---
_id: '2339'
alternative_title:
- Contemporary Mathematics
author:
- first_name: Robert
full_name: Robert Seiringer
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: 'Seiringer R. Symmetry breaking in a model of a rotating Bose gas. In: Weder
R, Exner P, Grébert B, eds. Vol 307. World Scientific Publishing; 2002:281-286.
doi:10.1090/conm/307'
apa: 'Seiringer, R. (2002). Symmetry breaking in a model of a rotating Bose gas.
In R. Weder, P. Exner, & B. Grébert (Eds.) (Vol. 307, pp. 281–286). Presented
at the QMath: Mathematical Results in Quantum Physics, World Scientific Publishing.
https://doi.org/10.1090/conm/307'
chicago: Seiringer, Robert. “Symmetry Breaking in a Model of a Rotating Bose Gas.”
edited by Richardo Weder, Pavel Exner, and Benoit Grébert, 307:281–86. World Scientific
Publishing, 2002. https://doi.org/10.1090/conm/307.
ieee: 'R. Seiringer, “Symmetry breaking in a model of a rotating Bose gas,” presented
at the QMath: Mathematical Results in Quantum Physics, 2002, vol. 307, pp. 281–286.'
ista: 'Seiringer R. 2002. Symmetry breaking in a model of a rotating Bose gas. QMath:
Mathematical Results in Quantum Physics, Contemporary Mathematics, vol. 307, 281–286.'
mla: Seiringer, Robert. Symmetry Breaking in a Model of a Rotating Bose Gas.
Edited by Richardo Weder et al., vol. 307, World Scientific Publishing, 2002,
pp. 281–86, doi:10.1090/conm/307.
short: R. Seiringer, in:, R. Weder, P. Exner, B. Grébert (Eds.), World Scientific
Publishing, 2002, pp. 281–286.
conference:
name: 'QMath: Mathematical Results in Quantum Physics'
date_created: 2018-12-11T11:57:05Z
date_published: 2002-01-01T00:00:00Z
date_updated: 2021-01-12T06:56:53Z
day: '01'
doi: 10.1090/conm/307
editor:
- first_name: Richardo
full_name: Weder, Richardo
last_name: Weder
- first_name: Pavel
full_name: Exner, Pavel
last_name: Exner
- first_name: Benoit
full_name: Grébert, Benoit
last_name: Grébert
extern: 1
intvolume: ' 307'
month: '01'
page: 281 - 286
publication_status: published
publisher: World Scientific Publishing
publist_id: '4587'
quality_controlled: 0
status: public
title: Symmetry breaking in a model of a rotating Bose gas
type: conference
volume: 307
year: '2002'
...
---
_id: '2349'
abstract:
- lang: eng
text: The Bose-Einstein condensation (BEC) of the ground state of bosonic atoms
in a trap was discussed. The BEC was proved for bosons with two-body repulsive
interaction potentials in the dilute limit, starting from the basic Schrodinger
equation. The BEC was 100% into the state which minimized the Gross-Pitaevskii
energy functional. The analysis also included rigorous proof of BEC in a physically
realistic, continuum model.
author:
- first_name: Élliott
full_name: Lieb, Élliott H
last_name: Lieb
- first_name: Robert
full_name: Robert Seiringer
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: Lieb É, Seiringer R. Proof of Bose-Einstein condensation for dilute trapped
gases. Physical Review Letters. 2002;88(17):1704091-1704094. doi:10.1103/PhysRevLett.88.170409
apa: Lieb, É., & Seiringer, R. (2002). Proof of Bose-Einstein condensation for
dilute trapped gases. Physical Review Letters. American Physical Society.
https://doi.org/10.1103/PhysRevLett.88.170409
chicago: Lieb, Élliott, and Robert Seiringer. “Proof of Bose-Einstein Condensation
for Dilute Trapped Gases.” Physical Review Letters. American Physical Society,
2002. https://doi.org/10.1103/PhysRevLett.88.170409.
ieee: É. Lieb and R. Seiringer, “Proof of Bose-Einstein condensation for dilute
trapped gases,” Physical Review Letters, vol. 88, no. 17. American Physical
Society, pp. 1704091–1704094, 2002.
ista: Lieb É, Seiringer R. 2002. Proof of Bose-Einstein condensation for dilute
trapped gases. Physical Review Letters. 88(17), 1704091–1704094.
mla: Lieb, Élliott, and Robert Seiringer. “Proof of Bose-Einstein Condensation for
Dilute Trapped Gases.” Physical Review Letters, vol. 88, no. 17, American
Physical Society, 2002, pp. 1704091–94, doi:10.1103/PhysRevLett.88.170409.
short: É. Lieb, R. Seiringer, Physical Review Letters 88 (2002) 1704091–1704094.
date_created: 2018-12-11T11:57:08Z
date_published: 2002-04-29T00:00:00Z
date_updated: 2021-01-12T06:56:56Z
day: '29'
doi: 10.1103/PhysRevLett.88.170409
extern: 1
intvolume: ' 88'
issue: '17'
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/math-ph/0112032
month: '04'
oa: 1
page: 1704091 - 1704094
publication: Physical Review Letters
publication_status: published
publisher: American Physical Society
publist_id: '4577'
quality_controlled: 0
status: public
title: Proof of Bose-Einstein condensation for dilute trapped gases
type: journal_article
volume: 88
year: '2002'
...
---
_id: '2350'
abstract:
- lang: eng
text: Using the Pauli-Fierz model of non-relativistic quantum electrodynamics, we
calculate the binding energy of an electron in the field of a nucleus of charge
Z and in presence of the quantized radiation field. We consider the case of small
coupling constant α, but fixed Zα and ultraviolet cut-off Λ. We prove that after
renormalizing the mass the binding energy has, to leading order in α, a finite
limit as Λ goes to infinity; i.e., the cut-off can be removed. The expression
for the ground state energy shift thus obtained agrees with Bethe's formula for
small values of Zα, but shows a different behavior for bigger values.
acknowledgement: "We are grateful to Elliott Lieb for helpful discussions. C.H. was
supported by a Marie Curie Fellowship of the European Community programme “Improving
Human Research Potential and the Socioeconomic Knowledge Base” under contract number
HPMFCT-2000-00660 and by the Deutsche Forschungsgemeinschaft, and acknowledges kind
hospitality at Princeton University, where part of this work was done. R.S. was
supported by the Austrian Science Fund in the form of an Erwin Schrödinger Fellowship.\r\n"
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Christian
full_name: Hainzl, Christian
last_name: Hainzl
- first_name: Robert
full_name: Seiringer, Robert
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: Hainzl C, Seiringer R. Mass renormalization and energy level shift in non-relativistic
QED. Advances in Theoretical and Mathematical Physics. 2002;6(5):847-871.
doi:10.4310/ATMP.2002.v6.n5.a3
apa: Hainzl, C., & Seiringer, R. (2002). Mass renormalization and energy level
shift in non-relativistic QED. Advances in Theoretical and Mathematical Physics.
International Press. https://doi.org/10.4310/ATMP.2002.v6.n5.a3
chicago: Hainzl, Christian, and Robert Seiringer. “Mass Renormalization and Energy
Level Shift in Non-Relativistic QED.” Advances in Theoretical and Mathematical
Physics. International Press, 2002. https://doi.org/10.4310/ATMP.2002.v6.n5.a3.
ieee: C. Hainzl and R. Seiringer, “Mass renormalization and energy level shift in
non-relativistic QED,” Advances in Theoretical and Mathematical Physics,
vol. 6, no. 5. International Press, pp. 847–871, 2002.
ista: Hainzl C, Seiringer R. 2002. Mass renormalization and energy level shift in
non-relativistic QED. Advances in Theoretical and Mathematical Physics. 6(5),
847–871.
mla: Hainzl, Christian, and Robert Seiringer. “Mass Renormalization and Energy Level
Shift in Non-Relativistic QED.” Advances in Theoretical and Mathematical Physics,
vol. 6, no. 5, International Press, 2002, pp. 847–71, doi:10.4310/ATMP.2002.v6.n5.a3.
short: C. Hainzl, R. Seiringer, Advances in Theoretical and Mathematical Physics
6 (2002) 847–871.
date_created: 2018-12-11T11:57:09Z
date_published: 2002-09-01T00:00:00Z
date_updated: 2023-07-26T08:29:28Z
day: '01'
doi: 10.4310/ATMP.2002.v6.n5.a3
extern: '1'
external_id:
arxiv:
- math-ph/0205044v3
intvolume: ' 6'
issue: '5'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/math-ph/0205044
month: '09'
oa: 1
oa_version: Published Version
page: 847 - 871
publication: Advances in Theoretical and Mathematical Physics
publication_identifier:
issn:
- 1095-0761
publication_status: published
publisher: International Press
publist_id: '4574'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Mass renormalization and energy level shift in non-relativistic QED
type: journal_article
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 6
year: '2002'
...
---
_id: '2351'
abstract:
- lang: eng
text: We study the Gross-Pitaevskii functional for a rotating two-dimensional Bose
gas in a trap. We prove that there is a breaking of the rotational symmetry in
the ground state; more precisely, for any value of the angular velocity and for
large enough values of the interaction strength, the ground state of the functional
is not an eigenfunction of the angular momentum. This has interesting consequences
on the Bose gas with spin; in particular, the ground state energy depends non-trivially
on the number of spin components, and the different components do not have the
same wave function. For the special case of a harmonic trap potential, we give
explicit upper and lower bounds on the critical coupling constant for symmetry
breaking.
author:
- first_name: Robert
full_name: Robert Seiringer
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: Seiringer R. Gross-Pitaevskii theory of the rotating Bose gas. Communications
in Mathematical Physics. 2002;229(3):491-509. doi:10.1007/s00220-002-0695-2
apa: Seiringer, R. (2002). Gross-Pitaevskii theory of the rotating Bose gas. Communications
in Mathematical Physics. Springer. https://doi.org/10.1007/s00220-002-0695-2
chicago: Seiringer, Robert. “Gross-Pitaevskii Theory of the Rotating Bose Gas.”
Communications in Mathematical Physics. Springer, 2002. https://doi.org/10.1007/s00220-002-0695-2.
ieee: R. Seiringer, “Gross-Pitaevskii theory of the rotating Bose gas,” Communications
in Mathematical Physics, vol. 229, no. 3. Springer, pp. 491–509, 2002.
ista: Seiringer R. 2002. Gross-Pitaevskii theory of the rotating Bose gas. Communications
in Mathematical Physics. 229(3), 491–509.
mla: Seiringer, Robert. “Gross-Pitaevskii Theory of the Rotating Bose Gas.” Communications
in Mathematical Physics, vol. 229, no. 3, Springer, 2002, pp. 491–509, doi:10.1007/s00220-002-0695-2.
short: R. Seiringer, Communications in Mathematical Physics 229 (2002) 491–509.
date_created: 2018-12-11T11:57:09Z
date_published: 2002-09-01T00:00:00Z
date_updated: 2021-01-12T06:56:57Z
day: '01'
doi: 10.1007/s00220-002-0695-2
extern: 1
intvolume: ' 229'
issue: '3'
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/math-ph/0110010
month: '09'
oa: 1
page: 491 - 509
publication: Communications in Mathematical Physics
publication_status: published
publisher: Springer
publist_id: '4575'
quality_controlled: 0
status: public
title: Gross-Pitaevskii theory of the rotating Bose gas
type: journal_article
volume: 229
year: '2002'
...
