Curriculum Vitae
(January
2022)
Link to ADS
Other
publications/works
A selection of my talks, etc.
Outreach
My efforts to transmit a passion
Miguel A. Sánchez-Conde
[Slovenia, Aug 2015]
Welcome!
I’m an ‘Atracción de
Talento’ tenure-track at the Institute for Theoretical
Physics (IFT UAM-CSIC) and the Department of
Theoretical Physics, Universidad Autónoma de Madrid.
Leader of the DArk Matter, AStroparticle and COsmology
group (DAMASCO).
My current research focuses
on the search for dark matter with gamma rays.
I am a member of the
Fermi-LAT Collaboration (coordinator of the dark
matter working group), of the Cherenkov
Telescope Array (CTA) Consortium, and former member of
MAGIC.
Recently, I also joined the
DESI Collaboration.
My work also focuses on
understanding the structural properties of dark matter
halos and subhalos via numerical simulations, their
formation and evolution over cosmic time, and the
implications for dark matter searches.
Selected
(10) PUBLICATIONS
Sensitivity of the
Cherenkov Telescope Array to dark subhalos
J. Coronado-Blázquez, M.
Doro, M.A. Sánchez-Conde,
2021, PDU, 32, 100845
Unidentified gamma-ray
sources as targets for indirect dark matter detection
with the Fermi-LAT
J. Coronado-Blázquez, M.A. Sánchez-Conde, et al.,
2019, JCAP, 07, 020
Characterization of subhalo
structural properties and implications for dark matter
annihilation signals
A. Moliné, M.A. Sánchez-Conde, S.
Palomares and F. Prada, 2017, MNRAS, 466, 4974
Sensitivity
projections for dark matter searches with the Fermi
Large Area Telescope
E. Charles, M.A. Sánchez-Conde, et al.
(the Fermi LAT Collab.), 2016, Physics Reports, 636, 1
The nature of the Diffuse
Gamma-Ray Background
M. Fornasa and M.A. Sánchez-Conde, 2015,
Physics Reports, 598, 1
Limits on Dark Matter
Annihilation Signals from the Fermi LAT 4-year
Measurement of the Isotropic Gamma-ray Background
M. Ackermann et al. (The
Fermi LAT Coll., M.A.
Sánchez-Conde corresponding author), 2015,
JCAP, 09, 008
The flattening of the
concentration-halo mass relation towards low halo
masses and its implications for the annihilation
signal boost
M.A.
Sánchez-Conde and F. Prada, 2013, MNRAS, 442,
2271
Dark matter searches with
Cherenkov telescopes: nearby dwarf galaxies or local
galaxy clusters?
M.A.
Sánchez-Conde, M. Cannoni, F. Zandanel, M.
Gómez and F. Prada, 2011, JCAP, 12, 011
Hints of the existence of
Axion-Like-Particles from the gamma-ray spectra of
cosmological sources
M.A.
Sánchez-Conde, D. Paneque, E. Bloom, F. Prada
and A. Domínguez, 2009, PRD, 79, 123511
Upper limits on the VHE
gamma-ray emission from the Willman 1 satellite galaxy
with the MAGIC telescope
E. Aliu et al. (the MAGIC
Collab. M.A. Sánchez-Conde corresponding
author) 2009, ApJ, 697, 1299
My RESEARCH INTERESTS
include:
Gamma-ray dark
matter searches
Diffuse
gamma-ray backgrounds
Formation/evolution
of CDM halos
CDM
halo substructure
Numerical cosmological simulations
General: Astroparticles &
Cosmology
EDUCATION and past
POSITIONS:
Postdoc @ Oskar Klein Centre, Stockholm U.
[Sep’14
- Feb’17]
Postdoc @ KIPAC/SLAC, Stanford
[Sep’11
- Aug’14]
Postdoc @ Instituto de Astrofísica de
Canarias [Dec’09 -
Aug’11]
PhD. Astrophysics @ Universidad de Granada, Instituto
de Astrofísica de Andalucía - CSIC
[Oct 2009]
CONTACT DETAILS and CV
Institute
for Theoretical Physics (IFT)
Department of Theoretical
Physics (DFT)
Universidad Autónoma de
Madrid (UAM)
E-mail: miguel.sanchezconde@uam.es
Phone: (+34) 91 299 9867
Skype: masconde
MEMBER
of:
The Fermi
Large Area Telescope
Collaboration
(scientific coordinator of the
Dark Matter WG)
The CTA
Consortium
(former scientific coordinator of
the Dark Matter WG)
The DESI Collaboration
MULTIDARK
Spanish project
(chair of the gamma rays and cosmic
rays Dark Matter WG)
--- Last updated: 24/Jan/22 ---