About: Using red clump stars to correct the Gaia DR1 parallaxes

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scientific article published in Astronomy and Astrophysics

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в січні 2017 (uk) article publié dans la revue scientifique Astronomy and Astrophysics (fr) im Januar 2017 veröffentlichter wissenschaftlicher Artikel (de) scientific article published in Astronomy and Astrophysics (en)
publication date	wds:Q58263145-098E2C28-653A-474B-B2B2-9587296762A3
publication date	2017-01-26 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58263145-AB2226E9-4AA8-4688-AEC7-8CAB904D8C40
language of work or name	English
cites work	wds:Q58263145-1BB49DF4-F469-448E-A443-11C562C878C7 wds:Q58263145-3FA13B9A-45F0-4DE4-A994-832DEA519E2B wds:Q58263145-5B7C2524-BAC8-4917-BA64-CA8B4AA1B465 wds:Q58263145-8C46BD27-2C7F-42C5-BF02-65564A3C062C wds:Q58263145-93A10F8A-7384-4502-A1A1-F4FEE8AFF3C5 wds:Q58263145-9C0D5BD3-45EF-4550-BE82-90BC44EFD167 wds:Q58263145-A1EF07A2-BEE0-404A-AB63-05C90985BAEF wds:Q58263145-BF7CC59A-8843-4E77-A8C2-388AA3AC06FB wds:Q58263145-D882ED08-5FBF-4672-8619-61462231153F wds:Q58263145-DCB05234-1A9A-419B-AEF7-7CB1E7086E36 wds:Q58263145-DD528341-FDA5-4DF3-BF6C-9F2BB9750047 wds:Q58263145-DF0E64E2-17B4-4287-93F3-BB1FBA10FB6E wds:Q58263145-E50C3016-95B0-4F4D-B362-DE6AE542D725
cites work	The Two Micron All Sky Survey (2MASS) Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties The relationship between infrared, optical, and ultraviolet extinction Star counts in the Galaxy. Simulating from very deep to very shallow photometric surveys with the TRILEGAL code Galactic archaeology: mapping and dating stellar populations with asteroseismology of red-giant stars The APOKASC catalog: an asteroseismic and spectroscopic joint survey of targets in the Kepler fields Bayesian distances and extinctions for giants observed by Kepler and APOGEE The K2 M67 study: revisiting old friends with K2 reveals oscillating red giants in the open cluster M67 Population effects on the red giant clump absolute magnitude: theKband Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars TheTycho-Gaiaastrometric solution Gaia data release 1. Astrometry: one billion positions, two million proper motions, and parallaxes Prospects for detecting asteroseismic binaries in Kepler data
author name string	wds:Q58263145-08313F4E-8C63-4BA1-A78F-D9B8EA6C4034 wds:Q58263145-0A702BFE-1A8D-4751-9B82-AAE1B4048E3B wds:Q58263145-1966D9E3-F815-45A7-92E5-9FC39A91F404 wds:Q58263145-3AD0CB73-CAE4-47A5-9221-2F1EFD29B099 wds:Q58263145-3BD35938-4D54-40E4-AA8B-D84121E4522E wds:Q58263145-62C0ACC5-CA11-4A52-8E43-32940C1F0BC0 wds:Q58263145-A542ADC8-96D6-454A-9023-76957C8EF751 wds:Q58263145-C188B305-D148-4ABF-9A88-4E52C85B89DB wds:Q58263145-EEC689B7-FF97-4F16-9505-EEDDBB51F58B
author name string	Léo Girardi Caitlin D. Jones Guy R. Davies Mathew Schofield Thaíse S. Rodrigues Steven D. Kawaler Thomas S. H. North James S. Kuszlewicz Steven J. Hale
rdfs:label	Using red clump stars to correct the Gaia DR1 parallaxes (en) Using red clump stars to correct theGaiaDR1 parallaxes (nl)
skos:prefLabel	Using red clump stars to correct the Gaia DR1 parallaxes (en) Using red clump stars to correct theGaiaDR1 parallaxes (nl)
name	Using red clump stars to correct the Gaia DR1 parallaxes (en) Using red clump stars to correct theGaiaDR1 parallaxes (nl)
author	wds:Q58263145-48011932-3C80-432F-8CBD-29508DE57A64 wds:Q58263145-67E1F755-A037-4160-B2EE-AE55753D671C wds:Q58263145-74CD9397-0D06-47C6-9899-2B0EF5F78868 wds:Q58263145-C176D80E-14DC-4583-9387-A428928DEBB8 wds:Q58263145-C335AFAE-E8DD-44B3-93E2-C340A92F4724 wds:Q58263145-C37F820C-B3ED-4F64-94E4-A82AB24F0CE4 wds:Q58263145-D3EB12B8-6C2D-4CD4-AAFD-E1B3A1DB76E0 wds:Q58263145-EEEA620C-7386-4C4D-82FF-C3BEEDDF74A4 wds:Q58263145-F86688B8-60FE-4A78-A379-EF3593B1AA7C
author	Yvonne Elsworth Andrea Miglio Ian W. Roxburgh Mikkel N. Lund William J. Chaplin Tiago L. Campante Steven J Hale Ben Rendle Oliver Hall
title	wds:Q58263145-37890666-7CA2-46C3-823E-CC41780E81F0
title	Using red clump stars to correct the Gaia DR1 parallaxes (en)
page(s)	wds:Q58263145-87886375-2162-4A72-A8BE-2995C53DDCD8
page(s)	4–4
Internet Archive ID	wds:Q58263145-0C25DB13-0D1A-4A49-A5EB-7BEE9CB12697
Internet Archive ID	arxiv-1701.02506
instance of	wds:Q58263145-2C69FC33-CEFB-4A9A-83B4-11C96672C5DA
instance of	scholarly article
published in	wds:Q58263145-15F2F01E-F5B1-48B3-AF6F-06D5E87F0C13
published in	Astronomy and Astrophysics
volume	wds:Q58263145-BF207C49-5E5D-4C29-9A73-7006CA0DEDC8
volume	598
DOI	wds:Q58263145-4D5019F0-087F-4D33-91E6-EC3152A6A1DD
DOI	http://dx.doi.org/10.1051/0004-6361/201630066
DOI	10.1051/0004-6361/201630066
arXiv ID	wds:Q58263145-FF1A460B-65BA-4CB3-8825-4FA1E72ADB35
arXiv ID	1701.02506
ADS bibcode	wds:Q58263145-D337F0FD-2B9E-46BF-81A0-3EA76BD6CA09
ADS bibcode	2017A&A...598L...4D
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58263145
is cites work of	The masses of retired A stars with asteroseismology: Kepler and K2 observations of exoplanet hosts

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