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| group = [[Sao (moon)|Sao]] group ...in their search, which included [[Halimede (moon)|Halimede]], [[Sao (moon)|Sao]], [[Laomedeia (moon)|Laomedeia]], and [[Neso (moon)|Neso]].<ref name="Holm ...

| group = [[Neso (moon)|Neso]] group ...elative sizes of moons are indicated by the size of their symbols, and the Sao and Neso groups of Neptunian moons are labeled. Data as of February 2024.]] ...

...]&nbsp;75264, [[Bright Star Catalogue|HR]]&nbsp;5708, [[Star catalogue#SAO|SAO]]&nbsp;225712 .<ref name=SIMBAD/> ...is a probable member of the [[Scorpius–Centaurus association]], a [[moving group]] of stars that originated together and share a similar trajectory through ...

...> on this [https://djm.cc/constellation.html website].|name=Constellation|group=note}} |names={{odlist|HD=54475|HIP=34339|HR=2691|CD=-40 2930|SAO=218465|TIC=157533670|TYC=7633-2698-1|WISE=J070707.07-405335.6}}}} ...

...anyi | F=7 Dra | BD=+67°764 | FK5=3020 | HD=111335 | HIP=62423 | HR=4863 | SAO=15902 }}<ref name=SIMBAD/> ...Astronomical Union]] organized a [[IAU Working Group on Star Names|Working Group on Star Names]] (WGSN)<ref name=WGSN/> to catalogue and standardize proper ...

...Catalogue|HR]] 2930, [[Smithsonian Astrophysical Observatory Star Catalog|SAO]] 60247.<ref name=SIMBAD/> ....iau.org/science/scientific_bodies/working_groups/280/ | title=IAU Working Group on Star Names (WGSN)|access-date=22 May 2016}}</ref> to catalog and standar ...

| class = F9.5IV<ref name="Teff"/><ref name="HR"/><ref group="note">Despite the luminosity class of IV indicating a subgiant, the star l | b-v = 0.652 ± 0.002<ref name="van Leeuwen2007"/><ref group="note">Reddening = 0.077 (Casagrande et al. 2011)</ref><ref name="Casagrand ...

|absmag_v = −1.57<ref name = absmagv group=note/> |names = {{odlist|HIP =104357|HR = 8090|SAO = 126566|BD = +06°4754|AG = +06°2888|GC = 29548|HD = 201298|Gould = 12 G. E ...

| axis_unitless = 6.9 [[arc-second|mas]]<ref group=note>This is the photocentric semi-major axis, from the motion shown by the ...| F=17&nbsp;Orionis | BD=+02°&nbsp;888 | HD=33856 | HIP=24331 | HR=1698 | SAO=112528 }} ...

...sp;Cygni | BD=+53°&nbsp;2216 | FK5=726 | HD=181276 | HIP=94779 | HR=7328 | SAO=31537 }}, Angie C.G (Star registration) ...High-resolution spectroscopic study of red clump stars in the Galaxy: iron-group elements | journal=Monthly Notices of the Royal Astronomical Society | volu ...

{{Short description|Tokamak at the University of Sao Paulo, Brazil}} ...st3=Iberê Luiz |date=6 June 2022 |title=Website of the Oscillation Control Group |url=http://web.if.usp.br/controle/ }}</ref> ...

...Draper catalogue|HD]]&nbsp;98712, [[Smithsonian Astrophysical Observatory|SAO]]&nbsp;179801, [[Hipparcos catalogue|HIP]]&nbsp;55454 The SZ Crateris system is a member of the [[Ursa Major moving group]] of stars that have similar motions through space.<ref name=pasp118/> The ...

.../> on this [https://djm.cc/constellation.html website].|name=Constellation|group=note}} ...tions in the K band, which isn't is the best band to derive a metallicity.|group=note}} ...

| class = G1V-IV<ref group="note" name="SpecClass"/> | absmag_v = 3.610 ± 0.039<ref group="note" name="AbsMag"/> ...

...st4=Huang|first4=K.|date=2015|title=Paleomagnetism of Miocene volcanics on Sao Tome: Paleosecular variation at the Equator and a comparison to its latitud ...y fields from 150 Ma to present in 10 Ma increments |publisher=Geodynamics group at the [[Norwegian Geological Survey|Geological Survey of Norway]] |url-sta ...

[[File:Panorama Usina Costa Pinto Piracicaba SAO 10 2008.jpg|thumb|The Costa Pinto Production Plant in Piracicaba, Brazil. P ...e directly related to [[cancer]]s in the human body. One such example is a group that collected breath samples from a [[lung cancer]] patient to determine t ...

...Dubai London Madrid Milan Munich Paris Montreal Toronto Delhi Mexico City Sao Paulo Sydney Hong Kong Seoul Singapore Taipei Tokyo |isbn=978-0-13-604259-4 ...hmic bias|bias]] from a partially [[representative sample|representative]] group of annotators.<ref name="instructgptpaper"/> ...

...f Keynesians were critical of this synthesis interpretation of Keynes. One group focused on the disequilibrium aspects of Keynes's work, while the other too ...djust to changes in supply and demand.{{sfn|Skidelsky|2009|p=104}} Another group of Keynesians focused on disequilibrium economics and tried to reconcile th ...

...Neptune Barycenter" and "Center: Solar System Barycenter (@0)".)</ref><ref group=lower-alpha name=barycentre>Orbital elements refer to the Neptune barycentr ...24622|19|u=km}}}}<ref name="Seidelmann Archinal A'hearn et al. 2007"/><ref group=lower-alpha name=1bar/> ...

...had been detected, principally in Bristol, but with a genomically distinct group in Liverpool also carrying the mutation.<ref>{{cite web | title= Mutant Cov ...of <small><math>1.74^{14/6.5}=3.3</math></small> every two weeks. Another group came to similar conclusions, generating a replicative advantage, independen ...