ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO

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ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
Astroparticle physics in
     Poland’ 2019

       Tomasz Bulik
    University of Warsaw
     AstroCeNT, CAMK
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
Institutions and experiments
UW: University of Warsaw (HESS, CTA, VIRGO, ET, LSST, KM3NET, Hyper K)
UJ: Jagiellonian University (HESS, CTA, LSST, Virgo, Hyper K)
UMK: Nicolaus Copernicus University (HESS, CTA, LSST)
UŁ: University of Łódź (HESS, CTA, Auger)
UwB: University of Białystok (CTA, VIRGO, ET)
UZG: University of Zielona Gora (VIRGO, ET, CTA)
CAMK: Nicolaus Copernicus Astronomical Center, PAS (HESS, CTA, VIRGO, ET, Athena, LSST,
DarkSide, GADMC, DEAP)
IFJ: Institute of Nuclear Physics, PAS (HESS, CTA, HAWC, CREDO, Auger, BAIKAL)
IM: Institute of Mathematics, PAS(VIRGO, ET)
CBK: Cosmic Research Center, PAS (Athena, CTA)
NCBJ: National Center for Nuclear Research (CTA, CREDO, VIRGO, KM3NET,LSST, Hyper K, JEM-
EUSO)
CFT: Center for Theoretical Studies, PAS (LSST)
PW: Warsaw University of Technology (CTA)
US: University of Silesia (Hyper K)
AGH: University of Science and Technology (CTA, CREDO)
UWr: University of Wrocław (LSST, VIRGO)
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
Areas covered
●
    HE astronomy
    –   Photons
    –   Cosmic rays
●
    Neutrinos
●
    Gravitational waves
●
    Dark matter
●
    Cosmology
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
X and Gamma ray -
          astronomy
●
    Athena
●
    HESS
●
    MAGIC
●
    CTA
●
    HAWC
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
Athena
 ●
     Novel X-ray telescope, ESA large mission to be launched 2031
 ●
     CAMK,CBK
 ●
     R&D for two instruments-
 ●
     WFI: Filter Wheel Assembly (FWA) and Power Distribution Unit (PDU) with
     Filter Wheel Controller (FWC) and Remote Terminal Unit Power Board (RTUPB)
     X-IFU: Dewar Door (DD), Power Distribution Unit (PDU) and Latch-up Current
     Limiter (LCL).

The Polish groups are responsible for design, manufacture and delivery of   all the
subsystems.

 ●
     Current financing at 2.049 M€,planned 8.5M€
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
H.E.S.S.

●
    HE energy telescope in Namibia, Poland is a
    member since 2006
●
    UJ, UW, CAMK, IFJ, UMK
●
    Constributed collimation system for HESS II,
    mirrors, operating costs, shifts
●
    Funding from NCN totaling 8.5MPLN since 2006
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
MAGIC

●
    HE energy telescope in La Palma,
    observing for 15 years
●
    UŁ
●
    Common funds, shifts
●
    Participation in telescope activities
    including TOC, software, group
    leadership
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
CTA

●
    Next generation gamma ray observatory
●
    JU,IFJ, CAMK, UŁ, AGH, CBK, NCBJ, UMK, UZG, UwB,
    PW
●
    SST-1M project, mirrors for MST, LST commissioning,
    computing, site search and characterization, electronics
●
    Previous grants – 3.5M€, currently SST-1M – 1.6M€, and
    350k€ current costs.
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
HAWC

●
    Water Cherenkov gamma ray
    observatory in Mexico. Fully
    operational
●
    IFJ, 2.5 FTE and one PhD
●
    Data analysis, PMT calibration
●
    Two grants from NCN
ASTROPARTICLE PHYSICS IN POLAND' 2019 - TOMASZ BULIK UNIVERSITY OF WARSAW ASTROCENT, CAMK - CERN INDICO
Cosmic rays
●
    Auger
●
    CREDO
●
    JEM-EUSO
Auger

●
    High energy cosmic ray detector in Argentina.
●
    IFJ and UŁ
●
    Contributions: fluorescence detector parts,
    electronic components, assembly and testing
    of scintillator detectors
●
    Hardware 628kUSD, common fund 798kUSD
CREDO

