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VHE ray detectors in the Sierra Negra site

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Instituto Nacional de Astrof sica, ptica y Electr nica. Future Gamma-ray Observatories ... ray astronomy with GTM/LMT: the synergy with GLAST ... – PowerPoint PPT presentation

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Title: VHE ray detectors in the Sierra Negra site


1
VHE ?-ray detectors in the Sierra Negra site
  • Alberto Carramiñana
  • Instituto Nacional de Astrofísica, Óptica y
    Electrónica
  • Future Gamma-ray Observatories
  • Santa Fe, NM 12-May-2006

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Cofre de Perote
La Malinche
Sierra Negra Citlaltepetl
Popo Izta
Nevado de Toluca
Elección sitio, 1997
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?100 km
Ciudad de México
Sierra Negra
Puebla
Orizaba
Córdoba
7
?-ray astronomy with GTM/LMT the synergy with
GLAST
SEQUOIA Array of 32 heterodyne receivers tunable
between 80 and 115 GHz
SPEED Array of 4 frequency selective bolometers ?
simultaneous observations at 2.1, 1.4, 1.1 and
0.85mm.
  • The history of (obscured) galaxy formation in the
    Universe mm path to the EBL
  • 3 mm VLBI?
    Imaging the Galactic center back hole
  • Gamma-ray bursts
    afterglows host galaxies
  • Blazars
    multiwavelength IR background formation of
    AGNs
  • Nearby galaxies
    CO mapping ? GLAST emission models

AzTEC Bolometer camera (144) ? continuum
mapping at 1mm.
redshifts receiver has seen its first light
8
Typical rms sensitivity ? 3 mJy.Hz1/2
9
Consorcio Sierra Negra
  • Sierra Negra
  • from 4.6 km (15,000 feet) altitude
  • 19 latitude N
  • 4.5 hrs drive from Mexico City 2 hr from
    Puebla.
  • Consorcio SN All experiments at Sierra Negra
    site
  • GTM the 50m millimeter telescope (INAOE
    UMass)
  • RT5 solar and ISM 5m radio telescope
    (INAOE, IGeoUNAM, IAUNAM)
  • Solar neutron monitor in operation!
    (IGeoUNAM)
  • Antineutrones in construction (IFUNAM)
  • Rayos cósmicos operative in expansion (FCFM
    - BUAP)
  • Seismological study of Citlaltepetl
    (FI - BUAP)
  • MiniHawc?

10
HE Solar neutron event at Sierra Negra
Espectro de neutrones solares para el evento del
7 septiembre 2005
I ? E-3.9 para Egt100 MeV
11
Interest for MiniHAWC in Mexican institutions
  • UNAM I. Ciencias Nucleares
  • Lukas Nelllen (AGN - Auger)
  • G. Medina-Tanco (HECR)
  • UNAM I. Geofísica
  • José Valdés Galicia (Sun)
  • Alejandro Lara (Sun)
  • Universidad de Puebla
  • Humberto Salazar (CR)
  • Oscar Martínez (CR astro)
  • Cesar Álvarez (CR astro)
  • L. Díaz, Arturo Fernández
  • Universidad Michoacan
  • Luis Villaseñor (CR - Auger)
  • CINVESTAV
  • Arnulfo Zepeda (CR - Auger)
  • Universidad de Guanajuato
  • David Delepine, Moreno, Napsuciale, Reyes, Ureña
    (particles)
  • Andernach, Coziol, Migenes (astronomy dept)
  • INAOE
  • Alberto Carramiñana (gamma astronomy - LMT
    synergy)
  • Eduardo Mendoza (Sun, ISM)
  • UNAM Inst. Astronomía
  • Magdalena González (GRBs)
  • Dany Page (NS - th)
  • William Lee (GRBs - th)
  • Hector Hernández (opt. mw)
  • UNAM Inst. Física
  • Arturo Menchaca (CR - exp)
  • Rubén Alfaro (CR - exp)
  • Andres Sandoval (CR - exp)
  • Ernesto Belmont (CR - exp)

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Citlaltepetl y Sierra Negra, marzo 2003
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1 km
14
MiniHawc feasability
  • Identified location at 4050m
  • National Park authorities contacted and
    supportive (Consorcio SN promotes the National
    Park Management Plan).
  • First quotation and study for bringing up water
    (at 10 l/s ? 4 months)
  • Quotations for studies
    for demelting and digging
    the pond in process

15
Further possibilities
  • A 4_at_4 in Sierra Negra (spot at 4.3km)
  • San Pedro Mártir very dark site in the Baja
    California at 2.8 km with the OAN
    facilities
  • A deep search for dark, high duty cycle and
    extended sites above 2.5 - 3 km? ?
    infrastructure development
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