Matches in SemOpenAlex for { <https://semopenalex.org/work/W2048760185> ?p ?o ?g. }
- W2048760185 endingPage "1007" @default.
- W2048760185 startingPage "998" @default.
- W2048760185 abstract "Using a sample of 21 damped Lyman alpha systems (DLAs) and 35 sub-DLAs, we evaluate the D-index from high-resolution spectra of the Mg iiλ 2796 profile. This sample represents an increase in the sub-DLA statistics by a factor of 4 over the original D-index sample. We investigate various techniques to define the velocity spread (Δv) of the Mg ii line to determine an optimal D-index for the identification of DLAs. The success rate of DLA identification is 50–55 per cent, depending on the velocity limits used, improving by a few per cent when the column density of Fe ii is included in the D-index calculation. We recommend the set of parameters that are judged to be most robust, have a combination of high DLA identification rate (57 per cent) and low DLA miss rate (6 per cent) and most cleanly separate the DLAs and sub-DLAs (Kolmogorov–Smirnov probability 0.5 per cent). These statistics demonstrate that the D-index is the most efficient technique for selecting low-redshift DLA candidates: 65 per cent more efficient than selecting DLAs based on the equivalent widths of Mg ii and Fe ii alone. We also investigate the effect of resolution on determining the N(H i) of sub-DLAs. We convolve echelle spectra of sub-DLA Lyα profiles with Gaussians typical of the spectral resolution of instruments on the Hubble Space Telescope and compare the best-fitting N(H i) values at both the resolutions. We find that the fitted H i column density is systematically overestimated by ∼0.1 dex in the moderate-resolution spectra compared to the best fits to the original echelle spectra. This offset is due to blending of nearby Lyα clouds that are included in the damping wing fit at low resolution." @default.
- W2048760185 created "2016-06-24" @default.
- W2048760185 creator A5042374450 @default.
- W2048760185 creator A5051029980 @default.
- W2048760185 creator A5090814337 @default.
- W2048760185 date "2009-01-21" @default.
- W2048760185 modified "2023-09-23" @default.
- W2048760185 title "The kinematic signature of damped Lyman alpha systems: using theD-index to screen for high column density H i absorbers★" @default.
- W2048760185 cites W1497431922 @default.
- W2048760185 cites W1601620636 @default.
- W2048760185 cites W1649074782 @default.
- W2048760185 cites W1731370316 @default.
- W2048760185 cites W1749304276 @default.
- W2048760185 cites W1965038204 @default.
- W2048760185 cites W1971343676 @default.
- W2048760185 cites W1975202273 @default.
- W2048760185 cites W1975838751 @default.
- W2048760185 cites W1979711374 @default.
- W2048760185 cites W1979736849 @default.
- W2048760185 cites W1985054304 @default.
- W2048760185 cites W1986843949 @default.
- W2048760185 cites W1997395325 @default.
- W2048760185 cites W2008724305 @default.
- W2048760185 cites W2016169001 @default.
- W2048760185 cites W2017270781 @default.
- W2048760185 cites W2022920666 @default.
- W2048760185 cites W2038727728 @default.
- W2048760185 cites W2054131667 @default.
- W2048760185 cites W2054994303 @default.
- W2048760185 cites W2057582805 @default.
- W2048760185 cites W2064913047 @default.
- W2048760185 cites W2066043890 @default.
- W2048760185 cites W2066245072 @default.
- W2048760185 cites W2071186164 @default.
- W2048760185 cites W2072070020 @default.
- W2048760185 cites W2072709509 @default.
- W2048760185 cites W2089728050 @default.
- W2048760185 cites W2090894327 @default.
- W2048760185 cites W2099174109 @default.
- W2048760185 cites W2100461368 @default.
- W2048760185 cites W2103896241 @default.
- W2048760185 cites W2106243200 @default.
- W2048760185 cites W2121083155 @default.
- W2048760185 cites W2123197592 @default.
- W2048760185 cites W2134203113 @default.
- W2048760185 cites W2153198268 @default.
- W2048760185 cites W2157603621 @default.
- W2048760185 cites W2159264410 @default.
- W2048760185 cites W2164096156 @default.
- W2048760185 cites W2215615628 @default.
- W2048760185 cites W3098072422 @default.
- W2048760185 cites W3098576613 @default.
- W2048760185 cites W3098680034 @default.
- W2048760185 cites W3098733230 @default.
- W2048760185 cites W3100112514 @default.
- W2048760185 cites W3100457327 @default.
- W2048760185 cites W3103241106 @default.
- W2048760185 cites W3105376551 @default.
- W2048760185 cites W3105753195 @default.
- W2048760185 cites W3106102484 @default.
- W2048760185 cites W3122107026 @default.
- W2048760185 cites W3123692920 @default.
- W2048760185 cites W3124412437 @default.
- W2048760185 cites W4292508449 @default.
- W2048760185 cites W4300576734 @default.
- W2048760185 cites W4302346839 @default.
- W2048760185 doi "https://doi.org/10.1111/j.1365-2966.2008.14131.x" @default.
- W2048760185 hasPublicationYear "2009" @default.
- W2048760185 type Work @default.
- W2048760185 sameAs 2048760185 @default.
- W2048760185 citedByCount "15" @default.
- W2048760185 countsByYear W20487601852012 @default.
- W2048760185 countsByYear W20487601852015 @default.
- W2048760185 countsByYear W20487601852016 @default.
- W2048760185 countsByYear W20487601852020 @default.
- W2048760185 countsByYear W20487601852023 @default.
- W2048760185 crossrefType "journal-article" @default.
- W2048760185 hasAuthorship W2048760185A5042374450 @default.
- W2048760185 hasAuthorship W2048760185A5051029980 @default.
- W2048760185 hasAuthorship W2048760185A5090814337 @default.
- W2048760185 hasBestOaLocation W20487601851 @default.
- W2048760185 hasConcept C105795698 @default.
- W2048760185 hasConcept C121332964 @default.
- W2048760185 hasConcept C13355873 @default.
- W2048760185 hasConcept C136764020 @default.
- W2048760185 hasConcept C171606756 @default.
- W2048760185 hasConcept C2524010 @default.
- W2048760185 hasConcept C2777382242 @default.
- W2048760185 hasConcept C2779696439 @default.
- W2048760185 hasConcept C2780551164 @default.
- W2048760185 hasConcept C33923547 @default.
- W2048760185 hasConcept C39920418 @default.
- W2048760185 hasConcept C41008148 @default.
- W2048760185 hasConcept C44870925 @default.
- W2048760185 hasConcept C49453240 @default.
- W2048760185 hasConcept C64943373 @default.
- W2048760185 hasConcept C74650414 @default.
- W2048760185 hasConceptScore W2048760185C105795698 @default.