FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2040547829> ?p ?o ?g. }

• W2040547829 endingPage "392" @default.
• W2040547829 startingPage "388" @default.
• W2040547829 abstract "Abstract The photometric and RV techniques, although extremely efficient to detect and characterize planets, are, however, indirect techniques (as well as astrometry). Phenomena such as stellar pulsation, inhomogeneous convection, spots or magnetic cycles can prevent us from finding planets or they might degrade the parameters estimation. We will consider the challenges related to the knowledge of stellar activity for the next decade: detect telluric planets in the habitable zone of their stars (from G to M dwarfs), understand the activity in the low-mass end of M dwarf (on which will focus future near-infrared high-resolution spectrograph like SPIRou or CARMENES), limitation to the process of summing several transit observations (in order to characterize the atmospheric components) due to the variability of stellar activity (from the ground or with Spitzer or JWST), as well as the methods proposed and used to overcome this issue." @default.
• W2040547829 created "2016-06-24" @default.
• W2040547829 creator A5024503764 @default.
• W2040547829 creator A5034701856 @default.
• W2040547829 creator A5043111265 @default.
• W2040547829 creator A5051639942 @default.
• W2040547829 creator A5066527569 @default.
• W2040547829 creator A5073332770 @default.
• W2040547829 creator A5084594696 @default.
• W2040547829 creator A5087327428 @default.
• W2040547829 date "2012-08-01" @default.
• W2040547829 modified "2023-09-25" @default.
• W2040547829 title "Stellar Variabilities: Challenges for the Detection and Characterization of Exoplanets" @default.
• W2040547829 cites W1981376873 @default.
• W2040547829 cites W1987581036 @default.
• W2040547829 cites W2004802635 @default.
• W2040547829 cites W2038895269 @default.
• W2040547829 cites W2047449019 @default.
• W2040547829 cites W2102955220 @default.
• W2040547829 cites W2104072923 @default.
• W2040547829 cites W2128521479 @default.
• W2040547829 cites W2133670009 @default.
• W2040547829 cites W2950992121 @default.
• W2040547829 cites W3100984160 @default.
• W2040547829 cites W3102541646 @default.
• W2040547829 cites W3105218762 @default.
• W2040547829 cites W4293676342 @default.
• W2040547829 doi "https://doi.org/10.1017/s1743921313013227" @default.
• W2040547829 hasPublicationYear "2012" @default.
• W2040547829 type Work @default.
• W2040547829 sameAs 2040547829 @default.
• W2040547829 citedByCount "0" @default.
• W2040547829 crossrefType "journal-article" @default.
• W2040547829 hasAuthorship W2040547829A5024503764 @default.
• W2040547829 hasAuthorship W2040547829A5034701856 @default.
• W2040547829 hasAuthorship W2040547829A5043111265 @default.
• W2040547829 hasAuthorship W2040547829A5051639942 @default.
• W2040547829 hasAuthorship W2040547829A5066527569 @default.
• W2040547829 hasAuthorship W2040547829A5073332770 @default.
• W2040547829 hasAuthorship W2040547829A5084594696 @default.
• W2040547829 hasAuthorship W2040547829A5087327428 @default.
• W2040547829 hasBestOaLocation W20405478291 @default.
• W2040547829 hasConcept C101638190 @default.
• W2040547829 hasConcept C110472602 @default.
• W2040547829 hasConcept C121332964 @default.
• W2040547829 hasConcept C1276947 @default.
• W2040547829 hasConcept C133725777 @default.
• W2040547829 hasConcept C150846664 @default.
• W2040547829 hasConcept C162053735 @default.
• W2040547829 hasConcept C163479331 @default.
• W2040547829 hasConcept C17744445 @default.
• W2040547829 hasConcept C180537121 @default.
• W2040547829 hasConcept C199539241 @default.
• W2040547829 hasConcept C2778022998 @default.
• W2040547829 hasConcept C2778861254 @default.
• W2040547829 hasConcept C44870925 @default.
• W2040547829 hasConcept C4839761 @default.
• W2040547829 hasConcept C51244244 @default.
• W2040547829 hasConcept C51553727 @default.
• W2040547829 hasConcept C539828613 @default.
• W2040547829 hasConcept C87355193 @default.
• W2040547829 hasConceptScore W2040547829C101638190 @default.
• W2040547829 hasConceptScore W2040547829C110472602 @default.
• W2040547829 hasConceptScore W2040547829C121332964 @default.
• W2040547829 hasConceptScore W2040547829C1276947 @default.
• W2040547829 hasConceptScore W2040547829C133725777 @default.
• W2040547829 hasConceptScore W2040547829C150846664 @default.
• W2040547829 hasConceptScore W2040547829C162053735 @default.
• W2040547829 hasConceptScore W2040547829C163479331 @default.
• W2040547829 hasConceptScore W2040547829C17744445 @default.
• W2040547829 hasConceptScore W2040547829C180537121 @default.
• W2040547829 hasConceptScore W2040547829C199539241 @default.
• W2040547829 hasConceptScore W2040547829C2778022998 @default.
• W2040547829 hasConceptScore W2040547829C2778861254 @default.
• W2040547829 hasConceptScore W2040547829C44870925 @default.
• W2040547829 hasConceptScore W2040547829C4839761 @default.
• W2040547829 hasConceptScore W2040547829C51244244 @default.
• W2040547829 hasConceptScore W2040547829C51553727 @default.
• W2040547829 hasConceptScore W2040547829C539828613 @default.
• W2040547829 hasConceptScore W2040547829C87355193 @default.
• W2040547829 hasIssue "S293" @default.
• W2040547829 hasLocation W20405478291 @default.
• W2040547829 hasLocation W20405478292 @default.
• W2040547829 hasLocation W20405478293 @default.
• W2040547829 hasOpenAccess W2040547829 @default.
• W2040547829 hasPrimaryLocation W20405478291 @default.
• W2040547829 hasRelatedWork W1977912629 @default.
• W2040547829 hasRelatedWork W2008781654 @default.
• W2040547829 hasRelatedWork W2040547829 @default.
• W2040547829 hasRelatedWork W2314552474 @default.
• W2040547829 hasRelatedWork W2592156984 @default.
• W2040547829 hasRelatedWork W2947270536 @default.
• W2040547829 hasRelatedWork W2963354934 @default.
• W2040547829 hasRelatedWork W2963813302 @default.
• W2040547829 hasRelatedWork W2999478132 @default.
• W2040547829 hasRelatedWork W3099977695 @default.
• W2040547829 hasVolume "8" @default.
• W2040547829 isParatext "false" @default.

• next