Language:
English
日文
簡体中文
繁體中文
Help
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
Optimized dark matter searches in de...
~
Aleksic, Jelena.
Optimized dark matter searches in deep observations of Segue 1 with MAGIC[electronic resource] /
Record Type:
Language materials, printed : Monograph/item
[NT 15000414]:
523.1126
Title/Author:
Optimized dark matter searches in deep observations of Segue 1 with MAGIC/ by Jelena Aleksic.
Author:
Aleksic, Jelena.
Published:
Cham : : Springer International Publishing :, 2016.
Description:
xxxvii, 184 p. : : ill. (some col.), digital ;; 24 cm.
Contained By:
Springer eBooks
Subject:
Dark matter (Astronomy)
Subject:
Physics.
Subject:
Astrophysics and Astroparticles.
Subject:
Astronomy, Observations and Techniques.
Subject:
Elementary Particles, Quantum Field Theory.
ISBN:
9783319231235
ISBN:
9783319231228
[NT 15000228]:
Introduction -- Dark matter searches -- The MAGIC Telescopes -- Full Likelihood Method -- Dark Matter Searches in Dwarf Spheroidal Galaxy Segue 1 with MAGIC -- Future Prospects -- Conclusions.
[NT 15000229]:
This thesis presents the results of indirect dark matter searches in the gamma-ray sky of the near Universe, as seen by the MAGIC Telescopes. The author has proposed and led the 160 hours long observations of the dwarf spheroidal galaxy Segue 1, which is the deepest survey of any such object by any Cherenkov telescope so far. Furthermore, she developed and completely characterized a new method, dubbed "Full Likelihood", that optimizes the sensitivity of Cherenkov instruments for detection of gamma-ray signals of dark matter origin. Compared to the standard analysis techniques, this novel approach introduces a sensitivity improvement of a factor of two (i.e. it requires 4 times less observation time to achieve the same result) In addition, it allows a straightforward merger of results from different targets and/or detectors. By selecting the optimal observational target and combining its very deep exposure with the Full Likelihood analysis of the acquired data, the author has improved the existing MAGIC bounds to the dark matter properties by more than one order of magnitude. Furthermore, for particles more massive than a few hundred GeV, those are the strongest constraints from dwarf galaxies achieved by any gamma-ray instrument, both ground-based or space-borne alike.
Online resource:
http://dx.doi.org/10.1007/978-3-319-23123-5
Optimized dark matter searches in deep observations of Segue 1 with MAGIC[electronic resource] /
Aleksic, Jelena.
Optimized dark matter searches in deep observations of Segue 1 with MAGIC
[electronic resource] /by Jelena Aleksic. - Cham :Springer International Publishing :2016. - xxxvii, 184 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- Dark matter searches -- The MAGIC Telescopes -- Full Likelihood Method -- Dark Matter Searches in Dwarf Spheroidal Galaxy Segue 1 with MAGIC -- Future Prospects -- Conclusions.
This thesis presents the results of indirect dark matter searches in the gamma-ray sky of the near Universe, as seen by the MAGIC Telescopes. The author has proposed and led the 160 hours long observations of the dwarf spheroidal galaxy Segue 1, which is the deepest survey of any such object by any Cherenkov telescope so far. Furthermore, she developed and completely characterized a new method, dubbed "Full Likelihood", that optimizes the sensitivity of Cherenkov instruments for detection of gamma-ray signals of dark matter origin. Compared to the standard analysis techniques, this novel approach introduces a sensitivity improvement of a factor of two (i.e. it requires 4 times less observation time to achieve the same result) In addition, it allows a straightforward merger of results from different targets and/or detectors. By selecting the optimal observational target and combining its very deep exposure with the Full Likelihood analysis of the acquired data, the author has improved the existing MAGIC bounds to the dark matter properties by more than one order of magnitude. Furthermore, for particles more massive than a few hundred GeV, those are the strongest constraints from dwarf galaxies achieved by any gamma-ray instrument, both ground-based or space-borne alike.
ISBN: 9783319231235
Standard No.: 10.1007/978-3-319-23123-5doiSubjects--Topical Terms:
556609
Dark matter (Astronomy)
LC Class. No.: QB791.3
Dewey Class. No.: 523.1126
Optimized dark matter searches in deep observations of Segue 1 with MAGIC[electronic resource] /
LDR
:02492nam a2200325 a 4500
001
455309
003
DE-He213
005
20160801143341.0
006
m d
007
cr nn 008maaau
008
161227s2016 gw s 0 eng d
020
$a
9783319231235
$q
(electronic bk.)
020
$a
9783319231228
$q
(paper)
024
7
$a
10.1007/978-3-319-23123-5
$2
doi
035
$a
978-3-319-23123-5
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB791.3
072
7
$a
PHVB
$2
bicssc
072
7
$a
SCI005000
$2
bisacsh
082
0 4
$a
523.1126
$2
23
090
$a
QB791.3
$b
.A366 2016
100
1
$a
Aleksic, Jelena.
$3
653561
245
1 0
$a
Optimized dark matter searches in deep observations of Segue 1 with MAGIC
$h
[electronic resource] /
$c
by Jelena Aleksic.
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2016.
300
$a
xxxvii, 184 p. :
$b
ill. (some col.), digital ;
$c
24 cm.
490
1
$a
Springer theses,
$x
2190-5053
505
0
$a
Introduction -- Dark matter searches -- The MAGIC Telescopes -- Full Likelihood Method -- Dark Matter Searches in Dwarf Spheroidal Galaxy Segue 1 with MAGIC -- Future Prospects -- Conclusions.
520
$a
This thesis presents the results of indirect dark matter searches in the gamma-ray sky of the near Universe, as seen by the MAGIC Telescopes. The author has proposed and led the 160 hours long observations of the dwarf spheroidal galaxy Segue 1, which is the deepest survey of any such object by any Cherenkov telescope so far. Furthermore, she developed and completely characterized a new method, dubbed "Full Likelihood", that optimizes the sensitivity of Cherenkov instruments for detection of gamma-ray signals of dark matter origin. Compared to the standard analysis techniques, this novel approach introduces a sensitivity improvement of a factor of two (i.e. it requires 4 times less observation time to achieve the same result) In addition, it allows a straightforward merger of results from different targets and/or detectors. By selecting the optimal observational target and combining its very deep exposure with the Full Likelihood analysis of the acquired data, the author has improved the existing MAGIC bounds to the dark matter properties by more than one order of magnitude. Furthermore, for particles more massive than a few hundred GeV, those are the strongest constraints from dwarf galaxies achieved by any gamma-ray instrument, both ground-based or space-borne alike.
650
0
$a
Dark matter (Astronomy)
$3
556609
650
1 4
$a
Physics.
$3
171863
650
2 4
$a
Astrophysics and Astroparticles.
$3
465672
650
2 4
$a
Astronomy, Observations and Techniques.
$3
464241
650
2 4
$a
Elementary Particles, Quantum Field Theory.
$3
464245
710
2
$a
SpringerLink (Online service)
$3
463450
773
0
$t
Springer eBooks
830
0
$a
Springer theses.
$3
463746
856
4 0
$u
http://dx.doi.org/10.1007/978-3-319-23123-5
950
$a
Physics and Astronomy (Springer-11651)
based on 0 review(s)
Multimedia
Multimedia file
http://dx.doi.org/10.1007/978-3-319-23123-5
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login