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物理  2015 

lamost银河系大规模光谱巡天计划的进展和展望

, PP. 213-227

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Abstract:

?大天区面积多目标光纤光谱天文望远镜(lamost,又称郭守敬望远镜)是一台新型准中星仪式反射施密特望远镜。其有效口径4m,视场20平方度,配备了16台摄谱仪和4000根光纤,可同时获取至多4000个天体的光谱。光谱覆盖为370—910nm,分辨率为1800。为期5年的lamost银河系大规模恒星光谱巡天计划已于2012年秋启动,计划获取超过700万条恒星光谱,截至2014年6月已获得超过300万条光谱。文章简要回顾了银河系研究的重要性和现状,介绍了lamost银河系光谱巡天计划的科学意义和目标,数据采集、处理和分析进展以及已获得的初步科研成果,并对lamost银河系光谱巡天计划的未来进行了展望。

References

[1]  nordstr?mbetal.astronomyandastrophysics,2004,418:989
[2]  yorkdgetal.theastronomicaljournal,2000,120:1579
[3]  yannybetal.theastronomicaljournal,2009,137:4377
[4]  zhanghhetal.researchinastronomyandastrophysics,2014,14:456
[5]  leeysetal.theastronomicaljournal,2008,136:2022
[6]  leeysetal.theastronomicaljournal,2008,136:2050
[7]  wuyetal.researchinastronomyandastrophysics,2011,11:924
[8]  xiangmsetal.monthlynoticesoftheroyalastronomicalsociety,2015,448:822
[9]  chenbqetal.monthlynoticesoftheroyalastronomicalsociety,2014,443:1192
[10]  yuanhbetal.researchinastronomyandastrophysics,2010,10:599
[11]  huozyetal.researchinastronomyandastrophysics,2010,10:612
[12]  wuxbetal.researchinastronomyandastrophysics,2010,10:737
[13]  wuxbetal.researchinastronomyandastrophysics,2010,10:745
[14]  lihnetal.researchinastronomyandastrophysics,2010,10:753
[15]  zhaojketal.theastronomicaljournal,2013,145:169
[16]  zhangyyetal.theastronomicaljournal,2013,146:34
[17]  renjjetal.astronomyandastrophysics,2014,570:a107
[18]  zhengzetal.theastrophysicaljournalletters,2014,785:l23
[19]  zhongjetal.theastrophysicaljournalletters,2014,789:l2
[20]  zhaojketal.theastrophysicaljournal,2014,787:31
[21]  huozyetal.theastronomicaljournal,2013,145:159
[22]  dehnenw,binneyj.monthlynoticesoftheroyalastronomicalsociety,1998,298:387
[23]  huangyetal.monthlynoticesoftheroyalastronomicalsociety,2015,449:162
[24]  quillenacetal.monthlynoticesoftheroyalastronomicalsociety,2011,417:762
[25]  carlinjetal.theastrophysicaljournalletters,2013,777:l5(erratum:apjl,2014,784:l46)
[26]  rebassa-mansergasaetal.monthlynoticesoftheroyalastronomicalsociety,2014,submitted
[27]  ibataretal.theastrophysicaljournal,2007,671:1591
[28]  huoetal.2014,inpreparation
[29]  chenbqetal.monthlynoticesoftheroyalastronomicalsociety,2015,448:2187
[30]  huangyetal.monthlynoticesoftheroyalastronomicalsociety,2014,439:2927
[31]  str?mbergg.theastrophysicaljournal,1946,104:12
[32]  sch?nrichr,binneyj.monthlynoticesoftheroyalastronomicalsociety,2012,419:1546
[33]  widrowlmetal.theastrophysicaljournalletters,2012,750:l41
[34]  williamsmeketal.monthlynoticesoftheroyalastronomicalsociety,2013,436:101
[35]  mcconnachieawetal.monthlynoticesoftheroyalastronomicalsociety,2005,356:979
[36]  steinmetzmetal.theastronomicaljournal,2006,132:1645
[37]  allendeprietocetal.astronomischenachrichten,2008,329:1018
[38]  freemankc.galacticarchaeology:near-fieldcosmologyandtheformationofthemilkyway.in:aokiw,ishigakim,sudatetal.eds,proc.aspconference(vol.458).sanfrancisco,ca:astronomicalsocietyofthepacific,2012,393
[39]  perrymanmacetal.astronomyandastrophysics,2001,369:339
[40]  cuixqetal.researchinastronomyandastrophysics,2012,12:1197
[41]  zhaogetal.researchinastronomyandastrophysics,2012,12:723
[42]  denglcetal.researchinastronomyandastrophysics,2012,12:735
[43]  liuxwetal.settingthesceneforgaiaandlamost.in:feltzings,zhaog,waltonnetal.eds,proc.iausymp.298.cambridgeuniversitypress,2014.310—321,preprint(arxiv:1306.5376)
[44]  yuanhbetal.monthlynoticesoftheroyalastronomicalsociety,2015,448:855
[45]  zhanghhetal.researchinastronomyandastrophysics,2013,13:490
[46]  baizretal.researchinastronomyandastrophysics,inpreparation
[47]  schlegeldj,finkbeinerdp,davism.theastrophysicaljournal,1998,500:525
[48]  yuanhb,liuxw,xiangms.monthlynoticesoftheroyalastronomicalsociety,2013,430:2188
[49]  mcconnachieawetal.nature,2009,461:66

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