●
    Cosmic Ray Extremely Distributed
    Observatory
●
    IFJ, AGH, NCBJ, UŁ
●
    Software, phone apps, citizen
    science
●
    Two grants – total ~30k€
JEM-EUSO

●
    Space project to study extremely high
    energy cosmic rays, R&D stage
●
    NCBJ
●
    Polish contribution: high voltage power
    supply for PMTs, simulation data
    analysis, tests
●
    3 grants from NCN: total 1.1 M PLN
Neutrinos
●
    KM3NET
●
    Hyper K – see dr Łagoda’s talk
●
    BAIKAL
KM3Net
●
    Underwater neutrino observatory
    in the Mediterranean
●
    NCBJ
●
    Computing, software, simulations
●
    Current funding from NCN
    ~300kPLN/year
BAIKAL-GVD

●
    Deep underwater neutrino Cherenkov telescope looking for
    high energy neutrinos from astrophysical sources
●
    IFJ, 4 members, (2 FTE+1 student)
●
    Activities: data analysis, simulations, development of the
    acquisition software, R&D of the laser calibration system,
    and participation in tests and construction of the telescope.
Gravitational waves
●
    Virgo
●
    Einstein Telescope
VIRGO

●
    Gravitational wave observatory near Pisa Italy.
●
    IM, UW, CAMK, UwB, UZG, UWr, AGH
●
    Engineer on site, vacuum pumps. Seismic data
    acquisition system. Data analysis and
    simulations
●
    Funding: 5.6MPLN since 2010 form NCN,
    currently investment grant 4.3MPLN, and FNP
    program on Newtonian Noise 3.5 M PLN
ET
●
    Future 3rd generation
    GW observatory. Currently in early stage
●
    UW, PW, CAMK, IM, UwB, UZG, UwB
●
    ET future site characterizanion, science
    case, involvement in ET steering committee
●
    Site characterization – 1.3 MPLN from
    NCN, currently no direct funding
Cosmology
●
    LSST
LSST

●
    Large Synoptic Survey Telescope, in
    construction
●
    NCBJ, UJ, UW, UMK, CAMK, CFT
●
    Contributing part of operating costs
●
    Ministry grant for participation fee 86k$, +
    grants from NCN
Dark matter
●
    DarkSide
●
    Global Argon Dark Matter
    Collaboration
●
    DEAP
DEAP,DS,
     GADMC
●
    DEAP - currently taking data
●
    DEAP – AstroCeNT, DS, GADMC (UJ,
    AstroCeNT)
●
    Work on R&D, SiPMs, data acquisition, data
    analysis
●
    Radiopurity studies DS: UJ, AstroCeNT
●
    Funded through ActroCeNT
Astrocent
●
    A new addition to the Polish astroparticle scene
●
    International Research Agenda devoted to
    science and technology development for
    astroparticle physics
●
    Part of CAMK
●
    Already involved in VIRGO, DarkSide, Hyper-K,
    GADMC, DEAP
●
    Funding ~38M PLN for 5 years
LSST   Athen   HESS   MAGI   CTA   HAWC   CRED   Auger   Virgo   ET   KM3N   JEM-   BAIKA   DarkSi   DEAP   GADM
             a              C                   O                           ET     EUSO   L-GVD   de              C

UW     X              X             X                           X       X    X
UJ     X              X             X                           X                                 X
UMK    X              X             X
UŁ                           X      X                   X
UwB                                 X                           X       X
UZG                                 X                           X       X
CAM    X      X       X             X                           X       X                         X        X      X
K

IFJ                   X             X     X      X      X                                 X
IM                                                              X       X
CBK           X                     X
NCB    X                            X            X              X            X      X
J

CFT    X
PW                                  X
US

AGH                                 X            X
UWr
       X                                                        X
Summary
●
    Astroparticle physics is alive and well
●
     There is shift towards consolidating efforts to join
    new big flagship experiments, rather than maintain
    scattered presence
●
    With AstroCeNT the level of funding for the field has
    dramatically increased, and gives potential and
    good prospects for much more
●
    There is a number of theoretical studies not covered
    here as well.
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