---
_id: '2352'
abstract:
- lang: eng
text: We present a generalization of the Fefferman-de la Llave decomposition of
the Coulomb potential to quite arbitrary radial functions V on ℝn going to zero
at infinity. This generalized decomposition can be used to extend previous results
on N-body quantum systems with Coulomb interaction to a more general class of
interactions. As an example of such an application, we derive the high density
asymptotics of the ground state energy of jellium with Yukawa interaction in the
thermodynamic limit, using a correlation estimate by Graf and Solovej.
author:
- first_name: Christian
full_name: Hainzl, Christian
last_name: Hainzl
- first_name: Robert
full_name: Robert Seiringer
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
citation:
ama: Hainzl C, Seiringer R. General decomposition of radial functions on ℝn and
applications to N-body quantum systems. Letters in Mathematical Physics.
2002;61(1):75-84. doi:10.1023/A:1020204818938
apa: Hainzl, C., & Seiringer, R. (2002). General decomposition of radial functions
on ℝn and applications to N-body quantum systems. Letters in Mathematical Physics.
Springer. https://doi.org/10.1023/A:1020204818938
chicago: Hainzl, Christian, and Robert Seiringer. “General Decomposition of Radial
Functions on ℝn and Applications to N-Body Quantum Systems.” Letters in Mathematical
Physics. Springer, 2002. https://doi.org/10.1023/A:1020204818938.
ieee: C. Hainzl and R. Seiringer, “General decomposition of radial functions on
ℝn and applications to N-body quantum systems,” Letters in Mathematical Physics,
vol. 61, no. 1. Springer, pp. 75–84, 2002.
ista: Hainzl C, Seiringer R. 2002. General decomposition of radial functions on
ℝn and applications to N-body quantum systems. Letters in Mathematical Physics.
61(1), 75–84.
mla: Hainzl, Christian, and Robert Seiringer. “General Decomposition of Radial Functions
on ℝn and Applications to N-Body Quantum Systems.” Letters in Mathematical
Physics, vol. 61, no. 1, Springer, 2002, pp. 75–84, doi:10.1023/A:1020204818938.
short: C. Hainzl, R. Seiringer, Letters in Mathematical Physics 61 (2002) 75–84.
date_created: 2018-12-11T11:57:09Z
date_published: 2002-07-01T00:00:00Z
date_updated: 2021-01-12T06:56:58Z
day: '01'
doi: 10.1023/A:1020204818938
extern: 1
intvolume: ' 61'
issue: '1'
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/math-ph/0107011
month: '07'
oa: 1
page: 75 - 84
publication: Letters in Mathematical Physics
publication_status: published
publisher: Springer
publist_id: '4576'
quality_controlled: 0
status: public
title: General decomposition of radial functions on ℝn and applications to N-body
quantum systems
type: journal_article
volume: 61
year: '2002'
...
---
_id: '2353'
abstract:
- lang: eng
text: A commonly used theoretical definition of superfluidity in the ground state
of a Bose gas is based on the response of the system to an imposed velocity field
or, equivalently, to twisted boundary conditions in a box. We are able to carry
out this program in the case of a dilute interacting Bose gas in a trap, and we
prove that a gas with repulsive interactions is 100% superfluid in the dilute
limit in which the Gross-Pitaevskii equation is exact. This is the first example
in an experimentally realistic continuum model in which superfluidity is rigorously
verified.
acknowledgement: E.H.L. was partially supported by the U.S. National Science Foundation,
Grant No. PHY 98-20650. R.S. was supported by the Austrian Science Fund in the from
of an Erwin Schrödinger fellowship.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Élliott
full_name: Lieb, Élliott
last_name: Lieb
- first_name: Robert
full_name: Seiringer, Robert
id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
last_name: Seiringer
orcid: 0000-0002-6781-0521
- first_name: Jakob
full_name: Yngvason, Jakob
last_name: Yngvason
citation:
ama: Lieb É, Seiringer R, Yngvason J. Superfluidity in dilute trapped Bose gases.
Physical Review B - Condensed Matter and Materials Physics. 2002;66(13).
doi:10.1103/PhysRevB.66.134529
apa: Lieb, É., Seiringer, R., & Yngvason, J. (2002). Superfluidity in dilute
trapped Bose gases. Physical Review B - Condensed Matter and Materials Physics.
American Physical Society. https://doi.org/10.1103/PhysRevB.66.134529
chicago: Lieb, Élliott, Robert Seiringer, and Jakob Yngvason. “Superfluidity in
Dilute Trapped Bose Gases.” Physical Review B - Condensed Matter and Materials
Physics. American Physical Society, 2002. https://doi.org/10.1103/PhysRevB.66.134529.
ieee: É. Lieb, R. Seiringer, and J. Yngvason, “Superfluidity in dilute trapped Bose
gases,” Physical Review B - Condensed Matter and Materials Physics, vol.
66, no. 13. American Physical Society, 2002.
ista: Lieb É, Seiringer R, Yngvason J. 2002. Superfluidity in dilute trapped Bose
gases. Physical Review B - Condensed Matter and Materials Physics. 66(13).
mla: Lieb, Élliott, et al. “Superfluidity in Dilute Trapped Bose Gases.” Physical
Review B - Condensed Matter and Materials Physics, vol. 66, no. 13, American
Physical Society, 2002, doi:10.1103/PhysRevB.66.134529.
short: É. Lieb, R. Seiringer, J. Yngvason, Physical Review B - Condensed Matter
and Materials Physics 66 (2002).
date_created: 2018-12-11T11:57:10Z
date_published: 2002-10-01T00:00:00Z
date_updated: 2023-07-25T12:05:47Z
day: '01'
doi: 10.1103/PhysRevB.66.134529
extern: '1'
external_id:
arxiv:
- cond-mat/0205570
intvolume: ' 66'
issue: '13'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://arxiv.org/abs/cond-mat/0205570
month: '10'
oa: 1
oa_version: None
publication: Physical Review B - Condensed Matter and Materials Physics
publication_identifier:
issn:
- 0163-1829
publication_status: published
publisher: American Physical Society
publist_id: '4573'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Superfluidity in dilute trapped Bose gases
type: journal_article
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 66
year: '2002'
...
---
_id: '2420'
abstract:
- lang: eng
text: 'A corner cut in dimension d is a finite subset of N0d that can be separated
from its complement in N0d by an affine hyperplane disjoint from N0d. Corner cuts
were first investigated by Onn and Sturmfels [Adv. Appl. Math. 23 (1999) 29-48],
their original motivation stemmed from computational commutative algebra. Let
us write (Nd0k)cut for the set of corner cuts of cardinality k; in the computational
geometer''s terminology, these are the k-sets of N0d. Among other things, Onn
and Sturmfels give an upper bound of O(k2d(d-1)/(d+1)) for the size of (Nd0k)cut
when the dimension is fixed. In two dimensions, it is known (see [Corteel et al.,
Adv. Appl. Math. 23 (1) (1999) 49-53]) that #(Nd0k)cut = Θ(k log k). We will see
that in general, for any fixed dimension d, the order of magnitude of #(Nd0k)cut
is between kd-1 log k and (k log k)d-1. (It has been communicated to me that the
same bounds have been found independently by G. Rémond.) In fact, the elements
of (Nd0k)cut correspond to the vertices of a certain polytope, and what our proof
shows is that the above upper bound holds for the total number of flags of that
polytope.'
acknowledgement: "I first learned about corner cuts in a seminar talk in which Artur
Andrzejak\r\npresented the results from [6]. My work was initiated by that presentation
and\r\nby the discussions that followed it. I also thank Komei Fukuda, Ingo Schurr,
and\r\nEmo Welzl for helpful comments and discussions."
article_processing_charge: No
article_type: original
author:
- first_name: Uli
full_name: Wagner, Uli
id: 36690CA2-F248-11E8-B48F-1D18A9856A87
last_name: Wagner
orcid: 0000-0002-1494-0568
citation:
ama: Wagner U. On the number of corner cuts. Advances in Applied Mathematics.
2002;29(2):152-161. doi:10.1016/S0196-8858(02)00014-3
apa: Wagner, U. (2002). On the number of corner cuts. Advances in Applied Mathematics.
ACM. https://doi.org/10.1016/S0196-8858(02)00014-3
chicago: Wagner, Uli. “On the Number of Corner Cuts.” Advances in Applied Mathematics.
ACM, 2002. https://doi.org/10.1016/S0196-8858(02)00014-3.
ieee: U. Wagner, “On the number of corner cuts,” Advances in Applied Mathematics,
vol. 29, no. 2. ACM, pp. 152–161, 2002.
ista: Wagner U. 2002. On the number of corner cuts. Advances in Applied Mathematics.
29(2), 152–161.
mla: Wagner, Uli. “On the Number of Corner Cuts.” Advances in Applied Mathematics,
vol. 29, no. 2, ACM, 2002, pp. 152–61, doi:10.1016/S0196-8858(02)00014-3.
short: U. Wagner, Advances in Applied Mathematics 29 (2002) 152–161.
date_created: 2018-12-11T11:57:33Z
date_published: 2002-08-01T00:00:00Z
date_updated: 2023-07-25T11:55:42Z
day: '01'
doi: 10.1016/S0196-8858(02)00014-3
extern: '1'
intvolume: ' 29'
issue: '2'
language:
- iso: eng
month: '08'
oa_version: None
page: 152 - 161
publication: Advances in Applied Mathematics
publication_identifier:
issn:
- 0196-8858
publication_status: published
publisher: ACM
publist_id: '4505'
quality_controlled: '1'
scopus_import: '1'
status: public
title: On the number of corner cuts
type: journal_article
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 29
year: '2002'
...
---
_id: '2421'
abstract:
- lang: eng
text: Intersection graphs of disks and of line segments, respectively, have been
well studied, because of both, practical applications and theoretically interesting
properties of these graphs. Despite partial results, the complexity status of
the Clique problem for these two graph classes is still open. Here, we consider
the Clique problem for intersection graphs of ellipses which in a sense, interpolate
between disc and ellipses, and show that it is APX-hard in that case. Moreover,
this holds even if for all ellipses, the ratio of the larger over the smaller
radius is some prescribed number. To our knowledge, this is the first hardness
result for the Clique problem in intersection graphs of objects with finite description
complexity. We also describe a simple approximation algorithm for the case of
ellipses for which the ratio of radii is bounded.
alternative_title:
- LNCS
article_processing_charge: No
author:
- first_name: Christoph
full_name: Ambühl, Christoph
last_name: Ambühl
- first_name: Uli
full_name: Wagner, Uli
id: 36690CA2-F248-11E8-B48F-1D18A9856A87
last_name: Wagner
orcid: 0000-0002-1494-0568
citation:
ama: 'Ambühl C, Wagner U. On the Clique problem in intersection graphs of ellipses.
In: Proceedings of the 13th International Symposium on Algorithms and Computation.
Vol 2518. Springer; 2002:489-500. doi:10.1007/3-540-36136-7_43'
apa: 'Ambühl, C., & Wagner, U. (2002). On the Clique problem in intersection
graphs of ellipses. In Proceedings of the 13th International Symposium on Algorithms
and Computation (Vol. 2518, pp. 489–500). Vancouver, Canada: Springer. https://doi.org/10.1007/3-540-36136-7_43'
chicago: Ambühl, Christoph, and Uli Wagner. “On the Clique Problem in Intersection
Graphs of Ellipses.” In Proceedings of the 13th International Symposium on
Algorithms and Computation, 2518:489–500. Springer, 2002. https://doi.org/10.1007/3-540-36136-7_43.
ieee: C. Ambühl and U. Wagner, “On the Clique problem in intersection graphs of
ellipses,” in Proceedings of the 13th International Symposium on Algorithms
and Computation, Vancouver, Canada, 2002, vol. 2518, pp. 489–500.
ista: 'Ambühl C, Wagner U. 2002. On the Clique problem in intersection graphs of
ellipses. Proceedings of the 13th International Symposium on Algorithms and Computation.
