text:
DESCRIPTION = "Qt Thermostat Demo"
HOMEPAGE = "https://gitorious.org/thermostat-demo"

LICENSE = "BSD & CC-BY-SA-2.0 & CC-BY-SA-3.0 & MIT"
LIC_FILES_CHKSUM = "file://LICENSE;md5=93a105adb99011afa5baee932b560714 \
                    file://IMAGE-LICENSE;md5=fce98146123de13a189c234a5e4cfa0d \
                    file://API-LICENSE;md5=5e32280d79a1eab76729c50d79ecfe72 \
                    file://remote/MIT-LICENSE.txt;md5=6a24093faaae5d5c198578c88e220071 \
"

require recipes-core/matrix/matrix-gui-paths.inc

inherit qt-provider

PR = "r9"

DEPENDS += "${QT_DEPENDS_SVG} ${QT_DEPENDS_SCRIPT}"

BRANCH ?= "master"
SRCREV = "2512773c2d9da989e6a42c1e90b2b34496713072"

SRC_URI = " \
	git://gitorious.org/thermostat-demo/thermostat-demo.git;protocol=git \
"

SRC_URI += "${@base_conditional('QT_PROVIDER', 'qt5', 'file://0002-Replace-QtGui-with-QtWidgets-per-Qt5-migration-guide.patch \
	file://0003-Replace-fromAscii-toAscii-with-fromLatin1-toLatin1-p.patch', '', d)}"

S = "${WORKDIR}/git/"

do_install() {
	install -d ${D}/usr/bin
	install -m 0755 ${B}/ThermostatDemo ${D}/usr/bin/ThermostatDemo
	install -d ${D}${MATRIX_APP_DIR}/qt_tstat
	cp -rf ${S}/matrix-files/*  ${D}${MATRIX_APP_DIR}/qt_tstat
}

PACKAGES += "matrix-gui-thermostat-demo"

RDEPENDS_matrix-gui-thermostat-demo += "matrix-gui-apps-images matrix-gui-submenus-qt4"

FILES_matrix-gui-thermostat-demo += "${MATRIX_APP_DIR}/*"

repository: varigit/meta-arago-var

repo_name: varigit/meta-arago-var


text:
package output

import (
	"crypto/sha256"
	"fmt"
)

type File struct {
	name string
	content []byte
	origin string
	hash string
}

// Creates a new file object and calculates the hash of the given content
func NewFile(name string, content []byte, origin string) File {
	hash := fmt.Sprintf("%x", sha256.Sum256(content))[:6]
	return File{
		name:    name,
		content: content,
		origin:  origin,
		hash:    hash,
	}
}

license: MIT

repository: maride/pancap

license_type: permissive

repo_name: maride/pancap

branch_name: refs/heads/master

extension: go


text:
@MISC{Rybizki2018,
       author = {{Rybizki}, Jan and {Drimmel}, Ronald},
        title = "{gdr2\_completeness: GaiaDR2 data retrieval and manipulation}",
     keywords = {Software},
         year = "2018",
        month = "Nov",
          eid = {ascl:1811.018},
        pages = {ascl:1811.018},
archivePrefix = {ascl},
       eprint = {1811.018},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ascl.soft11018R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Jayasinghe2018b,
   author = {{Jayasinghe}, T. and {Stanek}, K.~Z. and {Kochanek}, C.~S. and
	{Shappee}, B.~J. and {Holoien}, T.~W.-S. and {Thompson}, T.~A. and
	{Prieto}, J.~L. and {Dong}, S. and {Pawlak}, M. and {Pejcha}, O. and
	{Shields}, J.~V. and {Pojmanski}, G. and {Otero}, S. and {Britt}, C.~A. and
	{Will}, D.},
    title = "{The ASAS-SN Catalog of Variable Stars II: Uniform Classification of 412,000 Known Variables}",
  journal = {arXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1809.07329},
 primaryClass = "astro-ph.SR",
 keywords = {Astrophysics - Solar and Stellar Astrophysics},
     year = 2018,
    month = sep,
   adsurl = {http://adsabs.harvard.edu/abs/2018arXiv180907329J},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Shapee2014,
   author = {{Shappee}, B.~J. and {Prieto}, J.~L. and {Grupe}, D. and {Kochanek}, C.~S. and
	{Stanek}, K.~Z. and {De Rosa}, G. and {Mathur}, S. and {Zu}, Y. and
	{Peterson}, B.~M. and {Pogge}, R.~W. and {Komossa}, S. and {Im}, M. and
	{Jencson}, J. and {Holoien}, T.~W.-S. and {Basu}, U. and {Beacom}, J.~F. and
	{Szczygie{\l}}, D.~M. and {Brimacombe}, J. and {Adams}, S. and
	{Campillay}, A. and {Choi}, C. and {Contreras}, C. and {Dietrich}, M. and
	{Dubberley}, M. and {Elphick}, M. and {Foale}, S. and {Giustini}, M. and
	{Gonzalez}, C. and {Hawkins}, E. and {Howell}, D.~A. and {Hsiao}, E.~Y. and
	{Koss}, M. and {Leighly}, K.~M. and {Morrell}, N. and {Mudd}, D. and
	{Mullins}, D. and {Nugent}, J.~M. and {Parrent}, J. and {Phillips}, M.~M. and
	{Pojmanski}, G. and {Rosing}, W. and {Ross}, R. and {Sand}, D. and
	{Terndrup}, D.~M. and {Valenti}, S. and {Walker}, Z. and {Yoon}, Y.
	},
    title = "{The Man behind the Curtain: X-Rays Drive the UV through NIR Variability in the 2013 Active Galactic Nucleus Outburst in NGC 2617}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1310.2241},
 primaryClass = "astro-ph.HE",
 keywords = {galaxies: active, galaxies: nuclei, galaxies: Seyfert, line: formation, line: profiles},
     year = 2014,
    month = jun,
   volume = 788,
      eid = {48},
    pages = {48},
      doi = {10.1088/0004-637X/788/1/48},
   adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...788...48S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Schlegel1998,
author = {David J Schlegel and Douglas P Finkbeiner and Marc Davis},
journal = {\apj},
title = {Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds},
pages = {525},
volume = {500},
year = {1998},
month = {Jun},
keywords = {ISM: DUST, COSMOLOGY: COSMIC MICROWAVE BACKGROUND, INTERPLANETARY MEDIUM, COSMOLOGY: DIFFUSE RADIATION, INFRARED: ISM: CONTINUUM, EXTINCTION},
date-added = {2010-06-20 00:01:39 -0430},
date-modified = {2010-06-20 00:01:39 -0430},
doi = {10.1086/305772},
pmid = {1998ApJ...500..525S},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ApJ...500..525S&link_type=ABSTRACT},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p2254},
rating = {0}
}

