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| ???org.dspace.app.webui.jsptag.ItemTag.dcfield??? | Value | Language |
|---|---|---|
| dc.contributor.advisor | 闕志鴻 | |
| dc.contributor.author | Yu-Ting Hsieh | en |
| dc.contributor.author | 謝侑廷 | zh_TW |
| dc.date.accessioned | 2021-06-08T00:43:18Z | - |
| dc.date.copyright | 2015-08-16 | |
| dc.date.issued | 2015 | |
| dc.date.submitted | 2015-08-13 | |
| dc.identifier.citation | [1] Gordon T. Richards, Xiaohui Fan, Heidi Jo Newberg, et al., Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample. 2002, arXiv:astro-ph/0202251 .
[2] John N. Bahcall, Sofia Kirhakos, David H. Saxe, Donald P. Schneider, Hubble Space Telescope Images of a Sample of Twenty Nearby Luminous Quasars. 1997, arXiv:astro-ph/9611163 . [3] Kasper B. Schmidt, Philip J. Marshall, Hans-Walter Rix, Sebastian Jester, Joseph F. Hennawi, Gregory Dobler, Selecting Quasars by their Intrinsic Variability. 2010, arXiv:1002.2642 [astro-ph.CO] . [4] Paul J. Francis, Eric J. Hooper, Chris D. Impey, The Ultraviolet Spectra of Radio-Loud And Radio-Quiet Quasars. 1993, AJ, 106, 417 . [5] Daniel E. Vanden Berk, Gordon T. Richards, Amanda Bauer, et al., Composite Quasar Spectra from the Sloan Digital Sky Survey. 2001 AJ, 122, 549 . [6] Donald P. Schneider, Gordon T. Richards, Patrick B. Hall, et al., The Sloan Digital Sky Survey Quasar Catalog V. Seventh Data Release. 2010, arXiv:1004.1167v1 [astro-ph.CO] . [7] Isabelle Paris, Patrick Petitjean, Eric Aubourg, et al., The Sloan Digital Sky Survey Quasar Catalog: Tenth Data Release. 2013, arXiv:1311.4870v1 [astro-ph.CO] . [8] E. A. Magnier, E. Schlafly, D. Finkbeiner, et al., The Pan-STARRS 1 Photometric Reference Ladder, Release 12.0. 2013, arXive:1303.3634v1 [astro-ph.IM] . [9] Kaiser N., in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. 2002 . [10] Kimberly M. Aller, Adam L. Kraus, Michael C. Liu, et al., A Pan-STARRS + UKIDSS Search for Yong, Wide Planetary-Mass Comparison in Upper Scorpius. 2013, arXiv:1307.0506 [astro-ph.SR] . [11] Heidi J. Newberg, Brian Yanny, Three-dimensional parameterization of the stellar locus with application to QSO color selection. 1997, Astrophys.J.Suppl. 113 (1997) 89 . [12] Željko Ivezić, J. Allyn Smith, Gajus Miknaitis, Sloan Digital Sky Survey Standard Star Catalog for Stripe 82: The Dawn of Industrial 1% Optical Photometry. 2007, AJ 134,973 . [13] Branimir Sesar, Željko Ivezić, Robert H. Lupton, Exploring the Variable Sky with the Sloan Digital Sky Survey. 2007, AJ 134:2236-2251 . [14] Daniel J. Eisenstein, James Liebert, Hugh C. Harris, A Catalog of Spectroscopic-ally Confirmed White Dwarfs from the Sloan Digital Sky Survey Data Release 4. 2006, arXiv:astro-ph/0606700v1 . [15] A. Misiriotis, E. M. Xilouris, J. Papamastorakis, P. Boumis, C. D. Goudis, The distribution of the ISM in the Milky Way. A three-dimensional large-scale model. 2006, arXiv:astro-ph/0607638v1 . [16] Vernesa Smolčić, Željko Ivezić, Gillian R. Knapp, A Second Stellar Color Locus: a Bridge from White Dwarfs to M stars. 2004, ApJ 615L141 . | |
| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/17772 | - |
