Matches in SemOpenAlex for { <https://semopenalex.org/work/W2809778922> ?p ?o ?g. }
Showing items 1 to 90 of
90
with 100 items per page.
- W2809778922 endingPage "926" @default.
- W2809778922 startingPage "914" @default.
- W2809778922 abstract "Occulting galaxy pairs have been used to determine the transmission and dust composition within the foreground galaxy. Observations of the nearly face-on ring-like debris disk around the solar-like star HD 107146 by HST/ACS in 2004 and HST/STIS in 2011 reveal that the debris ring is occulting an extended background galaxy over the subsequent decades. Our aim is to use 2004 HST observations of this system to model the galaxy and apply this to the 2011 observation in order to measure the transmission of the galaxy through the outer regions of the debris disk. We model the galaxy with an exponential disk and a S'{e}rsic pseudo-bulge in the V- and I-band, but irregularities due to small scale structure from star forming regions limits accurate determination of the foreground dust distribution. We show that debris ring transit photometry is feasible for optical depth increases of $Delta tau geq$ 0.04 ($1 sigma$) on tens of au scales the width of the background galaxy { when the 2011 STIS data are compared directly with new HST/STIS observations, instead of the use of a smoothed model as a reference." @default.
- W2809778922 created "2018-07-10" @default.
- W2809778922 creator A5047758262 @default.
- W2809778922 creator A5058085373 @default.
- W2809778922 creator A5058865181 @default.
- W2809778922 creator A5069984909 @default.
- W2809778922 creator A5082710668 @default.
- W2809778922 date "2018-07-11" @default.
- W2809778922 modified "2023-09-27" @default.
- W2809778922 title "Feasibility of the debris ring transit method for the solar-like star HD 107146 by an occulted galaxy" @default.
- W2809778922 cites W2013554814 @default.
- W2809778922 cites W2031179275 @default.
- W2809778922 cites W2045051805 @default.
- W2809778922 cites W2079227246 @default.
- W2809778922 cites W2083224201 @default.
- W2809778922 cites W2106988651 @default.
- W2809778922 cites W2114083330 @default.
- W2809778922 cites W2114282862 @default.
- W2809778922 cites W2124786300 @default.
- W2809778922 cites W2133725650 @default.
- W2809778922 cites W2142238829 @default.
- W2809778922 cites W2146380835 @default.
- W2809778922 cites W2163480877 @default.
- W2809778922 cites W2410523940 @default.
- W2809778922 cites W3098811604 @default.
- W2809778922 cites W3099299678 @default.
- W2809778922 cites W3099553619 @default.
- W2809778922 cites W3100643694 @default.
- W2809778922 cites W3103589725 @default.
- W2809778922 cites W3103688679 @default.
- W2809778922 cites W3104225838 @default.
- W2809778922 cites W4301256944 @default.
- W2809778922 cites W46714404 @default.
- W2809778922 doi "https://doi.org/10.1093/mnras/sty1829" @default.
- W2809778922 hasPublicationYear "2018" @default.
- W2809778922 type Work @default.
- W2809778922 sameAs 2809778922 @default.
- W2809778922 citedByCount "0" @default.
- W2809778922 crossrefType "journal-article" @default.
- W2809778922 hasAuthorship W2809778922A5047758262 @default.
- W2809778922 hasAuthorship W2809778922A5058085373 @default.
- W2809778922 hasAuthorship W2809778922A5058865181 @default.
- W2809778922 hasAuthorship W2809778922A5069984909 @default.
- W2809778922 hasAuthorship W2809778922A5082710668 @default.
- W2809778922 hasBestOaLocation W28097789222 @default.
- W2809778922 hasConcept C100905312 @default.
- W2809778922 hasConcept C121332964 @default.
- W2809778922 hasConcept C1276947 @default.
- W2809778922 hasConcept C150846664 @default.
- W2809778922 hasConcept C153294291 @default.
- W2809778922 hasConcept C2776023875 @default.
- W2809778922 hasConcept C44870925 @default.
- W2809778922 hasConcept C68271606 @default.
- W2809778922 hasConcept C73411000 @default.
- W2809778922 hasConcept C98444146 @default.
- W2809778922 hasConceptScore W2809778922C100905312 @default.
- W2809778922 hasConceptScore W2809778922C121332964 @default.
- W2809778922 hasConceptScore W2809778922C1276947 @default.
- W2809778922 hasConceptScore W2809778922C150846664 @default.
- W2809778922 hasConceptScore W2809778922C153294291 @default.
- W2809778922 hasConceptScore W2809778922C2776023875 @default.
- W2809778922 hasConceptScore W2809778922C44870925 @default.
- W2809778922 hasConceptScore W2809778922C68271606 @default.
- W2809778922 hasConceptScore W2809778922C73411000 @default.
- W2809778922 hasConceptScore W2809778922C98444146 @default.
- W2809778922 hasIssue "1" @default.
- W2809778922 hasLocation W28097789221 @default.
- W2809778922 hasLocation W28097789222 @default.
- W2809778922 hasLocation W28097789223 @default.
- W2809778922 hasLocation W28097789224 @default.
- W2809778922 hasLocation W28097789225 @default.
- W2809778922 hasOpenAccess W2809778922 @default.
- W2809778922 hasPrimaryLocation W28097789221 @default.
- W2809778922 hasRelatedWork W1641631973 @default.
- W2809778922 hasRelatedWork W1690707023 @default.
- W2809778922 hasRelatedWork W2018460911 @default.
- W2809778922 hasRelatedWork W2073641674 @default.
- W2809778922 hasRelatedWork W2146469479 @default.
- W2809778922 hasRelatedWork W2342416117 @default.
- W2809778922 hasRelatedWork W3098997918 @default.
- W2809778922 hasRelatedWork W3102549633 @default.
- W2809778922 hasRelatedWork W3102710178 @default.
- W2809778922 hasRelatedWork W4308191026 @default.
- W2809778922 hasVolume "480" @default.
- W2809778922 isParatext "false" @default.
- W2809778922 isRetracted "false" @default.
- W2809778922 magId "2809778922" @default.
- W2809778922 workType "article" @default.