@article{Catelan2004,
author = {M Catelan and Barton J Pritzl and Horace A Smith},
journal = {\apjs},
title = {The RR Lyrae Period-Luminosity Relation. I. Theoretical Calibration},
abstract = {We present a theoretical calibration of the RR Lyrae period-luminosity (PL) relation in the UBVRIJHK Johnson-Cousins-Glass system. Our theoretical work is based on calculations of synthetic horizontal branches (HBs) for several different metallicities, fully taking into account evolutionary effects besides the effect of chemical composition. Extensive tabulations of our results are provided, including convenient analytical formulae for the calculation of the coefficients of the period-luminosity relation in the different passbands as a function of HB type. We also provide ``average'' PL relations in IJHK, for applications in cases where the HB type is not known a priori; as well as a new calibration of the MV-[M/H] relation. These can be summarized as follows:MI=0.471-1.132logP+0.205logZ, MJ=-0.141-1.773logP+0.190logZ, MH=-0.551-2.313logP+0.178logZ, MK=-0.597-2.353logP+0.175logZ, andMV=2.288+0.882logZ+0.108(logZ)2.},
affiliation = {AA(Departamento de Astronom{\'\i}a y Astrof{\'\i}sica, Pontificia Universidad Cat{\'o}lica de Chile, Avenida Vicu{\~n}a Mackenna 4860, 782-0436 Macul, Santiago, Chile; mcatelan@astro.puc.cl), AB(Macalester College, 1600 Grand Avenue, Saint Paul, MN 55105; pritzl@macalester.edu), AC(Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824; smith@pa.msu.edu)},
pages = {633},
volume = {154},
year = {2004},
month = {Oct},
keywords = {STARS: VARIABLES: OTHER, Stars: Horizontal-Branch, Cosmology: Distance Scale},
date-added = {2010-04-20 14:06:13 -0430},
date-modified = {2010-04-22 08:46:59 -0430},
doi = {10.1086/422916},
pmid = {2004ApJS..154..633C},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ApJS..154..633C&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Catelan_2004.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p2200},
read = {Yes},
rating = {0}
}

@article{Neeley2017,
author = {Neeley, Jillian R and Marengo, Massimo and Bono, Giuseppe and Braga, Vittorio F and Dall'Ora, Massimo and Magurno, Davide and Marconi, Marcella and Trueba, Nicolas and Tognelli, Emanuele and Moroni, Pier G Prada and Beaton, Rachael L and Freedman, Wendy L and Madore, Barry F and Monson, Andrew J and Scowcroft, Victoria and Seibert, Mark and Stetson, Peter B},
title = {{On a new theoretical framework for RR Lyrae stars II: Mid--Infrared Period--Luminosity--Metallicity Relations}},
journal = {arXiv},
year = {2017},
eprint = {1705.01970v1},
eprinttype = {arxiv},
eprintclass = {astro-ph.SR},
month = may
}

@ARTICLE{Evans2018,
       author = {{Evans}, D.~W. and {Riello}, M. and {De Angeli}, F. and {Carrasco},
        J.~M. and {Montegriffo}, P. and {Fabricius}, C. and {Jordi}, C.
        and {Palaversa}, L. and {Diener}, C. and {Busso}, G. and
        {Cacciari}, C. and {van Leeuwen}, F.},
        title = "{Gaia Data Release 2: Photometric content and validation}",
      journal = {ArXiv e-prints},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = Apr,
          eid = {arXiv:1804.09368},
        pages = {arXiv:1804.09368},
archivePrefix = {arXiv},
       eprint = {1804.09368},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2018arXiv180409368E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Molnar2018,
       author = {{Moln{\'a}r}, L{\'a}szl{\'o} and {Plachy}, Emese and {Juh{\'a}sz},
        {\'A}ron L. and {Rimoldini}, Lorenzo},
        title = "{Gaia Data Release 2: Validation of the classification of RR Lyrae and
        Cepheid variables with the Kepler and K2 missions}",
      journal = {ArXiv e-prints},
     keywords = {Astrophysics - Solar and Stellar Astrophysics},
         year = 2018,
        month = May,
          eid = {arXiv:1805.11395},
        pages = {arXiv:1805.11395},
archivePrefix = {arXiv},
       eprint = {1805.11395},
 primaryClass = {Astrophysics - Solar and Stellar Astrophysics},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2018arXiv180511395M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{GaiaColEyer2018,
       author = {{Gaia Collaboration} and {Eyer}, L. and {Rimoldini}, L. and {Audard}, M.
        and {Anderson}, R.~I. and {Nienartowicz}, K. and {Glass}, F. and
        {Marchal}, O. and {Grenon}, M. and {Mowlavi}, N. and {Holl}, B.
        and {Clementini}, G. and {Aerts}, C. and {Mazeh}, T. and
        {Evans}, D.~W. and {Szabados}, L. and {co-authors}, 438},
        title = "{Gaia Data Release 2: Variable stars in the colour-absolute magnitude
        diagram}",
      journal = {ArXiv e-prints},
     keywords = {Astrophysics - Solar and Stellar Astrophysics},
         year = 2018,
        month = Apr,
          eid = {arXiv:1804.09382},
        pages = {arXiv:1804.09382},
archivePrefix = {arXiv},
       eprint = {1804.09382},
 primaryClass = {Astrophysics - Solar and Stellar Astrophysics},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2018arXiv180409382G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Holl2018,
       author = {{Holl}, B. and {Audard}, M. and {Nienartowicz}, K. and {Jevardat de
        Fombelle}, G. and {Marchal}, O. and {Mowlavi}, N. and
        {Clementini}, G. and {De Ridder}, J. and {Evans}, D.~W. and
        {Guy}, L.~P. and {Lanzafame}, A.~C. and {Lebzelter}, T. and
        {Rimoldini}, L. and {Roelens}, M. and {Zucker}, S. and
        {Distefano}, E. and {Garofalo}, A. and {Lecoeur-Ta{\"\i}bi}, I.
        and {Lopez}, M. and {Molinaro}, R. and {Muraveva}, T. and
        {Panahi}, A. and {Regibo}, S. and {Ripepi}, V. and {Sarro},
        L.~M. and {Aerts}, C. and {Anderson}, R.~I. and {Charnas}, J.
        and {Barblan}, F. and {Blanco-Cuaresma}, S. and {Busso}, G. and
        {Cuypers}, J. and {De Angeli}, F. and {Glass}, F. and {Grenon},
        M. and {Juh{\'a}sz}, {\'A}. L. and {Kochoska}, A. and {Koubsky},
        P. and {Lanza}, A.~F. and {Leccia}, S. and {Lorenz}, D. and
        {Marconi}, M. and {Marschalk}, G. and {Mazeh}, T. and {Messina},
        S. and {Mignard}, F. and {Moitinho}, A. and {Moln{\'a}r}, L. and
        {Morgenthaler}, S. and {Musella}, I. and {Ordenovic}, C. and
        {Ord{\'o}{\~n}ez}, D. and {Pagano}, I. and {Palaversa}, L. and
        {Pawlak}, M. and {Plachy}, E. and {Pr{\v{s}}a}, A. and {Riello},
        M. and {S{\"u}veges}, M. and {Szabados}, L. and {Szegedi-Elek},
        E. and {Votruba}, V. and {Eyer}, L.},
        title = "{Gaia Data Release 2: Summary of the variability processing \&
        analysis results}",
      journal = {ArXiv e-prints},
     keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics -
        Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = Apr,
          eid = {arXiv:1804.09373},
        pages = {arXiv:1804.09373},
archivePrefix = {arXiv},
       eprint = {1804.09373},
 primaryClass = {Astrophysics - Solar and Stellar Astrophysics},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2018arXiv180409373H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Muraveva2018,
       author = {{Muraveva}, Tatiana and {Delgado}, Hector E. and {Clementini}, Gisella
        and {Sarro}, Luis M. and {Garofalo}, Alessia},
        title = "{RR Lyrae stars as standard candles in the Gaia Data Release 2 Era}",
      journal = {ArXiv e-prints},
     keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics -
        Astrophysics of Galaxies},
         year = 2018,
        month = May,
          eid = {arXiv:1805.08742},
        pages = {arXiv:1805.08742},
archivePrefix = {arXiv},
       eprint = {1805.08742},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2018arXiv180508742M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Miceli2008,
author = {Antonino Miceli and Armin Rest and Christopher W Stubbs and Suzanne L Hawley and Kem H Cook and Eugene A Magnier and Kevin Krisciunas and Edward Bowell and Bruce Koehn},
journal = {\apj},
title = {Evidence for Distinct Components of the Galactic Stellar Halo from 838 RR Lyrae Stars Discovered in the LONEOS-I Survey},
abstract = {We present 838 ab-type RR Lyrae stars from the Lowell Observatory Near Earth Objects Survey Phase I (LONEOS-I). These objects cover 1430 deg2 and span distances ranging from 3 to 30 kpc from the Galactic center. Object selection is based on phased, photometric data with 28-50 epochs. We use this large sample to explore the bulk properties of the stellar halo, including the spatial distribution. The period-amplitude distribution of this sample shows that the majority of these RR Lyrae stars resemble Oosterhoff type I, but there is a significant fraction (26%) which have longer periods and appear to be Oosterhoff type II. We find that the radial distributions of these two populations have significantly different profiles (ρOoI~R-2.26+/-0.07 and ρOoII~R-2.88+/-0.11). This suggests that the stellar halo was formed by at least two distinct accretion processes and supports dual-halo models.},
affiliation = {AA(Astronomy and Physics Departments, University of Washington, Box 351580, Seattle, WA 98195-1580 amiceli@astro.washington.edu), AB(Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile; arest@ctio.noao.edu), AC(Department of Physics and Harvard-Smithsonian Center for Astrophysics, Harvard University, 17 Oxford Street, Cambridge, MA 02138), AD(Astronomy Department, University of Washington, Box 351580, Seattle, WA 98195-1580), AE(Lawrence Livermore N...},
pages = {865},
volume = {678},
year = {2008},
month = {May},
keywords = {Galaxies: Structure, Galaxies: Halos, galaxies: individual (Milky Way)},
date-added = {2009-12-04 13:01:31 -0430},
date-modified = {2010-06-03 20:24:29 -0430},
doi = {10.1086/533484},
pmid = {2008ApJ...678..865M},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...678..865M&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Miceli_2008.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p1958},
read = {Yes},
rating = {0}
}