ISAAC: International Symposium on Algorithms and Computation, LNCS, vol. 2518,
489–500.'
mla: Ambühl, Christoph, and Uli Wagner. “On the Clique Problem in Intersection Graphs
of Ellipses.” Proceedings of the 13th International Symposium on Algorithms
and Computation, vol. 2518, Springer, 2002, pp. 489–500, doi:10.1007/3-540-36136-7_43.
short: C. Ambühl, U. Wagner, in:, Proceedings of the 13th International Symposium
on Algorithms and Computation, Springer, 2002, pp. 489–500.
conference:
end_date: 2002-11-23
location: Vancouver, Canada
name: 'ISAAC: International Symposium on Algorithms and Computation'
start_date: 2002-11-21
date_created: 2018-12-11T11:57:34Z
date_published: 2002-01-01T00:00:00Z
date_updated: 2023-07-25T11:48:36Z
day: '01'
doi: 10.1007/3-540-36136-7_43
extern: '1'
intvolume: ' 2518'
language:
- iso: eng
month: '01'
oa_version: None
page: 489 - 500
publication: Proceedings of the 13th International Symposium on Algorithms and Computation
publication_identifier:
isbn:
- '9783540001423'
publication_status: published
publisher: Springer
publist_id: '4504'
quality_controlled: '1'
scopus_import: '1'
status: public
title: On the Clique problem in intersection graphs of ellipses
type: conference
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 2518
year: '2002'
...
---
_id: '2613'
abstract:
- lang: eng
text: In this investigation, we report identification and characterization of a
95 kDa postsynaptic density protein (PSD-95)/discs-large/ ZO-1 (PDZ) domain-containing
protein termed tamalin, also recently named GRP1-associated scaffold protein (GRASP),
that interacts with group 1 metabotropic glutamate receptors (mGluRs). The yeast
two-hybrid system and in vitro pull-down assays indicated that the PDZ domain-containing,
amino-terminal half of tamalin directly binds to the class I PDZ-binding motif
of group 1 mGluRs. The C-terminal half of tamalin also bound to cytohesins, the
members of guanine nucleotide exchange factors (GEFs) specific for the ADP-ribosylation
factor (ARF) family of small GTP-binding proteins. Tamalin mRNA is expressed predominantly
in the telencephalic region and highly overlaps with the expression of group 1
mGluR mRNAs. Both tamalin and cytohesin-2 were enriched and codistributed with
mGluR1a in postsynaptic membrane fractions. Importantly, recombinant and native
mGluR1a/tamalin/cytohesin-2 complexes were coimmunoprecipitated from transfected
COS-7 cells and rat brain tissue, respectively. Transfection of tamalin and mutant
tamalin lacking a cytohesin-binding domain caused an increase and decrease in
cell-surface expression of mGluR1a in COS-7 cells, respectively. Furthermore,
adenovirus-mediated expression of tamalin and dominant-negative tamalin facilitated
and reduced the neuritic distribution of endogenous mGluR5 in cultured hippocampal
neurons, respectively. The results indicate that tamalin plays a key role in the
association of group 1 mGluRs with the ARF-specific GEF proteins and contributes
to intracellular trafficking and the macromolecular organization of group 1 mGluRs
at synapses.
acknowledgement: This work was supported in part by research grants from the Ministry
of Education, Science and Culture of Japan. We thank Bert Vogelstein for providing
adenoviral recombination vectors and Haruhiko Bito for a gift of the enolase promoter
and technical advice. We are grateful to Atsushi Nishimune and Satoshi Kaneko for
technical advice and Kumlesh K. Dev for careful reading of this manuscript.
article_processing_charge: No
article_type: original
author:
- first_name: Jun
full_name: Kitano, Jun
last_name: Kitano
- first_name: Kouji
full_name: Kimura, Kouji
last_name: Kimura
- first_name: Yoshimitsu
full_name: Yamazaki, Yoshimitsu
last_name: Yamazaki
- first_name: Takeshi
full_name: Soda, Takeshi
last_name: Soda
- first_name: Ryuichi
full_name: Shigemoto, Ryuichi
id: 499F3ABC-F248-11E8-B48F-1D18A9856A87
last_name: Shigemoto
orcid: 0000-0001-8761-9444
- first_name: Yoshiaki
full_name: Nakajima, Yoshiaki
last_name: Nakajima
- first_name: Shigetada
full_name: Nakanishi, Shigetada
last_name: Nakanishi
citation:
ama: Kitano J, Kimura K, Yamazaki Y, et al. Tamalin, a PDZ domain-containing protein,
links a protein complex formation of group 1 metabotropic glutamate receptors
and the guanine nucleotide exchange factor cytohesins. Journal of Neuroscience.
2002;22(4):1280-1289. doi:10.1523/JNEUROSCI.22-04-01280.2002
apa: Kitano, J., Kimura, K., Yamazaki, Y., Soda, T., Shigemoto, R., Nakajima, Y.,
& Nakanishi, S. (2002). Tamalin, a PDZ domain-containing protein, links a
protein complex formation of group 1 metabotropic glutamate receptors and the
guanine nucleotide exchange factor cytohesins. Journal of Neuroscience.
Society for Neuroscience. https://doi.org/10.1523/JNEUROSCI.22-04-01280.2002
chicago: Kitano, Jun, Kouji Kimura, Yoshimitsu Yamazaki, Takeshi Soda, Ryuichi Shigemoto,
Yoshiaki Nakajima, and Shigetada Nakanishi. “Tamalin, a PDZ Domain-Containing
Protein, Links a Protein Complex Formation of Group 1 Metabotropic Glutamate Receptors
and the Guanine Nucleotide Exchange Factor Cytohesins.” Journal of Neuroscience.
Society for Neuroscience, 2002. https://doi.org/10.1523/JNEUROSCI.22-04-01280.2002.
ieee: J. Kitano et al., “Tamalin, a PDZ domain-containing protein, links
a protein complex formation of group 1 metabotropic glutamate receptors and the
guanine nucleotide exchange factor cytohesins,” Journal of Neuroscience,
vol. 22, no. 4. Society for Neuroscience, pp. 1280–1289, 2002.
ista: Kitano J, Kimura K, Yamazaki Y, Soda T, Shigemoto R, Nakajima Y, Nakanishi
S. 2002. Tamalin, a PDZ domain-containing protein, links a protein complex formation
of group 1 metabotropic glutamate receptors and the guanine nucleotide exchange
factor cytohesins. Journal of Neuroscience. 22(4), 1280–1289.
mla: Kitano, Jun, et al. “Tamalin, a PDZ Domain-Containing Protein, Links a Protein
Complex Formation of Group 1 Metabotropic Glutamate Receptors and the Guanine
Nucleotide Exchange Factor Cytohesins.” Journal of Neuroscience, vol. 22,
no. 4, Society for Neuroscience, 2002, pp. 1280–89, doi:10.1523/JNEUROSCI.22-04-01280.2002.
short: J. Kitano, K. Kimura, Y. Yamazaki, T. Soda, R. Shigemoto, Y. Nakajima, S.
Nakanishi, Journal of Neuroscience 22 (2002) 1280–1289.
date_created: 2018-12-11T11:58:40Z
date_published: 2002-02-15T00:00:00Z
date_updated: 2023-07-25T11:34:46Z
day: '15'
doi: 10.1523/JNEUROSCI.22-04-01280.2002
extern: '1'
external_id:
pmid:
- '11850456'
intvolume: ' 22'
issue: '4'
language:
- iso: eng
month: '02'
oa_version: None
page: 1280 - 1289
pmid: 1
publication: Journal of Neuroscience
publication_identifier:
issn:
- 0270-6474
publication_status: published
publisher: Society for Neuroscience
publist_id: '4285'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Tamalin, a PDZ domain-containing protein, links a protein complex formation
of group 1 metabotropic glutamate receptors and the guanine nucleotide exchange
factor cytohesins
type: journal_article
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 22
year: '2002'
...
---
_id: '2614'
abstract:
- lang: eng
text: Metabotropic glutamate receptors (mGluRs) from group III reduce glutamate
release. Because these receptors reduce cAMP levels, we explored whether this
signaling pathway contributes to release inhibition caused by mGluRs with low
affinity for L-2-amino-4-phosphonobutyrate (L-AP4). In biochemical experiments
with the population of cerebrocortical nerve terminals we find that L-AP4 (1 mM)
inhibited the Ca2+dependent-evoked release of glutamate by 25%. This inhibitory
effect was largely prevented by the pertussis toxin but was insensitive to inhibitors
of protein kinase C bisindolylmaleimide and protein kinase A H-89. Furthermore,
this inhibition was associated with reduction in N-type Ca2+ channel activity
in the absence of any detectable change in cAMP levels. In the presence of forskolin,
however, L-AP4 decreased the levels of cAMP. The activation of this additional
signaling pathway was very efficient in counteracting the facilitation of glutamate
release induced either by forskolin or the β-adrenergic receptor agonist isoproterenol.
Imaging experiments to measure Ca2+ dynamics in single nerve terminals showed
that L-AP4 strongly reduced the Ca2+ response in 28% of the nerve terminals. Moreover,
immunochemical experiments showed that 25-35% of the nerve terminals that were
immunopositive to synaptophysin were also immunoreactive to the low affinity L-AP4-sensitive
mGluR7. Then, mGluR7 mediates the inhibition of glutamate release caused by 1
mM L-AP4, primarily by a strong inhibition of Ca2+ channels, although high cAMP
uncovers the receptor ability to decrease cAMP.
acknowledgement: We thank Dr. Enrique Castro from Las Palmas University for critical
reading of the manuscript and M. Sefton for editorial assistance.
article_processing_charge: No
article_type: original
author:
- first_name: Carmelo
full_name: Millán, Carmelo
last_name: Millán
- first_name: Rafael
full_name: Luján, Rafael
last_name: Luján
- first_name: Ryuichi
full_name: Shigemoto, Ryuichi
id: 499F3ABC-F248-11E8-B48F-1D18A9856A87
last_name: Shigemoto
orcid: 0000-0001-8761-9444
- first_name: José
full_name: Sánchez Prieto, José
last_name: Sánchez Prieto
citation:
ama: Millán C, Luján R, Shigemoto R, Sánchez Prieto J. The inhibition of glutamate
release by metabotropic glutamate receptor 7 affects both [Ca2+]c and cAMP. Evidence
for a strong reduction of Ca2+ entry in single nerve terminals. Journal of
Biological Chemistry. 2002;277(16):14092-14101. doi:10.1074/jbc.M109044200
apa: Millán, C., Luján, R., Shigemoto, R., & Sánchez Prieto, J. (2002). The
inhibition of glutamate release by metabotropic glutamate receptor 7 affects both
[Ca2+]c and cAMP. Evidence for a strong reduction of Ca2+ entry in single nerve
terminals. Journal of Biological Chemistry. American Society for Biochemistry
and Molecular Biology. https://doi.org/10.1074/jbc.M109044200
chicago: Millán, Carmelo, Rafael Luján, Ryuichi Shigemoto, and José Sánchez Prieto.
