YNAO OpenIR  > 系外行星研究组
Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observations
Jaimes, R. Figuera1,2; Bramich, D. M.3; Kains, N.6; Skottfelt, J.4,5; Jorgensen, U. G.5; Horne, K.1; Dominik, M.1; Alsubai, K. A.3; Bozza, V.7,8; Burgdorf, M. J.26; Novati, S. Calchi7,9,10; Ciceri, S.25; D'Ago, G.10; Evans, D. F.21; Galianni, P.1; Gu SH(顾盛宏)12,13; Harpsoe, K. B. W.5; Haugbolle, T.5; Hinse, T. C.14; Hundertmark, M.1,5; Juncher, D.5; Kerins, E.29; Korhonen, H.5,15,24; Kuffmeier, M.5; Mancini, L.11; Peixinho, N.27,28; Popovas, A.5; Rabus, M.11,16; Rahvar, S.17; Scarpetta, G.7,8,10; Schmidt, R. W.18; Snodgrass, C.19,20; Southworth, J.21; Starkey, D.1; Street, R. A.22; Surdej, J.23; Tronsgaar, R.30; Unda-Sanzana, E.27; von Essen, C.30; Wang XB(王晓彬)12,13; Wertz, O.23; MiNDSTEp Consortium
Source PublicationASTRONOMY & ASTROPHYSICS
2016-08-01
Volume592
DOI10.1051/0004-6361/201628864
Contribution Rank第12完成单位
Indexed BySCI ; EI
Keywordatmospheric effects instrumentation: high angular resolution globular clusters: individual: NGC 6715 (M54) methods: observational stars: variables: general stars: variables: RR Lyrae
Abstract

Context. We show the benefits of using electron-multiplying CCDs and the shift-and-add technique as a tool to minimise the effects of atmospheric turbulence, such as blending between stars in crowded fields, and to avoid saturated stars in the fields observed. We intend to complete, or improve on, the census of the variable star population in globular cluster NGC 6715. 

Aims. Our aim is to obtain high-precision time-series photometry of the very crowded central region of this stellar system via the collection of better angular resolution images than has been previously achieved with conventional CCDs on ground-based telescopes. 

Methods. Observations were carried out using the Danish 1.54-m telescope at the ESO La Silla observatory in Chile. The telescope is equipped with an electron-multiplying CCD that enables short-exposure-time images to be obtained (ten images per second) that were stacked using the shift-and-add technique to produce the normal-exposure-time images (minutes). The high precision photometry was performed via difference image analysis employing the DanDIA pipeline. We attempted automatic detection of variable stars in the field. 

Results. We statistically analysed the light curves of 1405 stars in the crowded central region of NGC 6715 to automatically identify the variable stars present in this cluster. We found light curves for 17 previously known variable stars near the edges of our reference image (16 RR Lyrae and 1 semi-regular) and we discovered 67 new variables (30 RR Lyrae, 21 irregular (long-period type), 3 semi-regular, 1 W Virginis, 1 eclipsing binary, and 11 unclassified). Photometric measurements for these stars are available in electronic form through the Strasbourg Astronomical Data Centre.