@article{Cacciari2005,
author = {C Cacciari and T. M Corwin and B. W Carney},
journal = {\aj},
title = {A Multicolor and Fourier Study of RR Lyrae Variables in the Globular Cluster NGC 5272 (M3)},
abstract = {We have performed a detailed study of the pulsational and evolutionary characteristics of 133 RR Lyrae stars in the globular cluster NGC 5272 (M3) using highly accurate BVI data taken on five separate epochs. M3 seems to contain no less than ~32% of Blazhko stars, and the occurrence and characteristics of the Blazhko effect have been analyzed in detail. We have identified a good number (~14%) of overluminous RR Lyrae stars that are likely in a more advanced evolutionary stage off the zero-age horizontal branch (ZAHB). Physical parameters (i.e., temperature, luminosity, and mass) have been derived from B-V colors and accurate color-temperature calibration, and compared with horizontal-branch evolutionary models and with the requirements of stellar pulsation theory. Additional analysis by means of Fourier decomposition of the V light curves confirms, as expected, that no metallicity spread is present in M3. Evolution off the ZAHB does not affect [Fe/H] determinations, whereas Blazhko stars at low amplitude phase do affect [Fe/H] distributions, as they appear more metal-rich. Absolute magnitudes derived from Fourier coefficients might provide useful average estimates for groups of stars, if applicable, but do not give reliable individual values. Intrinsic colors derived from Fourier coefficients show significant discrepancies with the observed ones, and hence the resulting temperatures and temperature-related parameters are unreliable.},
affiliation = {AA(Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, Italy; cacciari@bo.astro.it), AB(Department of Physics, University of North Carolina, Charlotte, NC 28223; mcorwin@uncc.edu), AC(Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599; bruce@astro.unc.edu)},
pages = {267},
volume = {129},
year = {2005},
month = {Jan},
keywords = {STARS: VARIABLES: OTHER, Galaxy: Globular Clusters: Individual: Messier Number: M3, Stars: Fundamental Parameters},
date-added = {2010-04-30 09:38:59 -0430},
date-modified = {2010-04-30 09:40:04 -0430},
doi = {10.1086/426325},
pmid = {2005AJ....129..267C},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005AJ....129..267C&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Cacciari_2005.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p2207},
read = {Yes},
rating = {0}
}

@article{Drake2013a,
author = {Drake, A J and Catelan, M and Djorgovski, S G and Torrealba, G and Graham, M J and Belokurov, V and Koposov, S E and Mahabal, A and Prieto, J L and Donalek, C and Williams, R and Larson, S and Christensen, E and Beshore, E},
title = {{PROBING THE OUTER GALACTIC HALO WITH RR LYRAE FROM THE CATALINA SURVEYS}},
journal = {\apj},
year = {2013},
volume = {763},
number = {1},
pages = {32},
month = jan
}