“The Inhibition of Glutamate Release by Metabotropic Glutamate Receptor 7 Affects
Both [Ca2+]c and CAMP. Evidence for a Strong Reduction of Ca2+ Entry in Single
Nerve Terminals.” Journal of Biological Chemistry. American Society for
Biochemistry and Molecular Biology, 2002. https://doi.org/10.1074/jbc.M109044200.
ieee: C. Millán, R. Luján, R. Shigemoto, and J. Sánchez Prieto, “The inhibition
of glutamate release by metabotropic glutamate receptor 7 affects both [Ca2+]c
and cAMP. Evidence for a strong reduction of Ca2+ entry in single nerve terminals,”
Journal of Biological Chemistry, vol. 277, no. 16. American Society for
Biochemistry and Molecular Biology, pp. 14092–14101, 2002.
ista: Millán C, Luján R, Shigemoto R, Sánchez Prieto J. 2002. The inhibition of
glutamate release by metabotropic glutamate receptor 7 affects both [Ca2+]c and
cAMP. Evidence for a strong reduction of Ca2+ entry in single nerve terminals.
Journal of Biological Chemistry. 277(16), 14092–14101.
mla: Millán, Carmelo, et al. “The Inhibition of Glutamate Release by Metabotropic
Glutamate Receptor 7 Affects Both [Ca2+]c and CAMP. Evidence for a Strong Reduction
of Ca2+ Entry in Single Nerve Terminals.” Journal of Biological Chemistry,
vol. 277, no. 16, American Society for Biochemistry and Molecular Biology, 2002,
pp. 14092–101, doi:10.1074/jbc.M109044200.
short: C. Millán, R. Luján, R. Shigemoto, J. Sánchez Prieto, Journal of Biological
Chemistry 277 (2002) 14092–14101.
date_created: 2018-12-11T11:58:41Z
date_published: 2002-04-19T00:00:00Z
date_updated: 2023-07-25T10:16:44Z
day: '19'
ddc:
- '570'
doi: 10.1074/jbc.M109044200
extern: '1'
external_id:
pmid:
- '11825890'
file:
- access_level: open_access
checksum: 0290fcbbd9153ec654185b0c856f214c
content_type: application/pdf
creator: alisjak
date_created: 2023-07-25T10:13:16Z
date_updated: 2023-07-25T10:13:16Z
file_id: '13309'
file_name: 2002_JBC_Millan.pdf
file_size: 2105520
relation: main_file
success: 1
file_date_updated: 2023-07-25T10:13:16Z
has_accepted_license: '1'
intvolume: ' 277'
issue: '16'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
page: 14092 - 14101
pmid: 1
publication: Journal of Biological Chemistry
publication_identifier:
issn:
- 0021-9258
publication_status: published
publisher: American Society for Biochemistry and Molecular Biology
publist_id: '4284'
quality_controlled: '1'
scopus_import: '1'
status: public
title: The inhibition of glutamate release by metabotropic glutamate receptor 7 affects
both [Ca2+]c and cAMP. Evidence for a strong reduction of Ca2+ entry in single nerve
terminals
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: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 277
year: '2002'
...
---
_id: '1737'
abstract:
- lang: eng
text: A new solvent-free composite polymer electrolyte consisting of high-molecular
mass polyethylene oxide (PEO) filled with titanium oxide and containing LiI and
I2 was developed. The introduction of the inorganic filler (TiO2 Degussa P25)
into the polymer matrix produces dramatic morphological changes to the host polymer
structure. Upon addition of the inorganic oxide, the surface roughness increases,
with respect to the original polymer and in parallel, the fractal dimension decreases.
Both the thermograms and the atomic force microscope (AFM) pictures confirm the
amorphicity of the composite electrolyte. The polymer sub-units are held together
in a parallel orientation, forming straight long chains of about 500 nm in width,
along which TiO2 spherical particles of about 20-25 nm in diameter are distributed.
The polymer chains separated by the titania particles are arranged in a three-dimensional,
mechanically stable network, that creates free space and voids into which the
iodide/triodide anions can easily migrate. All solid-state dye-sensitized solar
cells fabricated using this composite electrolyte present high efficiencies (typical
maximum incident photon to current efficiency (IPCE) as high as 40% at 520 nm
and overall conversion efficiency (η) of 0.96% (Voc = 0.67 V, Jsc = 2.050 mA/cm2,
FF = 39%) under direct solar irradiation. Further improvement of the photovoltaic
performance is expected by optimization of the electrolyte parameters and of the
cell assembly.
acknowledgement: Financial support from NCSR “Demokritos” (Dimoerevna 598 project),
Empeirikeion Foundation and General Secretariat for Research and Technology of Greece
(EPET II, Greece–France and Greece–Czech Republic bilateral collaboration projects)
is also greatly acknowledged. G. Katsaros thanks the Greek State Scholarships Foundation
(IKY) for fellowship allowance
article_processing_charge: No
author:
- first_name: Georgios
full_name: Katsaros, Georgios
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
- first_name: Thomas
full_name: Stergiopoulos, Thomas
last_name: Stergiopoulos
- first_name: Iannis
full_name: Arabatzis, Iannis
last_name: Arabatzis
- first_name: Kyriaki
full_name: Papadokostaki, Kyriaki
last_name: Papadokostaki
- first_name: Polycarpos
full_name: Falaras, Polycarpos
last_name: Falaras
citation:
ama: 'Katsaros G, Stergiopoulos T, Arabatzis I, Papadokostaki K, Falaras P. A solvent-free
composite polymer/inorganic oxide electrolyte for high efficiency solid-state
dye-sensitized solar cells. Journal of Photochemistry and Photobiology A: Chemistry.
2002;149(1-3):191-198. doi:10.1016/S1010-6030(02)00027-8'
apa: 'Katsaros, G., Stergiopoulos, T., Arabatzis, I., Papadokostaki, K., & Falaras,
P. (2002). A solvent-free composite polymer/inorganic oxide electrolyte for high
efficiency solid-state dye-sensitized solar cells. Journal of Photochemistry
and Photobiology A: Chemistry. Elsevier. https://doi.org/10.1016/S1010-6030(02)00027-8'
chicago: 'Katsaros, Georgios, Thomas Stergiopoulos, Iannis Arabatzis, Kyriaki Papadokostaki,
and Polycarpos Falaras. “A Solvent-Free Composite Polymer/Inorganic Oxide Electrolyte
for High Efficiency Solid-State Dye-Sensitized Solar Cells.” Journal of Photochemistry
and Photobiology A: Chemistry. Elsevier, 2002. https://doi.org/10.1016/S1010-6030(02)00027-8.'
ieee: 'G. Katsaros, T. Stergiopoulos, I. Arabatzis, K. Papadokostaki, and P. Falaras,
“A solvent-free composite polymer/inorganic oxide electrolyte for high efficiency
solid-state dye-sensitized solar cells,” Journal of Photochemistry and Photobiology
A: Chemistry, vol. 149, no. 1–3. Elsevier, pp. 191–198, 2002.'
ista: 'Katsaros G, Stergiopoulos T, Arabatzis I, Papadokostaki K, Falaras P. 2002.
A solvent-free composite polymer/inorganic oxide electrolyte for high efficiency
solid-state dye-sensitized solar cells. Journal of Photochemistry and Photobiology
A: Chemistry. 149(1–3), 191–198.'
mla: 'Katsaros, Georgios, et al. “A Solvent-Free Composite Polymer/Inorganic Oxide
Electrolyte for High Efficiency Solid-State Dye-Sensitized Solar Cells.” Journal
of Photochemistry and Photobiology A: Chemistry, vol. 149, no. 1–3, Elsevier,
2002, pp. 191–98, doi:10.1016/S1010-6030(02)00027-8.'
short: 'G. Katsaros, T. Stergiopoulos, I. Arabatzis, K. Papadokostaki, P. Falaras,
Journal of Photochemistry and Photobiology A: Chemistry 149 (2002) 191–198.'
date_created: 2018-12-11T11:53:44Z
date_published: 2002-06-28T00:00:00Z
date_updated: 2023-07-26T08:56:55Z
day: '28'
doi: 10.1016/S1010-6030(02)00027-8
extern: '1'
intvolume: ' 149'
issue: 1-3
language:
- iso: eng
month: '06'
oa_version: None
page: 191 - 198
publication: 'Journal of Photochemistry and Photobiology A: Chemistry'
publication_identifier:
issn:
- 1010-6030
publication_status: published
publisher: Elsevier
publist_id: '5387'
status: public
title: A solvent-free composite polymer/inorganic oxide electrolyte for high efficiency
solid-state dye-sensitized solar cells
type: journal_article
user_id: ea97e931-d5af-11eb-85d4-e6957dddbf17
volume: 149
year: '2002'
...
---
_id: '1738'
abstract:
- lang: eng
text: New dyes of the type Ru(II)(bdmpp)(bpy) [where bdmpp is 2,6-bis(3,5-dimethyl-N-pyrazoyl)pyridine
and bpy is 2,2′-bipyridine-4,4′-dicarboxylic acid] are prepared and characterized
by infra-red (IR), mass (MS) and electrospray mass spectroscopy (ES-MS) as well
as 1H NMR (1D and 2D) spectroscopies. The compounds present broad and very high
intensity MLCT absorption bands in the visible and can be chemically anchored
on TiO2 films via ester-like linkage involving carboxylato groups. These complexes
have been tested with success as potential molecular antennas in dye-sensitized
solar cells. Both opaque and transparent nanocrystalline TiO2 thin film electrodes
obtained by a doctor blade technique sensitized by these complexes were incorporated
in a sandwich type regenerative photoelectrochemical solar cell containing 0.1M
LiI +0.01M I2 in propylene carbonate as well as a platinized conductive glass
counter electrode. The cell was characterized by Raman spectroscopy under anodic
and cathodic bias. Two new vibration bands were observed in the lower frequency
region. The first one at 112 cm-1 is due to tri-iodide formed on the photoactive
electrode, and the second one at 167 cm-1 is a sign of the dye/iodide interaction
and corresponds to a vibration in a chemically stable "DI" intermediate
species. Under direct sunlight illumination (solar irradiance of 60 mW/cm2) by
using a composite polymer solid state electrolyte, the cell ITO/TiO2/[Ru(II)(bdmpp)(bpy)(NCS)](PF6)/electrolyte/Pt-ITO
produced a continuous photocurrent as high as 4.29mA/cm2, and gave IPCE values
about half of the corresponding values obtained by the standard N3 dye under the
same conditions. The photovoltage is about 600 mV and the overall energy conversion
cell's efficiency is as high as 1.72%.
author:
- first_name: Polycarpos
full_name: Falaras, Polycarpos
last_name: Falaras
- first_name: Katerina
full_name: Chryssou, Katerina
last_name: Chryssou
- first_name: Thomas
full_name: Stergiopoulos, Thomas
last_name: Stergiopoulos
- first_name: Ioannis
full_name: Arabatzis, Ioannis M
last_name: Arabatzis
- first_name: Georgios
full_name: Georgios Katsaros
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
- first_name: Vincent
full_name: Catalano, Vincent J
last_name: Catalano
- first_name: Raif
full_name: Kurtaran, Raif
last_name: Kurtaran
- first_name: Anne
full_name: Hugot-Le Goff, Anne
last_name: Hugot Le Goff
- first_name: Marie
full_name: Bernard, Marie C
last_name: Bernard
citation:
ama: 'Falaras P, Chryssou K, Stergiopoulos T, et al. Dye-sensitization of titanium
dioxide thin films by Ru(II)-bpp-bpy complexes. In: Vol 4801. SPIE; 2002:125-135.
doi:10.1117/12.452446'
apa: Falaras, P., Chryssou, K., Stergiopoulos, T., Arabatzis, I., Katsaros, G.,
Catalano, V., … Bernard, M. (2002). Dye-sensitization of titanium dioxide thin
films by Ru(II)-bpp-bpy complexes (Vol. 4801, pp. 125–135). Presented at the Organic
Photovoltaics, SPIE. https://doi.org/10.1117/12.452446
chicago: Falaras, Polycarpos, Katerina Chryssou, Thomas Stergiopoulos, Ioannis Arabatzis,
Georgios Katsaros, Vincent Catalano, Raif Kurtaran, Anne Hugot Le Goff, and Marie
Bernard. “Dye-Sensitization of Titanium Dioxide Thin Films by Ru(II)-Bpp-Bpy Complexes,”
4801:125–35. SPIE, 2002. https://doi.org/10.1117/12.452446.
ieee: P. Falaras et al., “Dye-sensitization of titanium dioxide thin films
by Ru(II)-bpp-bpy complexes,” presented at the Organic Photovoltaics, 2002, vol.
