-353
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: Relativistic boost as the cause of periodicity in a massive black-hole binary
candidate
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 525
year: '2015'
...
---
_id: '17701'
abstract:
- lang: eng
text: Independent lines of evidence suggest that the first stars, which ended the
cosmic dark ages, came in pairs, rather than singly. This could change the prevailing
view that the early Universe had a Swiss-cheese-like appearance.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Haiman Z. A smoother end to the dark ages. Nature. 2011;472(7341):47-48.
doi:10.1038/472047a
apa: Haiman, Z. (2011). A smoother end to the dark ages. Nature. Springer
Science and Business Media LLC. https://doi.org/10.1038/472047a
chicago: Haiman, Zoltán. “A Smoother End to the Dark Ages.” Nature. Springer
Science and Business Media LLC, 2011. https://doi.org/10.1038/472047a.
ieee: Z. Haiman, “A smoother end to the dark ages,” Nature, vol. 472, no.
7341. Springer Science and Business Media LLC, pp. 47–48, 2011.
ista: Haiman Z. 2011. A smoother end to the dark ages. Nature. 472(7341), 47–48.
mla: Haiman, Zoltán. “A Smoother End to the Dark Ages.” Nature, vol. 472,
no. 7341, Springer Science and Business Media LLC, 2011, pp. 47–48, doi:10.1038/472047a.
short: Z. Haiman, Nature 472 (2011) 47–48.
date_created: 2024-09-06T08:47:22Z
date_published: 2011-04-06T00:00:00Z
date_updated: 2024-09-25T11:25:52Z
day: '06'
doi: 10.1038/472047a
extern: '1'
external_id:
arxiv:
- '1104.1189'
intvolume: ' 472'
issue: '7341'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.1104.1189'
month: '04'
oa: 1
oa_version: Preprint
page: 47-48
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: A smoother end to the dark ages
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 472
year: '2011'
...
---
_id: '6144'
abstract:
- lang: eng
text: Behaviours evolve by iterations of natural selection, but we have few insights
into the molecular and neural mechanisms involved. Here we show that some Caenorhabditis
elegans wild strains switch between two foraging behaviours in response to subtle
changes in ambient oxygen. This finely tuned switch is conferred by a naturally
variable hexacoordinated globin, GLB-5. GLB-5 acts with the atypical soluble guanylate
cyclases1,2,3, which are a different type of oxygen binding protein, to tune the
dynamic range of oxygen-sensing neurons close to atmospheric (21%) concentrations.
Calcium imaging indicates that one group of these neurons is activated when oxygen
rises towards 21%, and is inhibited as oxygen drops below 21%. The soluble guanylate
cyclase GCY-35 is required for high oxygen to activate the neurons; GLB-5 provides
inhibitory input when oxygen decreases below 21%. Together, these oxygen binding
proteins tune neuronal and behavioural responses to a narrow oxygen concentration
range close to atmospheric levels. The effect of the glb-5 gene on oxygen sensing
and foraging is modified by the naturally variable neuropeptide receptor npr-1
(refs 4, 5), providing insights into how polygenic variation reshapes neural circuit
function.
author:
- first_name: Annelie
full_name: Persson, Annelie
last_name: Persson
- first_name: Einav
full_name: Gross, Einav
last_name: Gross
- first_name: Patrick
full_name: Laurent, Patrick
last_name: Laurent
- first_name: Karl Emanuel
full_name: Busch, Karl Emanuel
last_name: Busch
- first_name: Hugo
full_name: Bretes, Hugo
last_name: Bretes
- first_name: Mario
full_name: de Bono, Mario
id: 4E3FF80E-F248-11E8-B48F-1D18A9856A87
last_name: de Bono
orcid: 0000-0001-8347-0443
citation:
ama: Persson A, Gross E, Laurent P, Busch KE, Bretes H, de Bono M. Natural variation
in a neural globin tunes oxygen sensing in wild Caenorhabditis elegans. Nature.