@article{Kunder2010,
author = {Andrea Kunder and Brian Chaboyer and Andrew Layden},
journal = {\aj},
title = {The Determination of Reddening from Intrinsic VR Colors of RR Lyrae Stars},
abstract = {New R-band observations of 21 local field RR Lyrae variable stars are used to explore the reliability of minimum light (V - R) colors as a tool for measuring interstellar reddening. For each star, R-band intensity mean magnitudes and light amplitudes are presented. Corresponding V-band light curves from the literature are supplemented with the new photometry, and (V - R) colors at minimum light are determined for a subset of these stars as well as for other stars in the literature. Two different definitions of minimum light color are examined, one which uses a Fourier decomposition to the V and R light curves to find (V - R) at minimum V-band light, (V - R) F min, and the other which uses the average color between the phase interval 0.5-0.8, (V - R)phi(0.5-0.8) min. From 31 stars with a wide range of metallicities and pulsation periods, the mean dereddened RR Lyrae color at minimum light is (V - R) F min,0 = 0.28 $\pm$ 0.02 mag and (V - R)phi(0.5-0.8) min,0 = 0.27 $\pm$ 0.02 mag. As was found by Guldenschuh et al. using (V - I) colors, any dependence of the star's minimum light color on metallicity or pulsation amplitude is too weak to be formally detected. We find that the intrinsic (V - R) of Galactic bulge RR Lyrae stars are similar to those found by their local counterparts and hence that bulge RR0 Lyrae stars do not have anomalous colors as compared to the local RR Lyrae stars.},
affiliation = {AA(Dartmouth College, 6127 Wilder Lab, Hanover, NH 03755, USA Andrea.M.Kunder@dartmouth.edu), AB(Dartmouth College, 6127 Wilder Lab, Hanover, NH 03755, USA Brian.Chaboyer@dartmouth.edu), AC(Bowling Green State University, Bowling Green, OH 43403, USA layden@baade.bgsu.edu)},
pages = {415},
volume = {139},
year = {2010},
month = {Feb},
keywords = {STARS: ABUNDANCES, dust, extinction, stars: distances, , stars: Population II, Galaxy: center, Stars: Horizontal-Branch},
date-added = {2010-04-14 14:10:02 -0430},
date-modified = {2010-04-14 14:11:15 -0430},
doi = {10.1088/0004-6256/139/2/415},
pmid = {2010AJ....139..415K},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010AJ....139..415K&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Kunder_2010.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p2193},
read = {Yes},
rating = {0}
}

@ARTICLE{Zinn2014,
   author = {{Zinn}, R. and {Horowitz}, B. and {Vivas}, A.~K. and {Baltay}, C. and
	{Ellman}, N. and {Hadjiyska}, E. and {Rabinowitz}, D. and {Miller}, L.
	},
    title = "{La Silla QUEST RR Lyrae Star Survey: Region I}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1312.1602},
 keywords = {galaxies: individual: Sextans, Galaxy: halo, stars: variables: RR Lyrae, surveys},
     year = 2014,
    month = jan,
   volume = 781,
      eid = {22},
    pages = {22},
      doi = {10.1088/0004-637X/781/1/22},
   adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...781...22Z},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Harris2010,
   author = {{Harris}, W.~E.},
    title = "{A New Catalog of Globular Clusters in the Milky Way}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1012.3224},
 primaryClass = "astro-ph.GA",
 keywords = {Astrophysics - Galaxy Astrophysics},
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}

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}
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}
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}