4801, pp. 125–135.
ista: Falaras P, Chryssou K, Stergiopoulos T, Arabatzis I, Katsaros G, Catalano
V, Kurtaran R, Hugot Le Goff A, Bernard M. 2002. Dye-sensitization of titanium
dioxide thin films by Ru(II)-bpp-bpy complexes. Organic Photovoltaics vol. 4801,
125–135.
mla: Falaras, Polycarpos, et al. Dye-Sensitization of Titanium Dioxide Thin Films
by Ru(II)-Bpp-Bpy Complexes. Vol. 4801, SPIE, 2002, pp. 125–35, doi:10.1117/12.452446.
short: P. Falaras, K. Chryssou, T. Stergiopoulos, I. Arabatzis, G. Katsaros, V.
Catalano, R. Kurtaran, A. Hugot Le Goff, M. Bernard, in:, SPIE, 2002, pp. 125–135.
conference:
name: Organic Photovoltaics
date_created: 2018-12-11T11:53:45Z
date_published: 2002-01-01T00:00:00Z
date_updated: 2021-01-12T06:52:53Z
day: '01'
doi: 10.1117/12.452446
extern: 1
intvolume: ' 4801'
month: '01'
page: 125 - 135
publication_status: published
publisher: SPIE
publist_id: '5385'
quality_controlled: 0
status: public
title: Dye-sensitization of titanium dioxide thin films by Ru(II)-bpp-bpy complexes
type: conference
volume: 4801
year: '2002'
...
---
_id: '1739'
abstract:
- lang: eng
text: Poly(ethylene oxide)/titania polymer electrolyte based photoelectrochemical
cells have been fabricated with Ru(dcbpy)2(NCS)2 complex as the sensitizer and
nanoporous TiO2 films as photoanodes. The introduction of the titania filler into
the poly(ethylene oxide) matrix reduces the crystallinity of the polymer and enhances
the mobility of the 1-/13 - redox couple, resulting in outstanding overall conversion
efficiency (4.2% under direct sunlight illumination) of the corresponding dye-sensitized
nanocrystalline TiO2 solar cell, one of the best efficiencies reported to date
for a solid-state device.
acknowledgement: 'Financial support from NCSR “Demokritos” and GSRT-Greece is greatly
acknowledged. '
author:
- first_name: Thomas
full_name: Stergiopoulos, Thomas
last_name: Stergiopoulos
- first_name: Iannis
full_name: Arabatzis, Iannis M
last_name: Arabatzis
- first_name: Georgios
full_name: Georgios Katsaros
id: 38DB5788-F248-11E8-B48F-1D18A9856A87
last_name: Katsaros
- first_name: Polycarpos
full_name: Falaras, Polycarpos
last_name: Falaras
citation:
ama: Stergiopoulos T, Arabatzis I, Katsaros G, Falaras P. Binary Polyethylene Oxide/Titania
Solid-State Redox Electrolyte for Highly Efficient Nanocrystalline TiO2 Photoelectrochemical
Cells. Nano Letters. 2002;2(11):1259-1261. doi:10.1021/nl025798u
apa: Stergiopoulos, T., Arabatzis, I., Katsaros, G., & Falaras, P. (2002). Binary
Polyethylene Oxide/Titania Solid-State Redox Electrolyte for Highly Efficient
Nanocrystalline TiO2 Photoelectrochemical Cells. Nano Letters. American
Chemical Society. https://doi.org/10.1021/nl025798u
chicago: Stergiopoulos, Thomas, Iannis Arabatzis, Georgios Katsaros, and Polycarpos
Falaras. “Binary Polyethylene Oxide/Titania Solid-State Redox Electrolyte for
Highly Efficient Nanocrystalline TiO2 Photoelectrochemical Cells.” Nano Letters.
American Chemical Society, 2002. https://doi.org/10.1021/nl025798u.
ieee: T. Stergiopoulos, I. Arabatzis, G. Katsaros, and P. Falaras, “Binary Polyethylene
Oxide/Titania Solid-State Redox Electrolyte for Highly Efficient Nanocrystalline
TiO2 Photoelectrochemical Cells,” Nano Letters, vol. 2, no. 11. American
Chemical Society, pp. 1259–1261, 2002.
ista: Stergiopoulos T, Arabatzis I, Katsaros G, Falaras P. 2002. Binary Polyethylene
Oxide/Titania Solid-State Redox Electrolyte for Highly Efficient Nanocrystalline
TiO2 Photoelectrochemical Cells. Nano Letters. 2(11), 1259–1261.
mla: Stergiopoulos, Thomas, et al. “Binary Polyethylene Oxide/Titania Solid-State
Redox Electrolyte for Highly Efficient Nanocrystalline TiO2 Photoelectrochemical
Cells.” Nano Letters, vol. 2, no. 11, American Chemical Society, 2002,
pp. 1259–61, doi:10.1021/nl025798u.
short: T. Stergiopoulos, I. Arabatzis, G. Katsaros, P. Falaras, Nano Letters 2 (2002)
1259–1261.
date_created: 2018-12-11T11:53:45Z
date_published: 2002-11-01T00:00:00Z
date_updated: 2021-01-12T06:52:53Z
day: '01'
doi: 10.1021/nl025798u
extern: 1
intvolume: ' 2'
issue: '11'
month: '11'
page: 1259 - 1261
publication: Nano Letters
publication_status: published
publisher: American Chemical Society
publist_id: '5386'
quality_controlled: 0
status: public
title: Binary Polyethylene Oxide/Titania Solid-State Redox Electrolyte for Highly
Efficient Nanocrystalline TiO2 Photoelectrochemical Cells
type: journal_article
volume: 2
year: '2002'
...
---
_id: '17723'
abstract:
- lang: eng
text: "The recent discovery of bright quasars around redshift z=6 suggests that
black holes (BHs) with masses in excess of 10^9 Msun have already assembled at
a very early stage in the evolution of the universe. An alternative interpretation
is that these quasars are powered by less massive BHs, but their fluxes are strongly
magnified through gravitational lensing by intervening galaxies. Here we analyze
the flux distribution of the Ly alpha emission of the quasar with the highest
known redshift, SDSS 1030+0524, at z=6.28. We show that this object could not
have been magnified by lensing by more than a factor of five. The constraint arises
from the large observed size, 30 (comoving) Mpc, of the ionized region around
this quasar, and relies crucially only on the assumption that the quasar is embedded
in a largely neutral IGM. Based on the line/continuum ratio of SDSS 1030+0524,
we argue further that this quasar also cannot be beamed by a significant factor.
We conclude that the minimum mass for its resident BH is 4 x 10^8 Msun (for magnification
by a factor of five); if the mass is this low, then the quasars had to switch
on prior to redshift z=9.\r\nFrom the size of the ionized region, we are also
able to place an absolute lower bound on the age of this quasar at t > 2 x 10^7
years."
article_processing_charge: No
article_type: original
author:
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: Renyue
full_name: Cen, Renyue
last_name: Cen
citation:
ama: Haiman Z, Cen R. A constraint on the gravitational lensing magnification and
age of the redshift z = 6.28 Quasar SDSS 1030+0524. The Astrophysical Journal.
2002;578(2):702-707. doi:10.1086/342610
apa: Haiman, Z., & Cen, R. (2002). A constraint on the gravitational lensing
magnification and age of the redshift z = 6.28 Quasar SDSS 1030+0524. The Astrophysical
Journal. American Astronomical Society. https://doi.org/10.1086/342610
chicago: Haiman, Zoltán, and Renyue Cen. “A Constraint on the Gravitational Lensing
Magnification and Age of the Redshift z = 6.28 Quasar SDSS 1030+0524.” The
Astrophysical Journal. American Astronomical Society, 2002. https://doi.org/10.1086/342610.
ieee: Z. Haiman and R. Cen, “A constraint on the gravitational lensing magnification
and age of the redshift z = 6.28 Quasar SDSS 1030+0524,” The Astrophysical
Journal, vol. 578, no. 2. American Astronomical Society, pp. 702–707, 2002.
ista: Haiman Z, Cen R. 2002. A constraint on the gravitational lensing magnification
and age of the redshift z = 6.28 Quasar SDSS 1030+0524. The Astrophysical Journal.
578(2), 702–707.
mla: Haiman, Zoltán, and Renyue Cen. “A Constraint on the Gravitational Lensing
Magnification and Age of the Redshift z = 6.28 Quasar SDSS 1030+0524.” The
Astrophysical Journal, vol. 578, no. 2, American Astronomical Society, 2002,
pp. 702–07, doi:10.1086/342610.
short: Z. Haiman, R. Cen, The Astrophysical Journal 578 (2002) 702–707.
date_created: 2024-09-06T09:11:03Z
date_published: 2002-10-20T00:00:00Z
date_updated: 2024-09-25T14:06:28Z
day: '20'
doi: 10.1086/342610
extern: '1'
intvolume: ' 578'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1086/342610
month: '10'
oa: 1
oa_version: Published Version
page: 702-707
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: A constraint on the gravitational lensing magnification and age of the redshift
z = 6.28 Quasar SDSS 1030+0524
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 578
year: '2002'
...
---
_id: '17739'
abstract:
- lang: eng
text: An extensive sample of galaxy clusters will be available in the coming years,
detected through their Sunyaev-Zeldovich effect (SZE). We use a semianalytic model
to study the scientific yield of combining SZE data with X-ray and optical follow-up
observations. If clusters at a given redshift z0 can be identified with virialized,
spherical halos, they populate a well-defined "fundamental plane" (FP) in the
parameter space of the three observables virial temperature (T), total Sunyaev-Zeldovich
flux decrement (ΔSν), and angular size (θ). The location and orientation of the
FP, as well as its redshift evolution, are sensitive to both the internal evolution
of clusters and to the underlying cosmological parameters. We show that if clusters
are not standard candles (e.g., because of feedback or energy injection), then
this can be inferred from the FP. Likewise, we study the dependence of the FP
on the cosmological parameters h, σ8, and Ω0, and quantify future constraints
on these parameters. We also show that in the absence of any nongravitational
effects, the scatter in the (ΔSν,T)-plane is significantly smaller than in either
the (θ,T) or the (θ,ΔSν) planes. As a result, the ΔSν-T relation can be an exceptionally
sensitive probe of both cluster physics and cosmological parameters. A comparison
of the amount of scatter in these three scaling relations will test the origin
(cosmological vs. stochastic) of the scatter.
article_processing_charge: No
article_type: original
author:
- first_name: Licia
full_name: Verde, Licia
last_name: Verde
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
- first_name: David N.
full_name: Spergel, David N.
last_name: Spergel
citation:
ama: Verde L, Haiman Z, Spergel DN. Are clusters standard candles? Galaxy cluster
scaling relations with the Sunyaev‐Zeldovich effect. The Astrophysical Journal.
