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Seljak is developing machine learning methods with applications to cosmology, astronomy, and other sciences. Notable examples include
Fourier-based Gaussian processes for analysis of time and/or spatially ordered data, generative models with explicit physics symmetries (translation, rotation), and
801:
Seljak, Uroš; Makarov, Alexey; McDonald, Patrick; Anderson, Scott F.; Bahcall, Neta A.; Brinkmann, J.; Burles, Scott; Cen, Renyue; Doi, Mamoru; Gunn, James E.; Ivezić, Željko (20 May 2005). "Cosmological parameter analysis including SDSS Ly α forest and galaxy bias: Constraints on the primordial
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Much of Seljak's recent work has been focused on how to extract fundamental properties of our universe from cosmological observations using analytical methods and numerical simulations. He has developed cosmological generative models of dark matter, stars and cosmic gas distributions.
359:
Seljak is actively developing methods for accelerated approximate
Bayesian methodologies, and applying them to cosmology, astronomy, and other sciences. Examples of this work are the MicroCanonical Hamiltonian and Langevin Monte Carlo and Deterministic Langevin Monte Carlo samplers.
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Seljak, Uroš; Zaldarriaga, Matias (1996). "A Line-of-Sight
Integration Approach to Cosmic Microwave Background Anisotropies".
732:
Seljak, Uroš; Makarov, Alexey; McDonald, Patrick; Trac, Hy (8 November 2006). "Can
Sterile Neutrinos Be the Dark Matter?".
1021:
980:
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326:, galaxy clustering and weak gravitational lensing, and the implications of these observations for the large scale
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in CMB polarization that are a tracer of primordial gravitational waves from inflation. Together with
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code for CMB Temperature, E and B-mode polarization, and for gravitational lensing effects on CMB.
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Seljak, Uroš (10 June 1997). "Measuring
Polarization in the Cosmic Microwave Background".
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629:"Galaxy Study Validates General Relativity on Cosmic Scale, Existence of Dark Matter"
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physics and astronomy departments in 2008. He holds a joint appointment with the
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239:. He is particularly well-known for his research in cosmology and approximate
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from the same institution in 1991. Seljak conducted his doctoral research at
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Seljak is a cosmologist who is particularly well-known for his research on
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235:) is a Slovenian cosmologist and a professor of astronomy and physics at
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sliced iterative transport methods for density estimation and sampling.
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967:"Commons:Wiki Science Competition 2019/Winners - Wikimedia Commons"
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Light propagation in a weakly perturbed expanding universe
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spectrum of fluctuations, neutrino mass, and dark energy".
542:, UC Berkeley physics department, retrieved 27 March 2011.
477:
Light propagation in a weakly perturbed expanding universe
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Members of the United States
National Academy of Sciences
865:"Analytic model for galaxy and dark matter clustering"
284:
210:
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100:
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69:
51:
32:
869:Monthly Notices of the Royal Astronomical Society
259:and carried out his undergraduate studies at the
981:"Lab Cosmologist Wins Science Photo Competition"
107:Professor in Physics and Astronomy Departments,
8:
1037:Massachusetts Institute of Technology alumni
292:International Centre for Theoretical Physics
267:. He graduated in 1989 and later received a
436:Honorary Doctorate, University of Ljubljana
333:In 1997, Seljak predicted the existence of
1052:Academic staff of the University of Zurich
1047:University of California, Berkeley faculty
178:Theoretical and observational astrophysics
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568:
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389:David and Lucille Packard Research Fellow
348:In 2000, he developed the halo model for
181:Statistical data analysis in astrophysics
1072:Fellows of the American Physical Society
420:Highest cited Slovenian scientist (2019)
466:
651:"Raumzeit-Wellen provozieren Forscher"
443:American Academy of Arts and Sciences
324:cosmic microwave background radiation
312:Lawrence Berkeley National Laboratory
273:Massachusetts Institute of Technology
7:
550:
548:
401:Helen B. Warner Prize for Astronomy
144:Helen B. Warner Prize for Astronomy
352:and galaxy clustering statistics.
282:After postdoctoral studies at the
237:University of California, Berkeley
25:
900:10.1046/j.1365-8711.2000.03715.x
863:Seljak, Uroš (11 October 2000).