@ARTICLE{Jurcsik2017,
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	{Nuspl}, J. and {Kolenberg}, K. and {F{\H u}r{\'e}sz}, G. and
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	},
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archivePrefix = "arXiv",
   eprint = {1702.03264},
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 keywords = {techniques: photometric, techniques: radial velocities, stars: horizontal branch, stars: oscillations (including pulsations), stars: variables: RR Lyrae, globular clusters: individual: M3},
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  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Jurcsik2014,
   author = {{Jurcsik}, J. and {Smitola}, P. and {Hajdu}, G. and {Nuspl}, J.
	},
    title = "{On the Modulation of RR Lyrae Stars in the Globular Cluster M3}",
  journal = {\apjl},
archivePrefix = "arXiv",
   eprint = {1411.1987},
 primaryClass = "astro-ph.SR",
 keywords = {globular clusters: individual: Messier 3, stars: horizontal-branch, stars: oscillations, stars: variables: RR Lyrae },
     year = 2014,
    month = dec,
   volume = 797,
      eid = {L3},
    pages = {L3},
      doi = {10.1088/2041-8205/797/1/L3},
   adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...797L...3J},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Jurcsik2012,
   author = {{Jurcsik}, J. and {Hajdu}, G. and {Szeidl}, B. and {Ol{\'a}h}, K. and
	{Kelemen}, J. and {S{\'o}dor}, {\'A}. and {Saha}, A. and {Mallick}, P. and
	{Claver}, J.},
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  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1109.4525},
 primaryClass = "astro-ph.SR",
 keywords = {stars: evolution, stars: horizontal branch, stars: oscillations, stars: variables: RR Lyrae, globular clusters: individual: M3},
     year = 2012,
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  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{LeeCarney1999,
   author = {{Lee}, J.-W. and {Carney}, B.~W.},
    title = "{RR Lyrae Luminosity Differences between Oosterhoff Group I and II Cluster Systems and the Origin of the Oosterhoff Dichotomy}",
  journal = {\aj},
 keywords = {GALAXY: FORMATION-GLOBULAR CLUSTERS: INDIVIDUAL (NGC 5272, NGC 7089), STARS: VARIABLES: RR LYRAE VARIABLE, STARS: HORIZONTAL-BRANCH, STARS: LUMINOSITY FUNCTION, MASS FUNCTION},
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    month = sep,
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    pages = {1373-1389},
      doi = {10.1086/301008},
   adsurl = {http://adsabs.harvard.edu/abs/1999AJ....118.1373L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Groenewegen2017,
   author = {{Groenewegen}, M.~A.~T.},
    title = "{Variable stars in the Gaia era: Mira, RR Lyrae, delta and Type-II Cepheids}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1706.02911},
 primaryClass = "astro-ph.SR",
 keywords = {Astrophysics - Solar and Stellar Astrophysics},
     year = 2017,
    month = jun,
   adsurl = {http://adsabs.harvard.edu/abs/2017arXiv170602911G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Clement1999,
   author = {{Clement}, C.~M. and {Shelton}, I.},
    title = "{The RR Lyrae Period-Amplitude Relation as a Clueto the Origin of the Oosterhoff Dichotomy}",
  journal = {\apjl},
   eprint = {astro-ph/9902289},
 keywords = {GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M3, GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M4, GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M5, GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M9, GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M68, GLOBULAR CLUSTERS: INDIVIDUAL (M92, M107), STARS: FUNDAMENTAL PARAMETERS, STARS: HORIZONTAL-BRANCH, STARS: VARIABLES: OTHER: (RR LYRAE), Galaxy: Globular Clusters: Individual: Messier Number: M3, Galaxy: Globular Clusters: Individual: Messier Number: M4, Galaxy: Globular Clusters: Individual: Messier Number: M5, Galaxy: Globular Clusters: Individual: Messier Number: M9, Galaxy: Globular Clusters: Individual: Messier Number: M68, globular clusters: individual (M92, Stars: Fundamental Parameters, Stars: Horizontal-Branch, Stars: Variables: Other: (RR Lyrae)},
     year = 1999,
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   adsurl = {http://adsabs.harvard.edu/abs/1999ApJ...515L..85C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Zorotovic2010,
   author = {{Zorotovic}, M. and {Catelan}, M. and {Smith}, H.~A. and {Pritzl}, B.~J. and
	{Aguirre}, P. and {Angulo}, R.~E. and {Aravena}, M. and {Assef}, R.~J. and
	{Contreras}, C. and {Cort{\'e}s}, C. and {De Martini}, G. and
	{Escobar}, M.~E. and {Gonz{\'a}lez}, D. and {Jofr{\'e}}, P. and
	{Lacerna}, I. and {Navarro}, C. and {Palma}, O. and {Prieto}, G.~E. and
	{Recabarren}, E. and {Trivi{\~n}o}, J. and {Vidal}, E.},
    title = "{The Globular Cluster NGC 5286. II. Variable Stars}",
  journal = {\aj},
archivePrefix = "arXiv",
   eprint = {0911.1686},
 primaryClass = "astro-ph.SR",
 keywords = {galaxies: dwarf, galaxies: star clusters, globular clusters: individual: NGC 5286, Hertzsprung-Russell diagram, stars: variables: other},
     year = 2010,
    month = feb,
   volume = 139,
    pages = {357-371},
      doi = {10.1088/0004-6256/139/2/357},
   adsurl = {http://adsabs.harvard.edu/abs/2010AJ....139..357Z},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{GaiaEyer2018,
   author = {{Gaia Collaboration} and {Eyer}, L. and {Rimoldini}, L. and
	{Audard}, M. and {Anderson}, R.~I. and {Nienartowicz}, K. and
	{Glass}, F. and {Marchal}, O. and {Grenon}, M. and {Mowlavi}, N. and
	{Holl}, B. and {Clementini}, G. and {Aerts}, C. and {Mazeh}, T. and
	{Evans}, D.~W. and {Szabados}, L. and {co-authors}, 4.},
    title = "{Gaia Data Release 2: Variable stars in the colour-absolute magnitude diagram}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1804.09382},
 primaryClass = "astro-ph.SR",
 keywords = {Astrophysics - Solar and Stellar Astrophysics},
     year = 2018,
    month = apr,
   adsurl = {http://adsabs.harvard.edu/abs/2018arXiv180409382G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Rimoldini2018,
   author = {{Rimoldini}, L. and {Eyer}, L. and {Mowlavi}, N. and {Evans}, D.~W. and
	{Nienartowicz}, K. and {Holl}, B. and {Audard}, M. and {Guy}, L.~P. and
	{Jevardat de Fombelle}, G. and {Lecoeur-Ta{\"i}bi}, I. and {Marchal}, O. and
	{Clementini}, G. and {Ripepi}, V. and {Garofalo}, A. and {Molinaro}, R. and
	{Muraveva}, T. and {Poretti}, E. and {Moln{\'a}r}, L. and {Plachy}, E. and
	{Juh{\'a}sz}, {\'A}.~L. and {Szabados}, L. and {De Ridder}, J. and
	{Regibo}, S. and {Sarro Baro}, L.~M. and {L{\'o}pez del Fresno}, M.
	},
    title = "{All-sky RR Lyrae Stars in the Gaia Data}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1804.04079},
 primaryClass = "astro-ph.SR",
 keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
     year = 2018,
    month = apr,
   adsurl = {http://adsabs.harvard.edu/abs/2018arXiv180404079R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Clementini2018,
   author = {{Clementini}, G. and {Ripepi}, V. and {Molinaro}, R. and {Garofalo}, A. and
	{Muraveva}, T. and {Rimoldini}, L. and {Guy}, L.~P. and {Jevardat de Fombelle}, G. and
	{Nienartowicz}, K. and {Audard}, M. and {Holl}, B. and {Leccia}, S. and
	{Marconi}, M. and {Musella}, I. and {Mowlavi}, N. and {Lecoeur-Taibi}, I. and
	{Eyer}, L. and {De Ridder}, J. and {Regibo}, S. and {Sarro}, L.~M. and
	{Szabados}, L. and {Evans}, D.~W. and {Riello}, M.},
    title = "{Gaia Data Release 2: Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1805.02079},
 primaryClass = "astro-ph.SR",
 keywords = {Astrophysics - Solar and Stellar Astrophysics},
     year = 2018,
    month = may,
   adsurl = {http://adsabs.harvard.edu/abs/2018arXiv180502079C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Catelan2004a,
   author = {{Catelan}, M. and {Pritzl}, B.~J. and {Smith}, H.~A.},
    title = "{The RR Lyrae Period-Luminosity Relation. I. Theoretical Calibration}",
  journal = {\apjs},
   eprint = {astro-ph/0406067},
 keywords = {Cosmology: Distance Scale, Stars: Horizontal-Branch, Stars: Variables: Other},
     year = 2004,
    month = oct,
   volume = 154,
    pages = {633-649},
      doi = {10.1086/422916},
   adsurl = {http://adsabs.harvard.edu/abs/2004ApJS..154..633C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Catelan2004b,
   author = {{Catelan}, M.},
    title = "{The Evolutionary Status of M3 RR Lyrae Variable Stars: Breakdown of the Canonical Framework?}",
  journal = {\apj},
   eprint = {astro-ph/0309188},
 keywords = {Galaxy: Globular Clusters: Individual: Messier Number: M3, Galaxy: Globular Clusters: Individual: Messier Number: M5, Stars: Evolution, Stars: Horizontal-Branch, Stars: Population II, Stars: Variables: Other},
     year = 2004,
    month = jan,
   volume = 600,
    pages = {409-418},
      doi = {10.1086/379657},
   adsurl = {http://adsabs.harvard.edu/abs/2004ApJ...600..409C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{Kinemuchi2006,
author = {K Kinemuchi and H. A Smith and P. R Wo{\'z}niak and T. A McKay},
journal = {\aj},
title = {Analysis of RR Lyrae Stars in the Northern Sky Variability Survey},
abstract = {We use data from the Northern Sky Variability Survey (NSVS), obtained from the first-generation Robotic Optical Transient Search Experiment (ROTSE-I), to identify and study RR Lyrae variable stars in the solar neighborhood. We initially identified 1197 RRab (RR0) candidate stars brighter than the ROTSE median magnitude V=14. Periods, amplitudes, and mean V magnitudes are determined for a subset of 1188 RRab stars with well-defined light curves. Metallicities are determined for 589 stars by the Fourier parameter method and by the relationship between period, amplitude, and [Fe/H]. We comment on the difficulties of clearly classifying RRc (RR1) variables in the NSVS data set. Distances to the RRab stars are calculated using an adopted luminosity-metallicity relation with corrections for interstellar extinction. The 589 RRab stars in our final sample are used to study the properties of the RRab population within 5 kpc of the Sun. The Bailey diagram of period versus amplitude shows that the largest component of this sample belongs to Oosterhoff type I. Metal-rich ([Fe/H]>-1) RRab stars appear to be associated with the Galactic disk. Our metal-rich RRab sample may include a thin-disk, as well as a thick-disk population, although the uncertainties are too large to establish this. There is some evidence among the metal-rich RRab stars for a decline in scale height with increasing [Fe/H], as was found by Layden. The distribution of RRab stars with -1<[Fe/H]<-1.25 indicates that within this metallicity range the RRab stars are a mixture of stars belonging to halo and disk populations.},
affiliation = {AA(Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824; Current address: Department of Physics and Astronomy, University of Wyoming, Department 3905, Laramie, WY 82071.), AB(Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824), AC(Los Alamos National Laboratory, Los Alamos, NM 87545), AD(Department of Physics, University of Michigan, 2477 Randall Laboratory, Ann Arbor, MI 48109)},
note = {(c) 2006: The American Astronomical Society},
pages = {1202},
volume = {132},
year = {2006},
month = {Sep},
keywords = {Stars: Variables: Other, Galaxy: Disk},
date-added = {2009-04-13 13:34:29 -0430},
date-modified = {2010-04-17 10:17:57 -0430},
doi = {10.1086/506198},
pmid = {2006AJ....132.1202K},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006AJ....132.1202K&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Kinemuchi_2006.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p1792},
read = {Yes},
rating = {0}
}

