期刊
ASTRONOMY & ASTROPHYSICS
卷 605, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201629925
关键词
astrometry; parallaxes; stars: distances; stars: variables: Cepheids; stars: variables: RR Lyrae; methods: data analysis
资金
- Agenzia Spaziale Italiana (ASI) [I/037/08/0, I/058/10/0, 2014-025-R.0, 2014-025-R.1.2015, I/008/10/0, 2013/030/I.0]
- Algerian Centre de Recherche en Astronomie, Astrophysique et Geophysique of Bouzareah Observatory
- Austrian FWF Hertha Firnberg Programme [T359, P20046, P23737]
- BELgian federal Science Policy Office (BELSPO) through various PROgramme de Developpement d'Experiences scientifiques (PRODEX)
- Brazil-France exchange programmes FAPESPCOFECUB
- CAPES-COFECUB
- the Chinese National Science Foundation [NSFC 11573054]
- Czech-Republic Ministry of Education, Youth, and Sports [LG 15010]
- Danish Ministry of Science
- Estonian Ministry of Education and Research [IUT401]
- European Commission's Sixth Framework Programme through the European Leadership in Space Astrometry (ELSA) Marie Curie Research Training Network [MRTN-CT-2006-033481]
- European Commission's Sixth Framework Programme through Marie Curie Transfer-of-Knowledge (ToK) fellowship [MTKD-CT-2004-014188]
- European Commission [FP7-606740, 264895]
- European Research Council (ERC) [320360]
- European Union's Horizon 2020 research and innovation programme [670519]
- European Science Foundation (ESF)
- European Space Agency
- European Space Agency Plan for European Cooperating States (PECS) programme through grants for Slovenia
- Czech Space O ffice through ESA PECS contract [98058]
- Academy of Finland
- Magnus Ehrnrooth Foundation
- French Centre National de la Recherche Scientifique (CNRS) through action Defi MASTODONS
- French Centre National d'Etudes Spatiales (CNES)
- French L'Agence Nationale de la Recherche (ANR) investissements d'avenir Initiatives D'EXcellence (IDEX) programme PSL [ANR-10IDEX-0001-02]
- Region Aquitaine
- Universite de Bordeaux
- French Utinam Institute of the Universite de Franche-Comte
- Region de Franche-Comte
- Institut des Sciences de l'Univers (INSU)
- German Aerospace Agency (Deutsches Zentrum fur Luft-und Raumfahrt e.V., DLR) [50QG0501, 50QG0601, 50QG0602, 50QG0701, 50QG0901, 50QG1001, 50QG1101, 50QG140, 50QG1401, 50QG1402, 50QG1404]
- Hungarian Academy of Sciences through Lendulet Programme [LP2014-17]
- Hungarian National Research, Development, and Innovation O ffice [NKFIH K-115709, K-119517, PD-116175]
- Israel Ministry of Science and Technology [3-9082]
- Italian Istituto Nazionale di Astrofisica (INAF)
- Netherlands Organisation for Scientific Research (NWO) [NWO-M-614.061.414]
- VICI grant
- Netherlands Research School for Astronomy (NOVA)
- Polish National Science Centre through HARMONIA grant [2015/18/M/ST9/00544]
- Portugese Fundacao para a Ciencia e a Tecnologia (FCT) [PTDC/CTE-SPA/118692/2010, PDCTE/CTEAST/81711/2003, SFRH/BPD/74697/2010, PEstOE/AMB/UI4006/2011, UID/FIS/00099/2013, UID/EEA/00066/2013]
- Slovenian Research Agency
- Spanish Ministry of Economy MINECO-FEDER [AyA201455216, AyA2011-24052, ESP2013-48318-C2-R]
- ICCUB (Unidad de Excelencia Maria de Maeztu) [MDM-2014-0369, ESP2014-55996-C2-R]
- Swedish National Space Board (SNSB/Rymdstyrelsen)
- Swiss State Secretariat for Education, Research, and Innovation through the ESA PRODEX programme
- Swiss Mesures d'Accompagnement
- Swiss Activites Nationales Complementaires
- Swiss National Science Foundation
- United Kingdom Rutherford Appleton Laboratory
- United Kingdom Science and Technology Facilities Council (STFC) [PP/C506756/1, ST/I00047X/1]
- United Kingdom Space Agency (UKSA) [ST/K000578/1, ST/N000978/1]
Context. Parallaxes for 331 classical Cepheids, 31 Type II Cepheids, and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release 1 (DR1) as part of the Tycho-Gaia Astrometric Solution (TGAS). Aims. In order to test these first parallax measurements of the primary standard candles of the cosmological distance ladder, which involve astrometry collected by Gaia during the initial 14 months of science operation, we compared them with literature estimates and derived new period-luminosity (PL), period-Wesenheit (PW) relations for classical and Type II Cepheids and infrared PL, PL-metallicity (PLZ), and optical luminosity-metallicity (M-V-[Fe/H]) relations for the RR Lyrae stars, with zero points based on TGAS. Methods. Classical Cepheids were carefully selected in order to discard known or suspected binary systems. The final sample comprises 102 fundamental mode pulsators with periods ranging from 1.68 to 51.66 days (of which 33 with sigma(pi)/pi < 0.5). The Type II Cepheids include a total of 26 W Virginis and BL Herculis stars spanning the period range from 1.16 to 30.00 days (of which only 7 with sigma(pi)/pi < 0.5). The RR Lyrae stars include 200 sources with pulsation period ranging from 0.27 to 0.80 days (of which 112 with sigma(pi)/pi < 0.5). The new relations were computed using multi-band (V,I,J,K-s) photometry and spectroscopic metal abundances available in the literature, and by applying three alternative approaches: (i) linear least-squares fitting of the absolute magnitudes inferred from direct transformation of the TGAS parallaxes; (ii) adopting astrometry-based luminosities; and (iii) using a Bayesian fitting approach. The last two methods work in parallax space where parallaxes are used directly, thus maintaining symmetrical errors and allowing negative parallaxes to be used. The TGAS-based PL,PW,PLZ, and M-V- [Fe/H] relations are discussed by comparing the distance to the Large Magellanic Cloud provided by different types of pulsating stars and alternative fitting methods. Results. Good agreement is found from direct comparison of the parallaxes of RR Lyrae stars for which both TGAS and HST measurements are available. Similarly, very good agreement is found between the TGAS values and the parallaxes inferred from the absolute magnitudes of Cepheids and RR Lyrae stars analysed with the Baade-Wesselink method. TGAS values also compare favourably with the parallaxes inferred by theoretical model fitting of the multi-band light curves for two of the three classical Cepheids and one RR Lyrae star, which were analysed with this technique in our samples. The K-band PL relations show the significant improvement of the TGAS parallaxes for Cepheids and RR Lyrae stars with respect to the Hipparcos measurements. This is particularly true for the RR Lyrae stars for which improvement in quality and statistics is impressive. Conclusions. TGAS parallaxes bring a significant added value to the previous Hipparcos estimates. The relations presented in this paper represent the first Gaia-calibrated relations and form a work-in-progress milestone report in the wait for Gaia-only parallaxes of which a first solution will become available with Gaia Data Release 2 (DR2) in 2018.
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