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^ a b c 輝星星表第5版
^ “ ⇒#12 HIP 7513”. TPF-C Top 100. 2006年7月5日閲覧。
^ Holmberg et al. (2007年). “Record 970”. Geneva-Copenhagen Survey of Solar neighbourhood. 2008年11月19日閲覧。
^ a b Buccino, A. et al. (2006). ⇒“Ultraviolet Radiation Constraints around the Circumstellar Habitable Zones”. Icarus 183 (2): 491?503. doi:10.1016/j.icarus.2006.03.007. ⇒http://adsabs.harvard.edu/abs/2005astro.ph.12291B
^ a b Lowrance, P. et al. (2002). “A Distant Stellar Companion in the υ Andromedae System”. The Astrophysical Journal Letters 572 (1): L79-L81. doi:10.1086/341554. https://ui.adsabs.harvard.edu/abs/2002ApJ...572L..79L/abstract. 
^ “ ⇒Washington Double Star Catalog”. United States Naval Observatory. 2017年5月19日閲覧。
^ Butler et al. (1997). ⇒“Three New 51 Pegasi-Type Planets”. The Astrophysical Journal Letters 474 (2): L115?L118. doi:10.1086/310444. ⇒http://www.iop.org/EJ/article/1538-4357/474/2/L115/5590.html
^ Shkolnik, E. et al. (2005). ⇒“Hot Jupiters and Hot Spots: The Short- and Long-term Chromospheric Activity on Stars with Giant Planets”. The Astrophysical Journal 622 (2): 1075?1090. doi:10.1086/428037. ⇒http://www.iop.org/EJ/article/0004-637X/622/2/1075/61179.html
^ Butler et al. (1999). ⇒“Evidence for Multiple Companions to υ Andromedae”. The Astrophysical Journal 526 (2): 916?927. doi:10.1086/308035. ⇒http://www.iop.org/EJ/article/0004-637X/526/2/916/40403.html
^ a b c d Butler, R. et al. (2006). ⇒“Catalog of Nearby Exoplanets”. The Astrophysical Journal 646 (1): 505?522. doi:10.1086/504701. ⇒http://www.iop.org/EJ/article/0004-637X/646/1/505/64046.html.  ( ⇒web version)
^ McArthur, B., Benedict, G. F., Bean, J., & Martioli, E. (2007). “Planet Masses in the Upsilon Andromadae system determined with the HST Fine Guidance Sensors”. American Astronomical Society Meeting Abstracts 211. 
^ Han, I. et al. (2001). ⇒“Preliminary Astrometric Masses for Proposed Extrasolar Planetary Companions”. The Astrophysical Journal Letters 548: L57-L60. doi:10.1086/318927. ⇒http://www.iop.org/EJ/article/1538-4357/548/1/L57/005774.html
^ Pourbaix, D. and Arenou, F. (2001). “Screening the Hipparcos-based astrometric orbits of sub-stellar objects”. Astronomy and Astrophysics 372: 935?944. doi:10.1051/0004-6361:20010597. https://ui.adsabs.harvard.edu/abs/2001A%26A...372..935P/abstract. 
^ Benedict, George F.; McArthur, B. E.; Bean, J. L. (2007). “The υ Andromedae Planetary System - Hubble Space Telescope Astrometry and High-precision Radial Velocities”. Bulletin of the American Astronomical Society 38: 185.  Announced American Astronomical Society Meeting 210, #78.02
^ Lissauer, J., Rivera, E. (2001). ⇒“Stability analysis of the planetary system orbiting υ Andromedae. II. Simulations using new Lick observatory fits”. The Astrophysical Journal 554: 1141?1150. doi:10.1086/321426. ⇒http://simbad.u-strasbg.fr/cgi-bin/cdsbib?2001ApJ...554.1141L
^ Ford, E. et al. (2005). ⇒“Planet-planet scattering in the upsilon Andromedae system”. Nature 434: 873?876. doi:10.1038/nature03427. ⇒http://simbad.u-strasbg.fr/cgi-bin/cdsbib?2005Natur.434..873F
^ .mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation.cs-ja1 q,.mw-parser-output .citation.cs-ja2 q{quotes:"「""」""『""』"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free a,.mw-parser-output .citation .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited a,.mw-parser-output .id-lock-registration a,.mw-parser-output .citation .cs1-lock-limited a,.mw-parser-output .citation .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription a,.mw-parser-output .citation .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:#d33}.mw-parser-output .cs1-visible-error{color:#d33}.mw-parser-output .cs1-maint{display:none;color:#3a3;margin-left:0.3em}.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit}Rory Barnes; Richard Greenberg (2008). "Extrasolar Planet Interactions". arXiv:0801.3226v1 [astro-ph]。
^ Trilling, D. et al. (2000). ⇒“Circumstellar dust disks around stars with known planetary companions”. The Astrophysical Journal 529: 499?505. doi:10.1086/308280. ⇒http://simbad.u-strasbg.fr/cgi-bin/cdsbib?2000ApJ...529..499T
^ Curiel, S.; Canto, J.; Georgiev, L.; Chavez, C. E.; Poveda, A. (2011). ⇒“A fourth planet orbiting υ Andromedae”. Astronomy & Astrophysics 525: A78. Bibcode: 2011A&A...525A..78C. doi:10.1051/0004-6361/201015693. ⇒http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/abs/2011/01/aa15693-10/aa15693-10.html
^ a b c d e f g h i j Ligi, R.; Mourard, D.; Lagrange, A.M.; Perraut, K.; Boyajian, T.; Berio, Ph.; Nardetto, N.; TallonBosc, I. et al. (2012). ⇒“A new interferometric study of four exoplanet host stars : θ Cygni, 14 Andromedae, υ Andromedae and 42 Draconis”. Astronomy & Astrophysics 545: A5. arXiv:1208.3895. Bibcode: 2012A&A...545A...5L. doi:10.1051/0004-6361/201219467. ⇒http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201219467&Itemid=129

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