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	{Bailyn}, C. and {Baltay}, C. and {Bongiovanni}, A. and {Brice{\~n}o}, C. and
	{Bruzual}, G. and {Coppi}, P. and {Della Prugna}, F. and {Ellman}, N. and
	{Ferr{\'{\i}}n}, I. and {Gebhard}, M. and {Girard}, T. and {Hernandez}, J. and
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	{Schaefer}, B. and {Schenner}, H. and {Snyder}, J.~A. and {Sofia}, S. and
	{Stock}, J. and {van Altena}, W. and {Vicente}, B. and {Vieira}, K.
	},
    title = "{The QUEST RR Lyrae Survey. I. The First Catalog}",
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 keywords = {Galaxy: Halo, Stars: Variables: Other, Surveys},
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    pages = {1158-1175},
      doi = {10.1086/380929},
   adsurl = {http://adsabs.harvard.edu/abs/2004AJ....127.1158V},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Sesar2017c,
   author = {{Sesar}, B. and {Hernitschek}, N. and {Mitrovi{\'c}}, S. and
	{Ivezi{\'c}}, {\v Z}. and {Rix}, H.-W. and {Cohen}, J.~G. and
	{Bernard}, E.~J. and {Grebel}, E.~K. and {Martin}, N.~F. and
	{Schlafly}, E.~F. and {Burgett}, W.~S. and {Draper}, P.~W. and
	{Flewelling}, H. and {Kaiser}, N. and {Kudritzki}, R.~P. and
	{Magnier}, E.~A. and {Metcalfe}, N. and {Tonry}, J.~L. and {Waters}, C.
	},
    title = "{Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample}",
  journal = {\aj},
archivePrefix = "arXiv",
   eprint = {1611.08596},
 keywords = {catalogs, Galaxy: halo, methods: data analysis, methods: statistical, stars: variables: RR Lyrae, surveys},
     year = 2017,
    month = may,
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      eid = {204},
    pages = {204},
      doi = {10.3847/1538-3881/aa661b},
   adsurl = {http://adsabs.harvard.edu/abs/2017AJ....153..204S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Clementini2016b,
   author = {{Clementini}, G. and {Ripepi}, V. and {Leccia}, S. and {Mowlavi}, N. and
	{Lecoeur-Taibi}, I. and {Marconi}, M. and {Szabados}, L. and
	{Eyer}, L. and {Guy}, L.~P. and {Rimoldini}, L. and {Jevardat de Fombelle}, G. and
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	{De Angeli}, F. and {De Ridder}, J. and {Debosscher}, J. and
	{Evans}, D.~W. and {Klagyivik}, P. and {Musella}, I. and {Nienartowicz}, K. and
	{Ord{\'o}{\~n}ez}, D. and {Regibo}, S. and {Riello}, M. and
	{Sarro}, L.~M. and {S{\"u}veges}, M.},
    title = "{Gaia Data Release 1. The Cepheid and RR Lyrae star pipeline and its application to the south ecliptic pole region}",
  journal = {\aap},
archivePrefix = "arXiv",
   eprint = {1609.04269},
 primaryClass = "astro-ph.SR",
 keywords = {stars: general, stars: oscillations, stars: variables: Cepheids, stars: variables: RR Lyrae, methods: data analysis, Magellanic Clouds},
     year = 2016,
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      eid = {A133},
    pages = {A133},
      doi = {10.1051/0004-6361/201629583},
   adsurl = {http://adsabs.harvard.edu/abs/2016A%26A...595A.133C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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@ARTICLE{Muraveva2015,
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      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Drake2013b,
author = {Drake, A J and Catelan, M and Djorgovski, S G and Torrealba, G and Graham, M J and Mahabal, A and Prieto, J L and Donalek, C and Williams, R and Larson, S and Christensen, E and Beshore, E},
title = {{EVIDENCE FOR A MILKY WAY TIDAL STREAM REACHING BEYOND 100 kpc}},
journal = {\apj},
year = {2013},
volume = {765},
number = {2},
pages = {154},
month = feb
}

@article{Drake2013a,
author = {Drake, A J and Catelan, M and Djorgovski, S G and Torrealba, G and Graham, M J and Belokurov, V and Koposov, S E and Mahabal, A and Prieto, J L and Donalek, C and Williams, R and Larson, S and Christensen, E and Beshore, E},
title = {{PROBING THE OUTER GALACTIC HALO WITH RR LYRAE FROM THE CATALINA SURVEYS}},
journal = {\apj},
year = {2013},
volume = {763},
number = {1},
pages = {32},
month = jan
}

