Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico...

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OS EXPERIMENTOS protoMIRAX e MIRAX Manuel Antonio Castro Avila Jo˜ ao Braga, Fl´ avio D’Amico Workshop da Divis˜ ao de Astrof´ ısica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX e MIRAX 3 - 4 de maio de 2016 1 / 12

Transcript of Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico...

Page 1: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

OS EXPERIMENTOS protoMIRAX e MIRAX

Manuel Antonio Castro Avila

Joao Braga, Flavio D’Amico

Workshop da Divisao de Astrofısica

3 - 4 de maio de 2016

Manuel Castro protoMIRAX e MIRAX 3 - 4 de maio de 2016 1 / 12

Page 2: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

O protoMIRAX/MIRAX

PbSn

Cu

Mask

Collimator

Shielding

Detection plane

Rear shielding

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Page 3: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Componentes do ruıdo

Energy (MeV)1−10 1 10

-1 M

eV-1

sr

-1 s

-2P

hoto

ns c

m

3−10

2−10

1−10

1

10 °0 - 65°65 - 95

°95 - 130°130 - 180

-ray photonsγAtmospheric

Energy (MeV)1 10

-1 M

eV-1

sr

-1 s

-2P

artic

les

cm 3−10

2−10 Electrons

Energy (MeV)1 10 210

-1 M

eV-1

sr

-1 s

-2P

artic

les

cm

2−10

1−10

Neutrons

Energy (MeV)10 210 310 410 510

-1 M

eV-1

sr

-1 s

-2P

artic

les

cm

8−10

7−10

6−10

5−10

4−10 Primary protons

Secondary protons

Protons

Manuel Castro protoMIRAX e MIRAX 3 - 4 de maio de 2016 3 / 12

Page 4: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Energy (keV)10 210 310 410 510

-1 k

eV-1

sr

-1 s

-2P

hoto

ns c

m

10−10

9−10

8−10

7−10

6−10

5−10

4−10

3−10

2−10

1−10 -ray backgroundγCosmic diffuse

Energy (keV)10 210 310 410 510

-1 k

eV-1

sr

-1 s

-2P

hoto

ns c

m

7−10

6−10

5−10

4−10

3−10

2−10Albedo photons

Energy (keV)610 710

-1 k

eV-1

sr

-1 s

-2P

artic

les

cm

11−10

10−10

9−10

8−10 Galactic cosmic rays

Energy (keV)610

-1 k

eV-1

sr

-1 s

-2P

artic

les

cm

11−10

10−10

9−10

8−10 Trapped protons

Energy (keV)10 210 310 410 510 610

-1 k

eV-1

sr

-1 s

-2P

artic

les

cm

10−10

9−10

8−10

7−10

6−10

5−10

Neutrons

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Page 5: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Normalizacao

N =

∫IN cos θ dΩ dA dt dE ,

N = π AT

∫IN dE ,

dΩ = dφ sin θdθdA = R2 sinαdαdΦ

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Page 6: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Contribuicao do ruıdo

Energy (keV)210

)-5

10× (

-1 k

eV-1

s-2

Cou

nts

cm

30

40

50

607080

100

200

300

Total background

Gamma

Protons

Neutrons

protoMIRAX Background

Energy (keV)40 50 60 70 80 90 100 200

-1 k

eV-1

s-2

Cou

nts

cm

0.30.4

1

2

Electrons

)-5

10

×(-1

keV

-1 s

-2C

ount

s cm

Energy (keV)20 30 40 50 60 70 100 200

)-5

10

× (

-1 k

eV-1

s-2

Cou

nts

cm

0.81

2

34

10

20

30

100

200

300Total background

-ray radiationγCosmic diffuse

Albedo photons

Galactic Cosmic Rays

NeutronsTrapped protons

MIRAX Background

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Page 7: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Distribuicao espacial

-1Co

unts

sDetector number

1 2 3 4 5 6 7 8 9 10111213Detector number 12345678910111213

-310×

0

5

10

15

20

25

30

° - 65°-ray background: 0γ

Detector number1 2 3 4 5 6 7 8 9 10 1112 13

Detector number 12345678910111213

-310×

02468

10121416

° - 95°-ray background: 65γ

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number 12345678910111213

-310×

05

101520253035

° - 130°-ray background: 95γ

Detector number1 2 3 4 5 6 7 8 9 10 1112 13

Detector number 12345678910111213

-310×

02468

10121416

° - 180°-ray background: 130γ

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number 12345678910111213

-310×

05

1015202530354045

Primary Protons

Detector number1 2 3 4 5 6 7 8 9 10 1112 13

Detector number 12345678910111213

-310×

05

101520253035

Secondary Protons

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number 12345678910111213

-310×

00.20.40.60.8

11.21.41.61.8

22.22.4

Electrons

Detector number1 2 3 4 5 6 7 8 9 10 1112 13

Detector number 12345678910111213

-210×

0123456789

Neutrons

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Page 8: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

-1C

ount

s s

Detector number1 2 3 4 5 6 7 8 910111213

Detector number12345678910111213

-210×

0

2

4

6

8

10

-ray radiationγCosmic diffuse

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number12345678910111213

-210×

0

2

4

6

8

10

12

Albedo photons

Detector number1 2 3 4 5 6 7 8 910111213

Detector number12345678910111213

-310×

02468

101214

Galactic Cosmic Rays

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number12345678910111213

-310×

0

1

2

3

4

5

Neutrons

Detector number1 2 3 4 5 6 7 8 910111213

Detector number12345678910111213

-410×

05

101520253035

Trapped protons

Detector number1 2 3 4 5 6 7 8 9 10111213

Detector number12345678910111213

-210×

0

5

10

15

20

25

Total background

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Page 9: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Reconstrucao de imagens

Energy (keV)10 100

-1 k

eV-1

s-2

Pho

tons

cm

6−10

5−10

4−10

3−10

2−10

1−10Crab nebula

1E 1740.7-2942

GRS 1758-258

para o protoMIRAX

F (E) = F0(E) e−µ

ρ(E) x sec(z)

cos z(t) = sinϕ sin δ + cosϕ cos δ cos(t − α)

N =

∫S

∫ Emax

Emin

∫ T

0F0(E) e

−µρ

(E) x sec(z(t))dt dE dS

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Page 10: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Imagem reconstruıda

Angular coordinates (-10.05-6.70 -3.35 0 3.35 6.70 10.05

Angular coordinates (-10.05-6.70

-3.350

3.356.70

10.05

σ

050

100150200250300350400450

σ0

50

100

150

200

250

300

350

400

)°Angular coordinates (

-10.05 -6.70 -3.35 0 3.35 6.70 10.05

Angular coordinates ( -10.05-6.70

-3.350

3.356.70

10.05

σ

0

20

40

60

80

σ

0

10

20

30

40

50

60

70

80

Crab - MIRAX - 4h Crab - protoMIRAX - 4h

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Page 11: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

Angular coordinates (-10.05-6.70 -3.35 0 3.35 6.70 10.05

Angular coordinates (-10.05-6.70

-3.350

3.356.70

10.05

σ

0

5

10

15

20

σ

2−

0

2

4

6

8

10

12

14

16

18

Figura: 1E 1740.7−2942 e GRS 1758−258

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Page 12: Manuel Antonio Castro Avila - INPE · Manuel Antonio Castro Avila Jo~ao Braga, Fl avio D’Amico Workshop da Divis~ao de Astrof sica 3 - 4 de maio de 2016 Manuel Castro protoMIRAX

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