New type II Cepheids from VVV data towards the Galactic center. (arXiv:1904.12024v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Braga_V/0/1/0/all/0/1">V.F. Braga</a> (1,2), <a href="http://arxiv.org/find/astro-ph/1/au:+Ramos_R/0/1/0/all/0/1">R. Contreras Ramos</a> (1,3), <a href="http://arxiv.org/find/astro-ph/1/au:+Minniti_D/0/1/0/all/0/1">D. Minniti</a> (1,2,4), <a href="http://arxiv.org/find/astro-ph/1/au:+Lopes_C/0/1/0/all/0/1">C.E. Ferreira Lopes</a> (5), <a href="http://arxiv.org/find/astro-ph/1/au:+Catelan_M/0/1/0/all/0/1">M. Catelan</a> (3), <a href="http://arxiv.org/find/astro-ph/1/au:+Minniti_J/0/1/0/all/0/1">J.H. Minniti</a> (3,6), <a href="http://arxiv.org/find/astro-ph/1/au:+Nikzat_F/0/1/0/all/0/1">F. Nikzat</a> (3), <a href="http://arxiv.org/find/astro-ph/1/au:+Zoccali_M/0/1/0/all/0/1">M. Zoccali</a> (1,3) ((1) Instituto Milenio de Astrofísica, Santiago, Chile, (2) Departamento de Física, Facultad de Ciencias Exactas, Universidad Andrés Bello, Las Condes, Santiago, Chile, (3) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile, (4) Vatican Observatory, Vatican City State, Italy, (5) National Institute For Space Research (INPE/MCTI), S{ã}o José dos Campos — SP, Brazil, (6) European Southern Observatory, Santiago, Chile )
The Galactic center (GC) is the densest region of the Milky Way. Variability
surveys towards the GC potentially provide the largest number of variable stars
per square degree within the Galaxy. However, high stellar density is also a
drawback due to blending. Moreover, the GC is affected by extreme reddening,
therefore near infrared observations are needed. We plan to detect new variable
stars towards the GC, focusing on type II Cepheids (T2Cs) which have the
advantage of being brighter than RR Lyrae stars. We perform parallel
Lomb-Scargle and Generalized Lomb-Scargle periodogram analysis of the
$K_s$-band time series of the VISTA variables in the Via Lactea survey, to
detect periodicities. We employ statistical parameters to clean our sample. We
take account of periods, light amplitudes, distances, and proper motions to
provide a classification of the candidate variables. We detected 1,019 periodic
variable stars, of which 164 are T2Cs, 210 are Miras and 3 are classical
Cepheids. We also found the first anomalous Cepheid in this region. We compare
their photometric properties with overlapping catalogs and discuss their
properties on the color-magnitude and Bailey diagrams. We present the most
extensive catalog of T2Cs in the GC region to date. Offsets in E($J-K_s$) and
in the reddening law cause very large ($sim$1-2 kpc) uncertainties on
distances in this region. We provide a catalog which will be the starting point
for future spectroscopic surveys in the innermost regions of the Galaxy.
The Galactic center (GC) is the densest region of the Milky Way. Variability
surveys towards the GC potentially provide the largest number of variable stars
per square degree within the Galaxy. However, high stellar density is also a
drawback due to blending. Moreover, the GC is affected by extreme reddening,
therefore near infrared observations are needed. We plan to detect new variable
stars towards the GC, focusing on type II Cepheids (T2Cs) which have the
advantage of being brighter than RR Lyrae stars. We perform parallel
Lomb-Scargle and Generalized Lomb-Scargle periodogram analysis of the
$K_s$-band time series of the VISTA variables in the Via Lactea survey, to
detect periodicities. We employ statistical parameters to clean our sample. We
take account of periods, light amplitudes, distances, and proper motions to
provide a classification of the candidate variables. We detected 1,019 periodic
variable stars, of which 164 are T2Cs, 210 are Miras and 3 are classical
Cepheids. We also found the first anomalous Cepheid in this region. We compare
their photometric properties with overlapping catalogs and discuss their
properties on the color-magnitude and Bailey diagrams. We present the most
extensive catalog of T2Cs in the GC region to date. Offsets in E($J-K_s$) and
in the reddening law cause very large ($sim$1-2 kpc) uncertainties on
distances in this region. We provide a catalog which will be the starting point
for future spectroscopic surveys in the innermost regions of the Galaxy.
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