@ARTICLE{Torrealba2015,
   author = {{Torrealba}, G. and {Catelan}, M. and {Drake}, A.~J. and {Djorgovski}, S.~G. and
	{McNaught}, R.~H. and {Belokurov}, V. and {Koposov}, S. and
	{Graham}, M.~J. and {Mahabal}, A. and {Larson}, S. and {Christensen}, E.
	},
    title = "{Discovery of {\tilde}9000 new RR Lyrae in the southern Catalina surveys}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1410.7653},
 keywords = {methods: data analysis, methods: statistical, stars: variables: RR Lyrae, Galaxy: halo, Galaxy: structure},
     year = 2015,
    month = jan,
   volume = 446,
    pages = {2251-2266},
      doi = {10.1093/mnras/stu2274},
   adsurl = {http://adsabs.harvard.edu/abs/2015MNRAS.446.2251T},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Lafler1965,
author = {J Lafler and T. D Kinman},
journal = {ApJ Supplement},
title = {An RR Lyrae Star Survey with Ihe Lick 20-INCH Astrograph II. The Calculation of RR Lyrae Periods by Electronic Computer.},
abstract = {Abstract image available at: http://adsabs.harvard.edu/abs/1965ApJS...11..216L},
pages = {216},
volume = {11},
year = {1965},
month = {Jun},
date-added = {2010-01-19 13:50:31 -0430},
date-modified = {2010-01-19 13:50:47 -0430},
doi = {10.1086/190116},
pmid = {1965ApJS...11..216L},
URL = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965ApJS...11..216L&link_type=ABSTRACT},
local-url = {file://localhost/Users/cmateu/trabajo/articulos/Papers/Lafler_1965.pdf},
uri = {papers://3CF19FFD-9F37-4577-AFDC-1D7F0F338DCB/Paper/p2095},
rating = {0}
}

@ARTICLE{Schlafly2011,
       author = {{Schlafly}, Edward F. and {Finkbeiner}, Douglas P.},
        title = "{Measuring Reddening with Sloan Digital Sky Survey Stellar Spectra and
        Recalibrating SFD}",
      journal = {\apj},
     keywords = {dust, extinction, Galaxy: stellar content, ISM: clouds, Astrophysics -
        Galaxy Astrophysics},
         year = 2011,
        month = Aug,
       volume = {737},
          eid = {103},
        pages = {103},
          doi = {10.1088/0004-637X/737/2/103},
archivePrefix = {arXiv},
       eprint = {1012.4804},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2011ApJ...737..103S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Dambis2013,
       author = {{Dambis}, A.~K. and {Berdnikov}, L.~N. and {Kniazev}, A.~Y. and
        {Kravtsov}, V.~V. and {Rastorguev}, A.~S. and {Sefako}, R. and
        {Vozyakova}, O.~V.},
        title = "{RR Lyrae variables: visual and infrared luminosities, intrinsic colours
        and kinematics}",
      journal = {\mnras},
     keywords = {stars: distances, stars: kinematics and dynamics, stars: variables: RR
        Lyrae, Local Group, distance scale, Astrophysics - Galaxy
        Astrophysics},
         year = 2013,
        month = Nov,
       volume = {435},
        pages = {3206-3220},
          doi = {10.1093/mnras/stt1514},
archivePrefix = {arXiv},
       eprint = {1308.4727},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.3206D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

extension: bib


text:
/*
 *
 * Copyright 2020 gRPC authors.
 *
 * Licensed under the Apache License, Version 2.0 (the "License");
 * you may not use this file except in compliance with the License.
 * You may obtain a copy of the License at
 *
 *     http://www.apache.org/licenses/LICENSE-2.0
 *
 * Unless required by applicable law or agreed to in writing, software
 * distributed under the License is distributed on an "AS IS" BASIS,
 * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
 * See the License for the specific language governing permissions and
 * limitations under the License.
 *
 */

package weightedtarget

import (
	"encoding/json"
	"fmt"
	"google.golang.org/grpc/balancer/apis"
	"testing"
	"time"

	"github.com/google/go-cmp/cmp"
	"google.golang.org/grpc/attributes"
	"google.golang.org/grpc/balancer"
	"google.golang.org/grpc/balancer/roundrobin"
	"google.golang.org/grpc/connectivity"
	"google.golang.org/grpc/internal/hierarchy"
	"google.golang.org/grpc/resolver"
	"google.golang.org/grpc/serviceconfig"
	"google.golang.org/grpc/xds/internal/balancer/balancergroup"
	"google.golang.org/grpc/xds/internal/testutils"
)

type testConfigBalancerBuilder struct {
	balancer.Builder
}

func newTestConfigBalancerBuilder() *testConfigBalancerBuilder {
	return &testConfigBalancerBuilder{
		Builder: balancer.Get(roundrobin.Name),
	}
}

func (t *testConfigBalancerBuilder) Build(cc balancer.ClientConn, opts balancer.BuildOptions) balancer.Balancer {
	rr := t.Builder.Build(cc, opts)
	return &testConfigBalancer{
		Balancer: rr,
	}
}

const testConfigBalancerName = "test_config_balancer"

func (t *testConfigBalancerBuilder) Name() string {
	return testConfigBalancerName
}

type stringBalancerConfig struct {
	serviceconfig.LoadBalancingConfig
	s string
}

func (t *testConfigBalancerBuilder) ParseConfig(c json.RawMessage) (serviceconfig.LoadBalancingConfig, error) {
	// Return string without quotes.
	return stringBalancerConfig{s: string(c[1 : len(c)-1])}, nil
}

// testConfigBalancer is a roundrobin balancer, but it takes the balancer config
// string and append it to the backend addresses.
type testConfigBalancer struct {
	balancer.Balancer
}

func (b *testConfigBalancer) UpdateClientConnState(s balancer.ClientConnState) error {
	c, ok := s.BalancerConfig.(stringBalancerConfig)
	if !ok {
		return fmt.Errorf("unexpected balancer config with type %T", s.BalancerConfig)
	}
	oneMoreAddr := resolver.Address{Addr: c.s}
	s.BalancerConfig = nil
	s.ResolverState.Addresses = append(s.ResolverState.Addresses, oneMoreAddr)
	return b.Balancer.UpdateClientConnState(s)
}

func (b *testConfigBalancer) Close() {
	b.Balancer.Close()
}

var (
	wtbBuilder          balancer.Builder
	wtbParser           balancer.ConfigParser
	testBackendAddrStrs []string
)

const testBackendAddrsCount = 12

func init() {
	balancer.Register(newTestConfigBalancerBuilder())
	for i := 0; i < testBackendAddrsCount; i++ {
		testBackendAddrStrs = append(testBackendAddrStrs, fmt.Sprintf("%d.%d.%d.%d:%d", i, i, i, i, i))
	}
	wtbBuilder = balancer.Get(weightedTargetName)
	wtbParser = wtbBuilder.(balancer.ConfigParser)

	balancergroup.DefaultSubBalancerCloseTimeout = time.Millisecond
}

// TestWeightedTarget covers the cases that a sub-balancer is added and a
// sub-balancer is removed. It verifies that the addresses and balancer configs
// are forwarded to the right sub-balancer.
//
// This test is intended to test the glue code in weighted_target. Most of the
// functionality tests are covered by the balancer group tests.
func TestWeightedTarget(t *testing.T) {
	cc := testutils.NewTestClientConn(t)
	wtb := wtbBuilder.Build(cc, balancer.BuildOptions{})