| dc.description.abstract | 在這篇論文中，我們主要介紹一個在三維雙色圖中能夠區分一般星星與類星體之數值演算模型，並利用此模型來搜尋類星體候選者。這個方法對於類星體的強烈藍光輻射非常地敏感，因此藉由多波段觀測的方法，再利用類星體有別於一般星星的光度顏色之特性，我們可以有效地從一堆未知的星星挑選出類星體候選者。本文利用 Sloan Digital Sky Survey (SDSS) 的 Stripe 82 星場之資料庫作為本研究的測試基底，並且測試出的類星體候選者之篩選純度為 51.1%。本文同時也探討了不同類型的星星對在三維雙色圖中污染類星體的情形，並藉此提昇篩選純度至 58.1%。此外本文也會呈現我們的篩選純度與Richard 2002的研究兩者之間的差異。最後，我們將此研究方法應用於Pan-STARRS survey的四分之三天區的觀測資料，並使用了g, r, i, z 來搜尋類星體候選者。 | zh_TW |
| dc.description.abstract | This work describes the algorithm for distinguishing quasars from stars in 3D color-color space. This method is sensitive to blue emission of quasars, and we can identify the quasar candidates from unsolved targets via their non-stellar photometric colors in several bands. We use the Stripe 82 Catalog of Sloan Digital Sky Survey (SDSS) in a field of 286〖deg〗^2 as a trial set with a purity of 51.1%. We also discuss the contaminations of quasars from other different kinds of objects to improve the purity of quasar selection to 58.1% and compare our purity with previous work (Richards et al. 2002) [1]. Finally, we employ this method to the 3pi-sky data of Pan-STARRS survey (with g, r, i, z bands) to search for quasar candidates. | en |
| dc.description.provenance | Made available in DSpace on 2021-06-08T00:43:18Z (GMT). No. of bitstreams: 1 ntu-104-R00244004-1.pdf: 12631927 bytes, checksum: d00acd7a917e396237ec4d67c5ea3ecc (MD5) Previous issue date: 2015 | en |
| dc.description.tableofcontents | 口試委員審定書...i
誌謝...ii 摘要...iii Abstract...iv Contents...v List of Figures...vii List of Tables...xi 1 Introduction...1 2 Pan-STASSRS 1...4 2.1 The Pan-STARRS 1 3π Data...4 2.2 DVO Database and Extract Data...5 3 Quasar Candidate Selection Algorithm...8 3.1 Determine Data sets of Stellar Locus...10 3.2 Parameterization of the Stellar Locus...11 3.2.1 Destination of the Algorithm...11 3.2.2 Input Parameters...14 3.2.3 Fit Stellar Locus...15 3.3 Summery...20 4 Application of The Algorithm...23 4.1 Outlier Selection of Valid Quasars...23 4.2 Result...25 5 Discussion...28 5.1 Contaminations...28 5.1.1 Variable Stars...28 5.1.2 Valid White Dwarfs and WD+M Binaries...29 5.1.3 Result...32 5.2 U-Band Detection...32 5.3 Stellar Locus Data Checks...35 6 Quasar Candidates Searching on The PS1 3π Data...37 6.1 Milky Way Objects Rejecting...37 6.2 Result...38 7 Conclusion...40 7.1 Summary...40 7.2 Future Prospects...41 Bibliography...42 | |
| dc.language.iso | en | |
| dc.title | 多波段三維雙色圖之數值模型篩選類星體候選者之應用 | zh_TW |
| dc.title | The Selection of Quasar Candidates Using Three Dimensional Color-Color Diagram | en |
| dc.type | Thesis | |
| dc.date.schoolyear | 103-2 | |
| dc.description.degree | 碩士 | |
| dc.contributor.oralexamcommittee | 陳文屏,林俐暉,蘇游瑄 | |
| dc.subject.keyword | 類星體,三維雙色圖,史隆巡天計畫,泛星巡天計畫,多波段觀測, | zh_TW |
| dc.subject.keyword | Quasar,3D Color-Color Diagram,SDSS,Pan-STARRS,Multi-Waveband, | en |
| dc.relation.page | 43 | |
| dc.rights.note | 未授權 | |
| dc.date.accepted | 2015-08-13 | |
| dc.contributor.author-college | 理學院 | zh_TW |
| dc.contributor.author-dept | 天文物理研究所 | zh_TW |
| Appears in Collections: | 天文物理研究所 | |
Files in This Item:
| File | Size | Format | |
|---|---|---|---|
| ntu-104-1.pdf Restricted Access | 12.34 MB | Adobe PDF |
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