649:Becker, Markus (20 April 2005),
426:international winner (2019-2020)
184:Bayesian statistical methodology
956:, AAS, retrieved 27 March 2011.
608:Sincell, Mark (30 March 1999).
286:, he held faculty positions at
1032:University of Ljubljana alumni
1:
923:"2021 Gruber Cosmology Prize"
764:10.1103/PhysRevLett.97.191303
1042:Princeton University faculty
415:National Academy of Sciences
372:Seljak was awarded the 2021
610:"A New Lens on Dark Matter"
1088:
834:10.1103/PhysRevD.71.103515
257:Nova Gorica Grammar School
113:Senior Faculty Scientist,
673:The Astrophysical Journal
557:The Astrophysical Journal
430:Gruber Prize in Cosmology
408:American Physical Society
374:Gruber Prize in Cosmology
328:structure of the universe
222:
159:
150:Gruber Prize in Cosmology
91:, Slovenia (1989, 1991) *
39:
952:19 November 2010 at the
424:Wiki Science Competition
1057:People from Nova Gorica
947:Warner prize recipients
734:Physical Review Letters
261:University of Ljubljana
89:University of Ljubljana
1067:Sloan Research Fellows
474:Seljak, Uros̆ (1995).
614:Physical Review Focus
511:"Overview of CMBFAST"
395:Sloan Research Fellow
306:, before joining the
251:Seljak completed his
243:statistical methods.
231:(born 13 May 1966 in
27:Slovenian cosmologist
1022:Slovenian physicists
304:University of Zurich
288:Princeton University
891:2000MNRAS.318..203S
826:2005PhRvD..71j3515S
756:2006PhRvL..97s1303S
695:1997ApJ...482....6S
579:1996ApJ...469..437S
341:, he developed the
253:secondary education
217:Edmund Bertschinger
46:Uroš Seljak in 2011
382:Matias Zaldarriaga
368:Honours and awards
339:Matias Zaldarriaga
804:Physical Review D
413:Member of the US
378:Marc Kamionkowski
275:and received his
226:
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161:Scientific career
16:(Redirected from
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747:astro-ph/0602430
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450:Notable students
212:Doctoral advisor
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187:Machine learning
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987:. July 31, 2020
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954:Wayback Machine
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540:Faculty profile
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269:Master's degree
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128:E and B-modes,
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84:Alma mater
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875:(1): 203–213.
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703:10.1086/304123
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616:. Vol. 3.
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989:. Retrieved
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1012:1966 births
679:(1): 6–16.
659:(in German)
563:: 437–444.
350:dark matter
308:UC Berkeley
233:Nova Gorica
229:Uroš Seljak
109:UC Berkeley
101:Occupations
70:Citizenship
62:13 May 1966
34:Uroš Seljak
18:Uros Seljak
1006:Categories
991:August 15,
480:(Thesis).
462:References
441:Member of
302:, and the
58:1966-05-13
909:0035-8711
842:1550-7998
772:0031-9007
711:0004-637X
279:in 1995.
247:Biography
174:Cosmology
74:Slovenian
950:Archived
850:15237151
788:22565444
780:17155611
719:16825580
265:Slovenia
241:Bayesian
117:Berkeley
887:Bibcode
822:Bibcode
752:Bibcode
691:Bibcode
656:Spiegel
595:3015599
575:Bibcode
343:CMBFAST
335:B-modes
296:Trieste
255:at the
130:CMBFAST
95:(1995)
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445:(2024)
438:(2023)
432:(2021)
417:(2019)
410:(2013)
403:(2001)
397:(2001)
391:(2000)
318:Career
290:, the
205:(1995)
203:
196:Thesis
167:Fields
152:(2021)
146:(2001)
137:Awards
932:6 May
877:arXiv
846:S2CID
812:arXiv
784:S2CID
742:arXiv
715:S2CID
681:arXiv
591:S2CID
565:arXiv
300:Italy
132:code
993:2023
934:2021
905:ISSN
838:ISSN
776:PMID
768:ISSN
707:ISSN
522:2023
515:NASA
497:2023
380:and
115:LBNL
52:Born
895:doi
873:318
830:doi
760:doi
699:doi
677:482
583:doi
561:469
486:hdl
482:MIT
294:in
277:PhD
93:MIT
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