2002;581(1):5-19. doi:10.1086/344134
apa: Verde, L., Haiman, Z., & Spergel, D. N. (2002). Are clusters standard candles?
Galaxy cluster scaling relations with the Sunyaev‐Zeldovich effect. The Astrophysical
Journal. American Astronomical Society. https://doi.org/10.1086/344134
chicago: Verde, Licia, Zoltán Haiman, and David N. Spergel. “Are Clusters Standard
Candles? Galaxy Cluster Scaling Relations with the Sunyaev‐Zeldovich Effect.”
The Astrophysical Journal. American Astronomical Society, 2002. https://doi.org/10.1086/344134.
ieee: L. Verde, Z. Haiman, and D. N. Spergel, “Are clusters standard candles? Galaxy
cluster scaling relations with the Sunyaev‐Zeldovich effect,” The Astrophysical
Journal, vol. 581, no. 1. American Astronomical Society, pp. 5–19, 2002.
ista: Verde L, Haiman Z, Spergel DN. 2002. Are clusters standard candles? Galaxy
cluster scaling relations with the Sunyaev‐Zeldovich effect. The Astrophysical
Journal. 581(1), 5–19.
mla: Verde, Licia, et al. “Are Clusters Standard Candles? Galaxy Cluster Scaling
Relations with the Sunyaev‐Zeldovich Effect.” The Astrophysical Journal,
vol. 581, no. 1, American Astronomical Society, 2002, pp. 5–19, doi:10.1086/344134.
short: L. Verde, Z. Haiman, D.N. Spergel, The Astrophysical Journal 581 (2002) 5–19.
date_created: 2024-09-06T09:22:05Z
date_published: 2002-12-10T00:00:00Z
date_updated: 2024-09-26T14:09:02Z
day: '10'
doi: 10.1086/344134
extern: '1'
intvolume: ' 581'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1086/344134
month: '12'
oa: 1
oa_version: Published Version
page: 5-19
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: Are clusters standard candles? Galaxy cluster scaling relations with the Sunyaev‐Zeldovich
effect
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 581
year: '2002'
...
---
_id: '17746'
abstract:
- lang: eng
text: For a source of Lyα radiation embedded in a neutral intergalactic medium (IGM)
prior to the reionization epoch, the Lyα emission line is strongly suppressed
by the intervening IGM. The damping wing of the so-called Gunn-Peterson trough
can extend to the red side of the emission line and erase a significant fraction
of the total line flux. However, the transmitted fraction increases with the size
of the local cosmological H II region surrounding the source, and therefore with
the ionizing luminosity and age of the source. Motivated by the recent discovery
of a Lyα-emitting galaxy at a redshift z = 6.56 (Hu et al.), possibly prior to
the reionization of the IGM, we revisit the effects of a neutral IGM on the Lyα
emission line. We show that for faint sources with little or even no ionizing
continuum, a sufficiently broad (Δv ≳ 300 km s^-1) emission line can still remain
observable. In particular, the line detected by Hu et al. is consistent with a
source embedded in a neutral IGM. We provide characterizations of the asymmetry
and total transmitted flux of the Lyα line as functions of the ionizing emissivity
of its source. We argue that a statistical sample of Lyα emitters extending beyond
the reionization redshift can be a useful probe of reionization.
article_processing_charge: No
article_type: original
author:
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: Haiman Z. The detectability of high-redshift Lyα emission lines prior to the
reionization of the universe. The Astrophysical Journal. 2002;576(1):L1-L4.
doi:10.1086/343101
apa: Haiman, Z. (2002). The detectability of high-redshift Lyα emission lines prior
to the reionization of the universe. The Astrophysical Journal. American
Astronomical Society. https://doi.org/10.1086/343101
chicago: Haiman, Zoltán. “The Detectability of High-Redshift Lyα Emission Lines
Prior to the Reionization of the Universe.” The Astrophysical Journal.
American Astronomical Society, 2002. https://doi.org/10.1086/343101.
ieee: Z. Haiman, “The detectability of high-redshift Lyα emission lines prior to
the reionization of the universe,” The Astrophysical Journal, vol. 576,
no. 1. American Astronomical Society, pp. L1–L4, 2002.
ista: Haiman Z. 2002. The detectability of high-redshift Lyα emission lines prior
to the reionization of the universe. The Astrophysical Journal. 576(1), L1–L4.
mla: Haiman, Zoltán. “The Detectability of High-Redshift Lyα Emission Lines Prior
to the Reionization of the Universe.” The Astrophysical Journal, vol. 576,
no. 1, American Astronomical Society, 2002, pp. L1–4, doi:10.1086/343101.
short: Z. Haiman, The Astrophysical Journal 576 (2002) L1–L4.
date_created: 2024-09-06T09:34:46Z
date_published: 2002-07-31T00:00:00Z
date_updated: 2024-09-26T14:51:17Z
day: '31'
doi: 10.1086/343101
extern: '1'
intvolume: ' 576'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1086/343101
month: '07'
oa: 1
oa_version: Published Version
page: L1-L4
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: The detectability of high-redshift Lyα emission lines prior to the reionization
of the universe
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 576
year: '2002'
...
---
_id: '17779'
abstract:
- lang: eng
text: The first generation of stars is thought to have formed in low-mass halos
with Tvir < 10^4 K where H2 cooling is paramount. However, the efficiency of H2
formation and cooling in these halos may have been severely limited by feedback
processes. In this paper we investigate the radiative cooling and collapse of
halos with virial temperatures Tvir > 10^4 K, i.e., those that can cool in the
absence of H2 via neutral atomic lines. The evolution of these halos differs from
their less massive counterparts. Efficient atomic line radiation allows rapid
cooling to ~8000 K; subsequently the gas can contract nearly isothermally at this
temperature. In the absence of H2 molecules, the gas would likely settle into
a locally stable disk, and only disks with unusually low spin would be unstable.
However, we find that the initial atomic line cooling leaves a large, out-of-equilibrium
residual free electron fraction. This allows the molecular fraction to build up
to a universal value of x ≈ 10^-3, almost independently of initial density and
temperature. We show that this is a nonequilibrium freeze-out value that can be
understood in terms of timescale arguments. Unlike in less massive halos, H2 formation
and cooling is largely impervious to feedback from external UV fields, due to
the high initial densities achieved by atomic cooling. The newly formed molecules
cool the gas further to ~100 K and allow the gas to fragment on scales of a few
times 100 M☉. We investigate the importance of various feedback effects such as
H2 photodissociation from internal UV fields and radiation pressure due to Lyα
photon trapping, which are likely to regulate the efficiency of star formation.
article_processing_charge: No
article_type: original
author:
- first_name: S. Peng
full_name: Oh, S. Peng
last_name: Oh
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
citation:
ama: 'Oh SP, Haiman Z. Second‐generation objects in the universe: Radiative cooling
and collapse of halos with virial temperatures above 10^4 K. The Astrophysical
Journal. 2002;569(2):558-572. doi:10.1086/339393'
apa: 'Oh, S. P., & Haiman, Z. (2002). Second‐generation objects in the universe:
Radiative cooling and collapse of halos with virial temperatures above 10^4 K.
The Astrophysical Journal. American Astronomical Society. https://doi.org/10.1086/339393'
chicago: 'Oh, S. Peng, and Zoltán Haiman. “Second‐generation Objects in the Universe:
Radiative Cooling and Collapse of Halos with Virial Temperatures above 10^4 K.”
The Astrophysical Journal. American Astronomical Society, 2002. https://doi.org/10.1086/339393.'
ieee: 'S. P. Oh and Z. Haiman, “Second‐generation objects in the universe: Radiative
cooling and collapse of halos with virial temperatures above 10^4 K,” The Astrophysical
Journal, vol. 569, no. 2. American Astronomical Society, pp. 558–572, 2002.'
ista: 'Oh SP, Haiman Z. 2002. Second‐generation objects in the universe: Radiative
cooling and collapse of halos with virial temperatures above 10^4 K. The Astrophysical
Journal. 569(2), 558–572.'
mla: 'Oh, S. Peng, and Zoltán Haiman. “Second‐generation Objects in the Universe:
Radiative Cooling and Collapse of Halos with Virial Temperatures above 10^4 K.”
The Astrophysical Journal, vol. 569, no. 2, American Astronomical Society,
2002, pp. 558–72, doi:10.1086/339393.'
short: S.P. Oh, Z. Haiman, The Astrophysical Journal 569 (2002) 558–572.
date_created: 2024-09-06T10:14:24Z
date_published: 2002-04-20T00:00:00Z
date_updated: 2024-09-30T12:04:29Z
day: '20'
doi: 10.1086/339393
extern: '1'
intvolume: ' 569'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1086/339393
month: '04'
oa: 1
oa_version: Published Version
page: 558-572
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: 'Second‐generation objects in the universe: Radiative cooling and collapse
of halos with virial temperatures above 10^4 K'
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 569
year: '2002'
...
---
OA_type: free access
_id: '17798'
abstract:
- lang: eng
text: Recent discoveries by the Sloan Digital Sky Survey (SDSS) of four bright z
~ 6 quasars could constrain the mechanism by which the supermassive black holes
powering these sources are assembled. Here we compute the probability that the
fluxes of the quasars are strongly amplified by gravitational lensing and therefore
the likelihood that the black hole masses are overestimated when they are inferred
assuming Eddington luminosities. The poorly constrained shape of the intrinsic
quasar luminosity function (LF) at redshift ~6 results in a large range of possible
lensing probabilities. If the LF is either steep or extends to faint magnitudes,
the probability for amplification by a factor μ ≳ 10 (and with only one image
detectable by SDSS) can reach essentially 100%. We show that future observations,
in particular, of either the current four quasars at the high angular resolution
provided by the Hubble Space Telescope or an increased sample of ~20 z ~ 6 quasars
at the current angular resolution, should either discover several gravitational
lenses or else provide interesting new constraints on the shape of the z ~ 6 quasar
LF.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Julia M.
full_name: Comerford, Julia M.
last_name: Comerford
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
orcid: 0000-0003-3633-5403
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
citation:
ama: Comerford JM, Haiman Z, Schaye J. Constraining the Redshift z ~ 6 quasar luminosity
function using gravitational lensing. The Astrophysical Journal. 2002;580:63-72.
doi:10.1086/343116
apa: Comerford, J. M., Haiman, Z., & Schaye, J. (2002). Constraining the Redshift
z ~ 6 quasar luminosity function using gravitational lensing. The Astrophysical
Journal. American Astronomical Society. https://doi.org/10.1086/343116
chicago: Comerford, Julia M., Zoltán Haiman, and Joop Schaye. “Constraining the
Redshift z ~ 6 Quasar Luminosity Function Using Gravitational Lensing.” The
Astrophysical Journal. American Astronomical Society, 2002. https://doi.org/10.1086/343116.
ieee: J. M. Comerford, Z. Haiman, and J. Schaye, “Constraining the Redshift z ~
6 quasar luminosity function using gravitational lensing,” The Astrophysical
Journal, vol. 580. American Astronomical Society, pp. 63–72, 2002.
ista: Comerford JM, Haiman Z, Schaye J. 2002. Constraining the Redshift z ~ 6 quasar
luminosity function using gravitational lensing. The Astrophysical Journal. 580,
63–72.
mla: Comerford, Julia M., et al. “Constraining the Redshift z ~ 6 Quasar Luminosity
Function Using Gravitational Lensing.” The Astrophysical Journal, vol.
