jim hinton 2006 high energy stereoscopic system (h.e.s.s.) array of four 107 m 2 telescopes in...

15
Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.) Array of four 107 m 2 telescopes in Namibia, 120 m spacing 5° FOV Threshold 100 GeV Angular Resolution 0.1° Completed 2004 European/African Collaboration

Post on 30-Jan-2016

217 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

High Energy Stereoscopic System (H.E.S.S.) Array of four 107 m2

telescopes in Namibia, 120 m spacing

5° FOV Threshold 100 GeV Angular Resolution 0.1° Completed 2004 European/African

Collaboration

Page 2: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

H.E.S.S. Results

In the first two years of operation: First astronomical gamma-ray image (RX J1713.7)

• Nature 432, 75 (2004) New source class (X-ray binaries)

• Science 309, 745 (2005) First sensitive survey of the galactic plane

• Science 307, 1938 (2005) 16 publications in ApJ and A&A

Page 3: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

The Inner Galaxy

15 new -ray sources - at least 3 source classes

A snapshot of energetic particles in our galaxy

+30° 0°

-30°

Pulsar Wind Nebulae, X-ray binary, Supernova remnants, Unknown

Page 4: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

The Inner Galaxy

15 new -ray sources - at least 3 source classes

A snapshot of energetic particles in our galaxy

+30° 0°

-30°

Pulsar Wind Nebulae, X-ray binary, Supernova remnants, Unknown

Page 5: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

The Inner Galaxy

15 new -ray sources - at least 3 source classes

A snapshot of energetic particles in our galaxy

+30° 0°

Pulsar Wind Nebulae, X-ray binary, Supernova remnants, Unknown

Page 6: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

The Inner Galaxy

15 new -ray sources - at least 3 source classes

A snapshot of energetic particles in our galaxy

+30° 0°

-30°

Pulsar Wind Nebulae, X-ray binary, Supernova remnants, Unknown

Page 7: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

The Inner Galaxy

15 new -ray sources - at least 3 source classes

A snapshot of energetic particles in our galaxy

+30° 0°

-30°

Pulsar Wind Nebulae, X-ray binary, Supernova remnants, Unknown

Page 8: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

Unambiguous evidence for particle acceleration in an SNR shell

Resolved shell in VHE -rays

Close correlation between X-rays and -rays - could the VHE emission be IC?

• Hard to explain spectral shape and implied B-field is low...

X-rays: ASCA 1-3 keV (contours)

-rays: HESS (colour scale)

The SNR RX J1713.7-3946

Page 9: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

1 degree

Subtracted Image

The Galactic Centre

Contours of CS emission (molecular tracer)

Source coincident with supermassive black hole Sgr A*

Diffuse Emission Emission along the

plane is revealed by subtraction of strong sources...

Correlation with molecular material

• Cosmic rays interacting with molecular clouds

Nature, Feb. 9th 2006

Page 10: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

Extragalactic Sources

4 new extragalactic sources (all blazars) PKS 2005-489, 1ES 1101-232, H 2356-309, PG 1553+113 New limits on the EBL

Confirmation of M 87 (HEGRA), PKS 2155-304 (Durham), Mrk 421

Limits on Many blazars, starburst galaxy NGC 253

Page 11: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

H.E.S.S. Phase II

artist's impression!

Page 12: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

Page 13: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

Page 14: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

Page 15: Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV

Jim Hinton 2006

2000 2002 2004

Camera 1Camera 2

+Upgrade camera 1

Camera 3Camera 4+Upgrade Cameras 1, 2 & 3

June

February

September

December

First design Letter of Intent: '97

20032001

Mirrors on1st Telescope

1st Telescope structureGroundbreaking in Namibia

1999

HESS Collaboration Founded

ARSElectronics

Proposal

2005

HESS-IExploitation andDiscovery phase!

2007

2006 2008

First discussionson low-threshold

Telescope mechanicsdesign (MAN)

SAM prototests

New Camera design

Telescope structureinstall

Mirrorsinstall

HESS-IIFirst Light

Startelectronicsseries tests

Full Camera tests