2009;458(7241):1030-1033. doi:10.1038/nature07820
apa: Persson, A., Gross, E., Laurent, P., Busch, K. E., Bretes, H., & de Bono,
M. (2009). Natural variation in a neural globin tunes oxygen sensing in wild Caenorhabditis
elegans. Nature. Springer Nature. https://doi.org/10.1038/nature07820
chicago: Persson, Annelie, Einav Gross, Patrick Laurent, Karl Emanuel Busch, Hugo
Bretes, and Mario de Bono. “Natural Variation in a Neural Globin Tunes Oxygen
Sensing in Wild Caenorhabditis Elegans.” Nature. Springer Nature, 2009.
https://doi.org/10.1038/nature07820.
ieee: A. Persson, E. Gross, P. Laurent, K. E. Busch, H. Bretes, and M. de Bono,
“Natural variation in a neural globin tunes oxygen sensing in wild Caenorhabditis
elegans,” Nature, vol. 458, no. 7241. Springer Nature, pp. 1030–1033, 2009.
ista: Persson A, Gross E, Laurent P, Busch KE, Bretes H, de Bono M. 2009. Natural
variation in a neural globin tunes oxygen sensing in wild Caenorhabditis elegans.
Nature. 458(7241), 1030–1033.
mla: Persson, Annelie, et al. “Natural Variation in a Neural Globin Tunes Oxygen
Sensing in Wild Caenorhabditis Elegans.” Nature, vol. 458, no. 7241, Springer
Nature, 2009, pp. 1030–33, doi:10.1038/nature07820.
short: A. Persson, E. Gross, P. Laurent, K.E. Busch, H. Bretes, M. de Bono, Nature
458 (2009) 1030–1033.
date_created: 2019-03-21T07:48:44Z
date_published: 2009-04-23T00:00:00Z
date_updated: 2021-01-12T08:06:20Z
day: '23'
doi: 10.1038/nature07820
extern: '1'
external_id:
pmid:
- '19262507'
intvolume: ' 458'
issue: '7241'
language:
- iso: eng
month: '04'
oa_version: None
page: 1030-1033
pmid: 1
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: Natural variation in a neural globin tunes oxygen sensing in wild Caenorhabditis
elegans
type: journal_article
user_id: 3E5EF7F0-F248-11E8-B48F-1D18A9856A87
volume: 458
year: '2009'
...
---
_id: '17808'
abstract:
- lang: eng
text: Four recent observational results have challenged our understanding of high--redshift
galaxies, as they require the presence of far more ultraviolet photons than should
be emitted by normal stellar populations. First, there is significant ultraviolet
emission from Lyman Break Galaxies (LBGs) at wavelenghts shorter than 912Å. Second,
there is strong Lyman alpha emission from extended ``blobs'' with little or no
associated apparent ionizing continuum. Third, there is a population of galaxies
with unusually strong Lyman-alpha emission lines. And fourth, there is a strong
HeII (1640 Å) emission line in a composite of LBGs. The proposed explanations
for the first three observations are internally inconsistent, and the fourth puzzle
has remained hitherto unexplained. Here we show that all four problems are resolved
simultaneously if 10-30 percent of the stars in many galaxies at z ~ 3-4 are mainly
primordial - unenriched by elements heavier than helium ('metals'). Most models
of hierarchical galaxy formation assume efficient intra--galactic metal mixing,
and therefore do not predict metal-free star formation at redshifts significantly
below z ~5. Our results imply that micro-mixing of metals within galaxies is inefficient
on a ~ Gyr time-scale, a conclusion that can be verified with higher resolution
simulations, and future observations of the HeII emission line.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Raul
full_name: Jimenez, Raul
last_name: Jimenez
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Jimenez R, Haiman Z. Significant primordial star formation at redshifts z ≈
3–4. Nature. 2006;440(7083):501-504. doi:10.1038/nature04580
apa: Jimenez, R., & Haiman, Z. (2006). Significant primordial star formation
at redshifts z ≈ 3–4. Nature. Springer Science and Business Media LLC.
https://doi.org/10.1038/nature04580
chicago: Jimenez, Raul, and Zoltán Haiman. “Significant Primordial Star Formation
at Redshifts z ≈ 3–4.” Nature. Springer Science and Business Media LLC,
2006. https://doi.org/10.1038/nature04580.
ieee: R. Jimenez and Z. Haiman, “Significant primordial star formation at redshifts
z ≈ 3–4,” Nature, vol. 440, no. 7083. Springer Science and Business Media
LLC, pp. 501–504, 2006.
ista: Jimenez R, Haiman Z. 2006. Significant primordial star formation at redshifts
z ≈ 3–4. Nature. 440(7083), 501–504.
mla: Jimenez, Raul, and Zoltán Haiman. “Significant Primordial Star Formation at
Redshifts z ≈ 3–4.” Nature, vol. 440, no. 7083, Springer Science and Business
Media LLC, 2006, pp. 501–04, doi:10.1038/nature04580.
short: R. Jimenez, Z. Haiman, Nature 440 (2006) 501–504.
date_created: 2024-09-06T11:37:20Z
date_published: 2006-03-23T00:00:00Z
date_updated: 2024-09-25T14:01:07Z
day: '23'
doi: 10.1038/nature04580
extern: '1'
external_id:
arxiv:
- '0602450'
intvolume: ' 440'
issue: '7083'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.astro-ph/0602450'
month: '03'
oa: 1
oa_version: Preprint
page: 501-504
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1038/nature04774
scopus_import: '1'
status: public
title: Significant primordial star formation at redshifts z ≈ 3–4
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 440
year: '2006'
...