580, American Astronomical Society, 2002, pp. 63–72, doi:10.1086/343116.
short: J.M. Comerford, Z. Haiman, J. Schaye, The Astrophysical Journal 580 (2002)
63–72.
date_created: 2024-09-06T10:29:51Z
date_published: 2002-11-20T00:00:00Z
date_updated: 2024-11-12T09:40:33Z
day: '20'
doi: 10.1086/343116
extern: '1'
external_id:
arxiv:
- astro-ph/0206441
intvolume: ' 580'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.astro-ph/0206441
month: '11'
oa: 1
oa_version: Preprint
page: 63-72
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Constraining the Redshift z ~ 6 quasar luminosity function using gravitational
lensing
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 580
year: '2002'
...
---
OA_type: free access
_id: '17799'
abstract:
- lang: eng
text: The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey
that will eventually cover approximately one-quarter of the celestial sphere and
collect spectra of ≈106 galaxies, 100,000 quasars, 30,000 stars, and 30,000 serendipity
targets. In 2001 June, the SDSS released to the general astronomical community
its early data release, roughly 462 deg2 of imaging data including almost 14 million
detected objects and 54,008 follow-up spectra. The imaging data were collected
in drift-scan mode in five bandpasses (u, g, r, i, and z); our 95% completeness
limits for stars are 22.0, 22.2, 22.2, 21.3, and 20.5, respectively. The photometric
calibration is reproducible to 5%, 3%, 3%, 3%, and 5%, respectively. The spectra
are flux- and wavelength-calibrated, with 4096 pixels from 3800 to 9200 Å at R
≈ 1800. We present the means by which these data are distributed to the astronomical
community, descriptions of the hardware used to obtain the data, the software
used for processing the data, the measured quantities for each observed object,
and an overview of the properties of this data set.
article_processing_charge: No
article_type: original
author:
- first_name: Chris
full_name: Stoughton, Chris
last_name: Stoughton
- first_name: Robert H.
full_name: Lupton, Robert H.
last_name: Lupton
- first_name: Mariangela
full_name: Bernardi, Mariangela
last_name: Bernardi
- first_name: Michael R.
full_name: Blanton, Michael R.
last_name: Blanton
- first_name: Scott
full_name: Burles, Scott
last_name: Burles
- first_name: Francisco J.
full_name: Castander, Francisco J.
last_name: Castander
- first_name: A. J.
full_name: Connolly, A. J.
last_name: Connolly
- first_name: Daniel J.
full_name: Eisenstein, Daniel J.
last_name: Eisenstein
- first_name: Joshua A.
full_name: Frieman, Joshua A.
last_name: Frieman
- first_name: G. S.
full_name: Hennessy, G. S.
last_name: Hennessy
- first_name: Robert B.
full_name: Hindsley, Robert B.
last_name: Hindsley
- first_name: Željko
full_name: Ivezić, Željko
last_name: Ivezić
- first_name: Stephen
full_name: Kent, Stephen
last_name: Kent
- first_name: Peter Z.
full_name: Kunszt, Peter Z.
last_name: Kunszt
- first_name: Brian C.
full_name: Lee, Brian C.
last_name: Lee
- first_name: Avery
full_name: Meiksin, Avery
last_name: Meiksin
- first_name: Jeffrey A.
full_name: Munn, Jeffrey A.
last_name: Munn
- first_name: Heidi Jo
full_name: Newberg, Heidi Jo
last_name: Newberg
- first_name: R. C.
full_name: Nichol, R. C.
last_name: Nichol
- first_name: Tom
full_name: Nicinski, Tom
last_name: Nicinski
- first_name: Jeffrey R.
full_name: Pier, Jeffrey R.
last_name: Pier
- first_name: Gordon T.
full_name: Richards, Gordon T.
last_name: Richards
- first_name: Michael W.
full_name: Richmond, Michael W.
last_name: Richmond
- first_name: David J.
full_name: Schlegel, David J.
last_name: Schlegel
- first_name: J. Allyn
full_name: Smith, J. Allyn
last_name: Smith
- first_name: Michael A.
full_name: Strauss, Michael A.
last_name: Strauss
- first_name: Mark
full_name: SubbaRao, Mark
last_name: SubbaRao
- first_name: Alexander S.
full_name: Szalay, Alexander S.
last_name: Szalay
- first_name: Aniruddha R.
full_name: Thakar, Aniruddha R.
last_name: Thakar
- first_name: Douglas L.
full_name: Tucker, Douglas L.
last_name: Tucker
- first_name: Daniel E.
full_name: Vanden Berk, Daniel E.
last_name: Vanden Berk
- first_name: Brian
full_name: Yanny, Brian
last_name: Yanny
- first_name: Jennifer K.
full_name: Adelman, Jennifer K.
last_name: Adelman
- first_name: John E.
full_name: Anderson, Jr., John E.
last_name: Anderson, Jr.
- first_name: Scott F.
full_name: Anderson, Scott F.
last_name: Anderson
- first_name: James
full_name: Annis, James
last_name: Annis
- first_name: Neta A.
full_name: Bahcall, Neta A.
last_name: Bahcall
- first_name: J. A.
full_name: Bakken, J. A.
last_name: Bakken
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id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
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orcid: 0000-0003-3633-5403
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last_name: Sekiguchi
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full_name: Snedden, Stephanie A.
last_name: Snedden
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last_name: Stubbs
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full_name: Szokoly, Gyula P.
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full_name: Tabachnik, Serge
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full_name: Tsvetanov, Zlatan
last_name: Tsvetanov
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full_name: Uomoto, Alan
last_name: Uomoto
- first_name: Michael S.
full_name: Vogeley, Michael S.
last_name: Vogeley
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full_name: Voges, Wolfgang
last_name: Voges
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full_name: Waddell, Patrick
last_name: Waddell
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full_name: Walterbos, René
last_name: Walterbos
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full_name: Weinberg, David H.
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last_name: Wilhite
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full_name: Wolfe, David
last_name: Wolfe
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full_name: Yasuda, Naoki
last_name: Yasuda
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full_name: York, Donald G.
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citation:
ama: 'Stoughton C, Lupton RH, Bernardi M, et al. Sloan digital sky survey: Early
data release. The Astronomical Journal. 2002;123(1):485-548. doi:10.1086/324741'
apa: 'Stoughton, C., Lupton, R. H., Bernardi, M., Blanton, M. R., Burles, S., Castander,
F. J., … Zheng, W. (2002). Sloan digital sky survey: Early data release. The
Astronomical Journal. American Astronomical Society. https://doi.org/10.1086/324741'
chicago: 'Stoughton, Chris, Robert H. Lupton, Mariangela Bernardi, Michael R. Blanton,
Scott Burles, Francisco J. Castander, A. J. Connolly, et al. “Sloan Digital Sky
Survey: Early Data Release.” The Astronomical Journal. American Astronomical
Society, 2002. https://doi.org/10.1086/324741.'
ieee: 'C. Stoughton et al., “Sloan digital sky survey: Early data release,”
The Astronomical Journal, vol. 123, no. 1. American Astronomical Society,
pp. 485–548, 2002.'
ista: 'Stoughton C et al. 2002. Sloan digital sky survey: Early data release. The
Astronomical Journal. 123(1), 485–548.'
mla: 'Stoughton, Chris, et al. “Sloan Digital Sky Survey: Early Data Release.” The
Astronomical Journal, vol. 123, no. 1, American Astronomical Society, 2002,
pp. 485–548, doi:10.1086/324741.'
short: C. Stoughton, R.H. Lupton, M. Bernardi, M.R. Blanton, S. Burles, F.J. Castander,
A.J. Connolly, D.J. Eisenstein, J.A. Frieman, G.S. Hennessy, R.B. Hindsley, Ž.
Ivezić, S. Kent, P.Z. Kunszt, B.C. Lee, A. Meiksin, J.A. Munn, H.J. Newberg, R.C.
Nichol, T. Nicinski, J.R. Pier, G.T. Richards, M.W. Richmond, D.J. Schlegel, J.A.
Smith, M.A. Strauss, M. SubbaRao, A.S. Szalay, A.R. Thakar, D.L. Tucker, D.E.
Vanden Berk, B. Yanny, J.K. Adelman, J.E. Anderson, Jr., S.F. Anderson, J. Annis,
N.A. Bahcall, J.A. Bakken, M. Bartelmann, S. Bastian, A. Bauer, E. Berman, H.
Böhringer, W.N. Boroski, S. Bracker, C. Briegel, J.W. Briggs, J. Brinkmann, R.
Brunner, L. Carey, M.A. Carr, B. Chen, D. Christian, P.L. Colestock, J.H. Crocker,
I. Csabai, P.C. Czarapata, J. Dalcanton, A.F. Davidsen, J.E. Davis, W. Dehnen,
S. Dodelson, M. Doi, T. Dombeck, M. Donahue, N. Ellman, B.R. Elms, M.L. Evans,
L. Eyer, X. Fan, G.R. Federwitz, S. Friedman, M. Fukugita, R. Gal, B. Gillespie,
K. Glazebrook, J. Gray, E.K. Grebel, B. Greenawalt, G. Greene, J.E. Gunn, E. de
Haas, Z. Haiman, M. Haldeman, P.B. Hall, M. Hamabe, B. Hansen, F.H. Harris, H.
Harris, M. Harvanek, S.L. Hawley, J.J.E. Hayes, T.M. Heckman, A. Helmi, A. Henden,
C.J. Hogan, D.W. Hogg, D.J. Holmgren, J. Holtzman, C.-H. Huang, C. Hull, S.-I.
Ichikawa, T. Ichikawa, D.E. Johnston, G. Kauffmann, R.S.J. Kim, T. Kimball, E.
Kinney, M. Klaene, S.J. Kleinman, A. Klypin, G.R. Knapp, J. Korienek, J. Krolik,
R.G. Kron, J. Krzesiński, D.Q. Lamb, R.F. Leger, S. Limmongkol, C. Lindenmeyer,
D.C. Long, C. Loomis, J. Loveday, B. MacKinnon, E.J. Mannery, P.M. Mantsch, B.
Margon, P. McGehee, T.A. McKay, B. McLean, K. Menou, A. Merelli, H.J. Mo, D.G.
Monet, O. Nakamura, V.K. Narayanan, T. Nash, E.H. Neilsen, Jr., P.R. Newman, A.