	// Start with "cluster_1: round_robin".
	config1, err := wtbParser.ParseConfig([]byte(`{"targets":{"cluster_1":{"weight":1,"childPolicy":[{"round_robin":""}]}}}`))
	if err != nil {
		t.Fatalf("failed to parse balancer config: %v", err)
	}

	// Send the config, and an address with hierarchy path ["cluster_1"].
	wantAddr1 := resolver.Address{Addr: testBackendAddrStrs[0], Attributes: nil}
	if err := wtb.UpdateClientConnState(balancer.ClientConnState{
		ResolverState: resolver.State{Addresses: []resolver.Address{
			hierarchy.Set(wantAddr1, []string{"cluster_1"}),
		}},
		BalancerConfig: config1,
	}); err != nil {
		t.Fatalf("failed to update ClientConn state: %v", err)
	}

	// Verify that a subconn is created with the address, and the hierarchy path
	// in the address is cleared.
	addr1 := <-cc.NewSubConnAddrsCh
	if want := []resolver.Address{
		hierarchy.Set(wantAddr1, []string{}),
	}; !cmp.Equal(addr1, want, cmp.AllowUnexported(attributes.Attributes{})) {
		t.Fatalf("got unexpected new subconn addrs: %v", cmp.Diff(addr1, want, cmp.AllowUnexported(attributes.Attributes{})))
	}

	// Send subconn state change.
	sc1 := <-cc.NewSubConnCh
	wtb.UpdateSubConnState(sc1, balancer.SubConnState{ConnectivityState: connectivity.Connecting})
	wtb.UpdateSubConnState(sc1, balancer.SubConnState{ConnectivityState: connectivity.Ready})

	// Test pick with one backend.
	p1 := <-cc.NewPickerCh
	for i := 0; i < 5; i++ {
		gotSCSt, _ := p1.Pick(balancer.PickInfo{})
		if !cmp.Equal(gotSCSt.SubConn, sc1, cmp.AllowUnexported(testutils.TestSubConn{})) {
			t.Fatalf("picker.Pick, got %v, want SubConn=%v", gotSCSt, sc1)
		}
	}

	// Remove cluster_1, and add "cluster_2: test_config_balancer".
	wantAddr3Str := testBackendAddrStrs[2]
	config2, err := wtbParser.ParseConfig([]byte(
		fmt.Sprintf(`{"targets":{"cluster_2":{"weight":1,"childPolicy":[{%q:%q}]}}}`, testConfigBalancerName, wantAddr3Str),
	))
	if err != nil {
		t.Fatalf("failed to parse balancer config: %v", err)
	}

	// Send the config, and one address with hierarchy path "cluster_2".
	wantAddr2 := resolver.Address{Addr: testBackendAddrStrs[1], Attributes: nil}
	if err := wtb.UpdateClientConnState(balancer.ClientConnState{
		ResolverState: resolver.State{Addresses: []resolver.Address{
			hierarchy.Set(wantAddr2, []string{"cluster_2"}),
		}},
		BalancerConfig: config2,
	}); err != nil {
		t.Fatalf("failed to update ClientConn state: %v", err)
	}

	// Expect the address sent in the address list. The hierarchy path should be
	// cleared.
	addr2 := <-cc.NewSubConnAddrsCh
	if want := []resolver.Address{
		hierarchy.Set(wantAddr2, []string{}),
	}; !cmp.Equal(addr2, want, cmp.AllowUnexported(attributes.Attributes{})) {
		t.Fatalf("got unexpected new subconn addrs: %v", cmp.Diff(addr2, want, cmp.AllowUnexported(attributes.Attributes{})))
	}
	// Expect the other address sent as balancer config. This address doesn't
	// have hierarchy path.
	wantAddr3 := resolver.Address{Addr: wantAddr3Str, Attributes: nil}
	addr3 := <-cc.NewSubConnAddrsCh
	if want := []resolver.Address{wantAddr3}; !cmp.Equal(addr3, want, cmp.AllowUnexported(attributes.Attributes{})) {
		t.Fatalf("got unexpected new subconn addrs: %v", cmp.Diff(addr3, want, cmp.AllowUnexported(attributes.Attributes{})))
	}

	// The subconn for cluster_1 should be removed.
	scToRemove := <-cc.RemoveSubConnCh
	if !cmp.Equal(scToRemove, sc1, cmp.AllowUnexported(testutils.TestSubConn{})) {
		t.Fatalf("RemoveSubConn, want %v, got %v", sc1, scToRemove)
	}
	wtb.UpdateSubConnState(scToRemove, balancer.SubConnState{ConnectivityState: connectivity.Shutdown})

	sc2 := <-cc.NewSubConnCh
	wtb.UpdateSubConnState(sc2, balancer.SubConnState{ConnectivityState: connectivity.Connecting})
	wtb.UpdateSubConnState(sc2, balancer.SubConnState{ConnectivityState: connectivity.Ready})
	sc3 := <-cc.NewSubConnCh
	wtb.UpdateSubConnState(sc3, balancer.SubConnState{ConnectivityState: connectivity.Connecting})
	wtb.UpdateSubConnState(sc3, balancer.SubConnState{ConnectivityState: connectivity.Ready})

	// Test roundrobin pick with backends in cluster_2.
	p2 := <-cc.NewPickerCh
	want := []apis.SubConn{sc2, sc3}
	if err := testutils.IsRoundRobin(want, subConnFromPicker(p2)); err != nil {
		t.Fatalf("want %v, got %v", want, err)
	}
}

func subConnFromPicker(p balancer.Picker) func() apis.SubConn {
	return func() apis.SubConn {
		scst, _ := p.Pick(balancer.PickInfo{})
		return scst.SubConn
	}
}

gha_language: Go


text:
SUMMARY = "A dot-accessible dictionary (a la JavaScript objects)"
LICENSE = "MIT"
LIC_FILES_CHKSUM = "file://LICENSE.txt;md5=f0291cd32b2d6a91d9b19970c94d0a46"

SRC_URI = "https://github.com/F483/neobunch/archive/v${PV}.tar.gz"

SRC_URI[md5sum] = "487cc5023ba049fdf1bdd3a9e71280f2"
SRC_URI[sha256sum] = "f5a3eac5ba1413efd3754b4d21c1137653d33d67240f00edfb2e169db782cbc3"

inherit setuptools

RDEPENDS_${PN} = "python-six"

repository: xuechuance/meta-printing

repo_name: xuechuance/meta-printing

extension: bb