Funding ProjectDanish Natural Science Foundation (FNU) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation)[X-019-1-006] ; STFC[ST/M001296/1] ; POR-FSE Campania ; UK Science and Technology Facilities Council ; Sapere Aude Starting Grant from the Danish Council for Independent Research ; Danish National Research Foundation ; Korea Research Council of Fundamental Science & Technology (KRCF) via the KRCF Young Scientist Research Fellowship ; KASI[2013-9-400-00] ; KASI[2014-1-400-06] ; KASI[2015-1-850-04] ; Gemini-Conicyt Fund[32120036] ; Portuguese FCT - Foundation for Science and Technology ; European Social Fund[SFRH/BGCT/113686/2015] ; National Funds through FCT - Foundation for Science and Technology[UID/Multi/00611/2013] ; FEDER - European Regional Development Fund through COMPETE - Operational Programme Competitiveness and Internationalisation[POCI-01-0145-FEDER-006922] ; Communaute francaise de Belgique - Actions de recherche concertees - Academie Wallonie-Europe
Funding OrganizationDanish Natural Science Foundation (FNU) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation)[X-019-1-006] ; STFC[ST/M001296/1] ; POR-FSE Campania ; UK Science and Technology Facilities Council ; Sapere Aude Starting Grant from the Danish Council for Independent Research ; Danish National Research Foundation ; Korea Research Council of Fundamental Science & Technology (KRCF) via the KRCF Young Scientist Research Fellowship ; KASI[2013-9-400-00, 2014-1-400-06, 2015-1-850-04] ; Gemini-Conicyt Fund[32120036] ; Portuguese FCT - Foundation for Science and Technology ; European Social Fund[SFRH/BGCT/113686/2015] ; National Funds through FCT - Foundation for Science and Technology[UID/Multi/00611/2013] ; FEDER - European Regional Development Fund through COMPETE - Operational Programme Competitiveness and Internationalisation[POCI-01-0145-FEDER-006922] ; Communaute francaise de Belgique - Actions de recherche concertees - Academie Wallonie-Europe
Language英语
Subject Area天文学 ; 恒星与银河系
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherEDP SCIENCES S A
Publication Place17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN0004-6361
URL查看原文
WOS IDWOS:000384722600165
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSAGITTARIUS DWARF GALAXY ; RR-LYRAE VARIABLES ; DIFFERENCE IMAGE-ANALYSIS ; CROWDED CENTRAL REGION ; SPHEROIDAL GALAXY ; ACS SURVEY ; OOSTERHOFF DICHOTOMY ; DYNAMICAL MODELS ; GALACTIC BULGE ; BLACK-HOLE
EI Accession Number20163402722751
EI KeywordsStars
EI Classification Number443.1Atmospheric Properties - 657.2Extraterrestrial Physics and Stellar Phenomena - 941.4Optical Variables Measurements
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9753
Collection系外行星研究组
中国科学院天体结构与演化重点实验室
Corresponding AuthorJaimes, R. Figuera
Affiliation1.SUPA, School of Physics and Astronomy, University of St. Andrews, North Haugh, St Andrews, KY16 9SS, UK
2.European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching bei München, Germany
3.Qatar Environment and Energy Research Institute (QEERI), HBKU, Qatar Foundation, Doha, Qatar
4.Centre for Electronic Imaging, Dept. of Physical Sciences, The Open University, Milton Keynes MK7 6AA, UK
5.Niels Bohr Institute and Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5, 1350 Copenhagen K, Denmark
6.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
7.Dipartimento di Fisica “E. R. Caianiello”, Università di Salerno, via Giovanni Paolo II 132, 84084 Fisciano, Italy
8.Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, 80126 Napoli, Italy
9.NASA Exoplanet Science Institute, MS 100-22, California Institute of Technology, Pasadena CA 91125, USA
10.Istituto Internazionale per gli Alti Studi Scientifici (IIASS), 84019 Vietri Sul Mare, Italy
11.Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
12.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, PR China
13.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, PR China
14.Korea Astronomy and Space Science Institute, Daejeon 305-348, Republic of Korea
15.Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, 21500 Piikkiö, Finland
16.Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
17.Department of Physics, Sharif University of Technology, PO Box 11155-9161 Tehran, Iran
18.Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
19.Planetary and Space Sciences, Department of Physical Sciences, The Open University, Milton Keynes, MK7 6AA, UK
20.Max-Planck-Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany
21.Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
22.Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive,Suite 102, Goleta, CA 93117, USA
23.Institut d’Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 9c, 4000 Liège, Belgium
24.Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, 2100 Copenhagen Ø, Denmark
25.Department of Astronomy, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden
26.Meteorologisches Institut, Universität Hamburg, Bundesstraße 55, 20146 Hamburg, Germany
27.Universidad de Antofagasta, Unidad de Astronomía, Facultad Cs. Básicas, Av. U. de Antofagasta, 02800 Antofagasta, Chile
28.20 CITEUC – Centre for Earth and Space Science Research of the University of Coimbra, Observatório Astronómico da Universidade de Coimbra, 3040-004 Coimbra, Portugal
29.Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M139 PL, UK
30.Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark
Recommended Citation
GB/T 7714
Jaimes, R. Figuera,Bramich, D. M.,Kains, N.,et al. Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observations[J]. ASTRONOMY & ASTROPHYSICS,2016,592.
APA Jaimes, R. Figuera.,Bramich, D. M..,Kains, N..,Skottfelt, J..,Jorgensen, U. G..,...&MiNDSTEp Consortium.(2016).Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observations.ASTRONOMY & ASTROPHYSICS,592.
MLA Jaimes, R. Figuera,et al."Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observations".ASTRONOMY & ASTROPHYSICS 592(2016).
Files in This Item:
File Name/Size DocType Version Access License
Many new variable st(4711KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Jaimes, R. Figuera]'s Articles
[Bramich, D. M.]'s Articles
[Kains, N.]'s Articles
Baidu academic
Similar articles in Baidu academic
[Jaimes, R. Figuera]'s Articles
[Bramich, D. M.]'s Articles
[Kains, N.]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Jaimes, R. Figuera]'s Articles
[Bramich, D. M.]'s Articles
[Kains, N.]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: Many new variable stars discovered in the core of the globular cluster NGC 6715 (M 54) with EMCCD observations.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.