Nitta, M. Odenkirchen, N. Okada, S. Okamura, J.P. Ostriker, R. Owen, A.G. Pauls,
J. Peoples, R.S. Peterson, D. Petravick, A. Pope, R. Pordes, M. Postman, A. Prosapio,
T.R. Quinn, R. Rechenmacher, C.H. Rivetta, H.-W. Rix, C.M. Rockosi, R. Rosner,
K. Ruthmansdorfer, D. Sandford, D.P. Schneider, R. Scranton, M. Sekiguchi, G.
Sergey, R. Sheth, K. Shimasaku, S. Smee, S.A. Snedden, A. Stebbins, C. Stubbs,
I. Szapudi, P. Szkody, G.P. Szokoly, S. Tabachnik, Z. Tsvetanov, A. Uomoto, M.S.
Vogeley, W. Voges, P. Waddell, R. Walterbos, S. Wang, M. Watanabe, D.H. Weinberg,
R.L. White, S.D.M. White, B. Wilhite, D. Wolfe, N. Yasuda, D.G. York, I. Zehavi,
W. Zheng, The Astronomical Journal 123 (2002) 485–548.
date_created: 2024-09-06T10:32:06Z
date_published: 2002-01-01T00:00:00Z
date_updated: 2024-11-12T09:51:31Z
day: '01'
doi: 10.1086/324741
extern: '1'
intvolume: ' 123'
issue: '1'
language:
- iso: eng
month: '01'
oa_version: None
page: 485-548
publication: The Astronomical Journal
publication_identifier:
eissn:
- 1538-3881
issn:
- 0004-6256
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1086/340314
scopus_import: '1'
status: public
title: 'Sloan digital sky survey: Early data release'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 123
year: '2002'
...
---
OA_place: repository
OA_type: free access
_id: '17802'
abstract:
- lang: eng
text: The Sloan Digital Sky Survey has confirmed the existence of populations of
broad absorption line (BAL) quasars with various unusual properties. We present
and discuss 23 such objects and consider the implications of their wide range
of properties for models of BAL outflows and quasars in general. We have discovered
one BAL quasar with a record number of absorption lines. Two other similarly complex
objects with many narrow troughs show broad Mg II absorption extending longward
of their systemic host galaxy redshifts. This can be explained as absorption of
an extended continuum source by the rotation-dominated base of a disk wind. Five
other objects have absorption that removes an unprecedented ∼90% of all flux shortward
of Mg II. The absorption in one of them has varied across the ultraviolet with
an amplitude and rate of change as great as ever seen. This same object may also
show broad Hβ absorption. Numerous reddened BAL quasars have been found, including
at least one reddened mini-BAL quasar with very strong Fe II emission. The five
reddest objects have continuum reddenings of E(B-V) ≃ 0.5, and in two of them
we find strong evidence that the reddening curve is even steeper than that of
the SMC. We have found at least one object with absorption from Fe III but not
Fe II. This may be due to a high column density of moderately high ionization
gas, but the Fe III level populations must also be affected by some sort of resonance.
Finally, we have found two luminous, probably reddened high-redshift objects that
may be BAL quasars whose troughs partially cover different regions of the continuum
source as a function of velocity.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Patrick B.
full_name: Hall, Patrick B.
last_name: Hall
- first_name: Scott F.
full_name: Anderson, Scott F.
last_name: Anderson
- first_name: Michael A.
full_name: Strauss, Michael A.
last_name: Strauss
- first_name: Donald G.
full_name: York, Donald G.
last_name: York
- first_name: Gordon T.
full_name: Richards, Gordon T.
last_name: Richards
- first_name: Xiaohui
full_name: Fan, Xiaohui
last_name: Fan
- first_name: G. R.
full_name: Knapp, G. R.
last_name: Knapp
- first_name: Donald P.
full_name: Schneider, Donald P.
last_name: Schneider
- first_name: Daniel E.
full_name: Vanden Berk, Daniel E.
last_name: Vanden Berk
- first_name: T. R.
full_name: Geballe, T. R.
last_name: Geballe
- first_name: Amanda E.
full_name: Bauer, Amanda E.
last_name: Bauer
- first_name: Robert H.
full_name: Becker, Robert H.
last_name: Becker
- first_name: Marc
full_name: Davis, Marc
last_name: Davis
- first_name: Hans‐Walter
full_name: Rix, Hans‐Walter
last_name: Rix
- first_name: R. C.
full_name: Nichol, R. C.
last_name: Nichol
- first_name: Neta A.
full_name: Bahcall, Neta A.
last_name: Bahcall
- first_name: J.
full_name: Brinkmann, J.
last_name: Brinkmann
- first_name: Robert
full_name: Brunner, Robert
last_name: Brunner
- first_name: A. J.
full_name: Connolly, A. J.
last_name: Connolly
- first_name: Istvan
full_name: Csabai, Istvan
last_name: Csabai
- first_name: Mamoru
full_name: Doi, Mamoru
last_name: Doi
- first_name: Masataka
full_name: Fukugita, Masataka
last_name: Fukugita
- first_name: James E.
full_name: Gunn, James E.
last_name: Gunn
- first_name: Zoltán
full_name: Haiman, Zoltán
id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
last_name: Haiman
orcid: 0000-0003-3633-5403
- first_name: Michael
full_name: Harvanek, Michael
last_name: Harvanek
- first_name: Timothy M.
full_name: Heckman, Timothy M.
last_name: Heckman
- first_name: G. S.
full_name: Hennessy, G. S.
last_name: Hennessy
- first_name: Naohisa
full_name: Inada, Naohisa
last_name: Inada
- first_name: Željko
full_name: Ivezić, Željko
last_name: Ivezić
- first_name: David
full_name: Johnston, David
last_name: Johnston
- first_name: S.
full_name: Kleinman, S.
last_name: Kleinman
- first_name: Julian H.
full_name: Krolik, Julian H.
last_name: Krolik
- first_name: Jurek
full_name: Krzesinski, Jurek
last_name: Krzesinski
- first_name: Peter Z.
full_name: Kunszt, Peter Z.
last_name: Kunszt
- first_name: D. Q.
full_name: Lamb, D. Q.
last_name: Lamb
- first_name: Daniel C.
full_name: Long, Daniel C.
last_name: Long
- first_name: Robert H.
full_name: Lupton, Robert H.
last_name: Lupton
- first_name: Gajus
full_name: Miknaitis, Gajus
last_name: Miknaitis
- first_name: Jeffrey A.
full_name: Munn, Jeffrey A.
last_name: Munn
- first_name: Vijay K.
full_name: Narayanan, Vijay K.
last_name: Narayanan
- first_name: Eric
full_name: Neilsen, Eric
last_name: Neilsen
- first_name: P. R.
full_name: Newman, P. R.
last_name: Newman
- first_name: Atsuko
full_name: Nitta, Atsuko
last_name: Nitta
- first_name: Sadanori
full_name: Okamura, Sadanori
last_name: Okamura
- first_name: Laura
full_name: Pentericci, Laura
last_name: Pentericci
- first_name: Jeffrey R.
full_name: Pier, Jeffrey R.
last_name: Pier
- first_name: David J.
full_name: Schlegel, David J.
last_name: Schlegel
- first_name: S.
full_name: Snedden, S.
last_name: Snedden
- first_name: Alexander S.
full_name: Szalay, Alexander S.
last_name: Szalay
- first_name: Anirudda R.
full_name: Thakar, Anirudda R.
last_name: Thakar
- first_name: Zlatan
full_name: Tsvetanov, Zlatan
last_name: Tsvetanov
- first_name: Richard L.
full_name: White, Richard L.
last_name: White
- first_name: Wei
full_name: Zheng, Wei
last_name: Zheng
citation:
ama: Hall PB, Anderson SF, Strauss MA, et al. Unusual broad absorption line quasars
from the sloan digital sky survey. The Astrophysical Journal Supplement Series.
2002;141(2):267-309. doi:10.1086/340546
apa: Hall, P. B., Anderson, S. F., Strauss, M. A., York, D. G., Richards, G. T.,
Fan, X., … Zheng, W. (2002). Unusual broad absorption line quasars from the sloan
digital sky survey. The Astrophysical Journal Supplement Series. American
Astronomical Society. https://doi.org/10.1086/340546
chicago: Hall, Patrick B., Scott F. Anderson, Michael A. Strauss, Donald G. York,
Gordon T. Richards, Xiaohui Fan, G. R. Knapp, et al. “Unusual Broad Absorption
Line Quasars from the Sloan Digital Sky Survey.” The Astrophysical Journal
Supplement Series. American Astronomical Society, 2002. https://doi.org/10.1086/340546.
ieee: P. B. Hall et al., “Unusual broad absorption line quasars from the
sloan digital sky survey,” The Astrophysical Journal Supplement Series,
vol. 141, no. 2. American Astronomical Society, pp. 267–309, 2002.
ista: Hall PB, Anderson SF, Strauss MA, York DG, Richards GT, Fan X, Knapp GR, Schneider
DP, Vanden Berk DE, Geballe TR, Bauer AE, Becker RH, Davis M, Rix H, Nichol RC,
Bahcall NA, Brinkmann J, Brunner R, Connolly AJ, Csabai I, Doi M, Fukugita M,
Gunn JE, Haiman Z, Harvanek M, Heckman TM, Hennessy GS, Inada N, Ivezić Ž, Johnston
D, Kleinman S, Krolik JH, Krzesinski J, Kunszt PZ, Lamb DQ, Long DC, Lupton RH,
Miknaitis G, Munn JA, Narayanan VK, Neilsen E, Newman PR, Nitta A, Okamura S,
Pentericci L, Pier JR, Schlegel DJ, Snedden S, Szalay AS, Thakar AR, Tsvetanov
Z, White RL, Zheng W. 2002. Unusual broad absorption line quasars from the sloan
digital sky survey. The Astrophysical Journal Supplement Series. 141(2), 267–309.
mla: Hall, Patrick B., et al. “Unusual Broad Absorption Line Quasars from the Sloan
Digital Sky Survey.” The Astrophysical Journal Supplement Series, vol.
141, no. 2, American Astronomical Society, 2002, pp. 267–309, doi:10.1086/340546.
short: P.B. Hall, S.F. Anderson, M.A. Strauss, D.G. York, G.T. Richards, X. Fan,
G.R. Knapp, D.P. Schneider, D.E. Vanden Berk, T.R. Geballe, A.E. Bauer, R.H. Becker,
M. Davis, H. Rix, R.C. Nichol, N.A. Bahcall, J. Brinkmann, R. Brunner, A.J. Connolly,
I. Csabai, M. Doi, M. Fukugita, J.E. Gunn, Z. Haiman, M. Harvanek, T.M. Heckman,
G.S. Hennessy, N. Inada, Ž. Ivezić, D. Johnston, S. Kleinman, J.H. Krolik, J.
Krzesinski, P.Z. Kunszt, D.Q. Lamb, D.C. Long, R.H. Lupton, G. Miknaitis, J.A.
Munn, V.K. Narayanan, E. Neilsen, P.R. Newman, A. Nitta, S. Okamura, L. Pentericci,
J.R. Pier, D.J. Schlegel, S. Snedden, A.S. Szalay, A.R. Thakar, Z. Tsvetanov,
R.L. White, W. Zheng, The Astrophysical Journal Supplement Series 141 (2002) 267–309.
date_created: 2024-09-06T11:30:40Z
date_published: 2002-08-01T00:00:00Z
date_updated: 2024-11-12T10:02:25Z
day: '01'
doi: 10.1086/340546
extern: '1'
external_id:
arxiv:
- astro-ph/0203252
intvolume: ' 141'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.astro-ph/0203252
month: '08'
oa: 1
oa_version: Preprint
page: 267-309
publication: The Astrophysical Journal Supplement Series
publication_identifier:
eissn:
- 1538-4365
issn:
- 0067-0049
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Unusual broad absorption line quasars from the sloan digital sky survey
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 141
year: '2002'
...