---
_id: '17792'
abstract:
- lang: eng
text: Which came first, the stars and gas that make up a galaxy, or the giant black
hole at its centre? Observations of a distant galaxy, caught as it forms, could
help solve this chicken-and-egg problem.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Haiman Z. Caught in the act? Nature. 2004;430(7003):979-980. doi:10.1038/430979a
apa: Haiman, Z. (2004). Caught in the act? Nature. Springer Science and Business
Media LLC. https://doi.org/10.1038/430979a
chicago: Haiman, Zoltán. “Caught in the Act?” Nature. Springer Science and
Business Media LLC, 2004. https://doi.org/10.1038/430979a.
ieee: Z. Haiman, “Caught in the act?,” Nature, vol. 430, no. 7003. Springer
Science and Business Media LLC, pp. 979–980, 2004.
ista: Haiman Z. 2004. Caught in the act? Nature. 430(7003), 979–980.
mla: Haiman, Zoltán. “Caught in the Act?” Nature, vol. 430, no. 7003, Springer
Science and Business Media LLC, 2004, pp. 979–80, doi:10.1038/430979a.
short: Z. Haiman, Nature 430 (2004) 979–980.
date_created: 2024-09-06T10:24:04Z
date_published: 2004-08-25T00:00:00Z
date_updated: 2024-09-30T14:07:00Z
day: '25'
doi: 10.1038/430979a
extern: '1'
external_id:
arxiv:
- '0408479'
intvolume: ' 430'
issue: '7003'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: ' https://doi.org/10.48550/arXiv.astro-ph/0408479'
month: '08'
oa: 1
oa_version: Preprint
page: 979-980
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Science and Business Media LLC
quality_controlled: '1'
scopus_import: '1'
status: public
title: Caught in the act?
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 430
year: '2004'
...
---
OA_type: closed access
_id: '18369'
article_processing_charge: No
article_type: letter_note
author:
- first_name: Michael M.
full_name: Bronstein, Michael M.
last_name: Bronstein
- first_name: Alexander
full_name: Bronstein, Alexander
id: 58f3726e-7cba-11ef-ad8b-e6e8cb3904e6
last_name: Bronstein
orcid: 0000-0001-9699-8730
citation:
ama: Bronstein MM, Bronstein AM. Biometrics was no match for hair-raising tricks.
Nature. 2002;420(6917):739-739. doi:10.1038/420739a
apa: Bronstein, M. M., & Bronstein, A. M. (2002). Biometrics was no match for
hair-raising tricks. Nature. Springer Nature. https://doi.org/10.1038/420739a
chicago: Bronstein, Michael M., and Alex M. Bronstein. “Biometrics Was No Match
for Hair-Raising Tricks.” Nature. Springer Nature, 2002. https://doi.org/10.1038/420739a.
ieee: M. M. Bronstein and A. M. Bronstein, “Biometrics was no match for hair-raising
tricks,” Nature, vol. 420, no. 6917. Springer Nature, pp. 739–739, 2002.
ista: Bronstein MM, Bronstein AM. 2002. Biometrics was no match for hair-raising
tricks. Nature. 420(6917), 739–739.
mla: Bronstein, Michael M., and Alex M. Bronstein. “Biometrics Was No Match for
Hair-Raising Tricks.” Nature, vol. 420, no. 6917, Springer Nature, 2002,
pp. 739–739, doi:10.1038/420739a.
short: M.M. Bronstein, A.M. Bronstein, Nature 420 (2002) 739–739.
date_created: 2024-10-15T11:20:54Z
date_published: 2002-12-19T00:00:00Z
date_updated: 2024-10-21T09:06:34Z
day: '19'
doi: 10.1038/420739a
extern: '1'
external_id:
pmid:
- '12490915'
intvolume: ' 420'
issue: '6917'
language:
- iso: eng
month: '12'
oa_version: None
page: 739-739
pmid: 1
publication: Nature
publication_identifier:
issn:
- 0028-0836
- 1476-4687
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Biometrics was no match for hair-raising tricks
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 420
year: '2002'
...