FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2185979087> ?p ?o ?g. }

• W2185979087 endingPage "121" @default.
• W2185979087 startingPage "121" @default.
• W2185979087 abstract "The WFC3 Infrared Spectroscopic Parallel Survey (WISP) uses the Hubble Space Telescope (HST) infrared grism capabilities to obtain slitless spectra of thousands of galaxies over a wide redshift range including the peak of star formation history of the Universe. We select a population of very strong emission-line galaxies with rest-frame equivalent widths higher than 200 A. A total of 176 objects are found over the redshift range 0.35 < z < 2.3 in the 180 arcmin^2 area we analyzed so far. After estimating the AGN fraction in the sample, we show that this population consists of young and low-mass starbursts with higher specific star formation rates than normal star-forming galaxies at any redshift. After spectroscopic follow-up of one of these galaxies with Keck/LRIS, we report the detection at z = 0.7 of an extremely metal-poor galaxy with 12+Log(O/H)= 7.47 +- 0.11. The nebular emission-lines can substantially affect the broadband flux density with a median brightening of 0.3 mag, with examples producing brightening of up to 1 mag. The presence of strong emission lines in low-z galaxies can mimic the color-selection criteria used in the z ~ 8 dropout surveys. In order to effectively remove low redshift interlopers, deep optical imaging is needed, at least 1 mag deeper than the bands in which the objects are detected. Finally, we empirically demonstrate that strong nebular lines can lead to an overestimation of the mass and the age of galaxies derived from fitting of their SED. Without removing emission lines, the age and the stellar mass estimates are overestimated by a factor of 2 on average and up to a factor of 10 for the high-EW galaxies. Therefore the contribution of emission lines should be systematically taken into account in SED fitting of star-forming galaxies at all redshifts." @default.
• W2185979087 created "2016-06-24" @default.
• W2185979087 creator A5005327872 @default.
• W2185979087 creator A5023602707 @default.
• W2185979087 creator A5023653646 @default.
• W2185979087 creator A5026363701 @default.
• W2185979087 creator A5029531883 @default.
• W2185979087 creator A5031916357 @default.
• W2185979087 creator A5050987956 @default.
• W2185979087 creator A5054403413 @default.
• W2185979087 creator A5056953216 @default.
• W2185979087 creator A5068853533 @default.
• W2185979087 creator A5069632551 @default.
• W2185979087 creator A5077019414 @default.
• W2185979087 creator A5078931158 @default.
• W2185979087 creator A5080825960 @default.
• W2185979087 creator A5084601892 @default.
• W2185979087 creator A5087399697 @default.
• W2185979087 date "2011-11-29" @default.
• W2185979087 modified "2023-10-02" @default.
• W2185979087 title "VERY STRONG EMISSION-LINE GALAXIES IN THE WFC3 INFRARED SPECTROSCOPIC PARALLEL SURVEY AND IMPLICATIONS FOR HIGH-REDSHIFT GALAXIES^," @default.
• W2185979087 cites W1603995462 @default.
• W2185979087 cites W1622230873 @default.
• W2185979087 cites W1921696651 @default.
• W2185979087 cites W1966867730 @default.
• W2185979087 cites W1968595293 @default.
• W2185979087 cites W1968921050 @default.
• W2185979087 cites W1970660289 @default.
• W2185979087 cites W1972507852 @default.
• W2185979087 cites W1975080613 @default.
• W2185979087 cites W1977110390 @default.
• W2185979087 cites W1980904486 @default.
• W2185979087 cites W1981780603 @default.
• W2185979087 cites W1985952407 @default.
• W2185979087 cites W1993217083 @default.
• W2185979087 cites W1994671833 @default.
• W2185979087 cites W1994915027 @default.
• W2185979087 cites W1995619964 @default.
• W2185979087 cites W1997015919 @default.
• W2185979087 cites W2006316173 @default.
• W2185979087 cites W2008241787 @default.
• W2185979087 cites W2013575191 @default.
• W2185979087 cites W2013741966 @default.
• W2185979087 cites W2017980472 @default.
• W2185979087 cites W2018539983 @default.
• W2185979087 cites W2031942083 @default.
• W2185979087 cites W2036036577 @default.
• W2185979087 cites W2044093857 @default.
• W2185979087 cites W2048152489 @default.
• W2185979087 cites W2049518851 @default.
• W2185979087 cites W2054851301 @default.
• W2185979087 cites W2058924998 @default.
• W2185979087 cites W2060449082 @default.
• W2185979087 cites W2066255054 @default.
• W2185979087 cites W2067857092 @default.
• W2185979087 cites W2070499796 @default.
• W2185979087 cites W2074094455 @default.
• W2185979087 cites W2084503903 @default.
• W2185979087 cites W2086328762 @default.
• W2185979087 cites W2087088410 @default.
• W2185979087 cites W2088134590 @default.
• W2185979087 cites W2103144440 @default.
• W2185979087 cites W2105153534 @default.
• W2185979087 cites W2112625578 @default.
• W2185979087 cites W2123681429 @default.
• W2185979087 cites W2124999166 @default.
• W2185979087 cites W2125977823 @default.
• W2185979087 cites W2128384154 @default.
• W2185979087 cites W2131053676 @default.
• W2185979087 cites W2134675659 @default.
• W2185979087 cites W2150995848 @default.
• W2185979087 cites W2157917411 @default.
• W2185979087 cites W2162125418 @default.
• W2185979087 cites W2166365370 @default.
• W2185979087 cites W2167122496 @default.
• W2185979087 cites W3098337129 @default.
• W2185979087 cites W3098362140 @default.
• W2185979087 cites W3098542485 @default.
• W2185979087 cites W3098784892 @default.
• W2185979087 cites W3098813210 @default.
• W2185979087 cites W3098866659 @default.
• W2185979087 cites W3099248425 @default.
• W2185979087 cites W3100361538 @default.
• W2185979087 cites W3100682178 @default.
• W2185979087 cites W3100930659 @default.
• W2185979087 cites W3100949304 @default.
• W2185979087 cites W3101580377 @default.
• W2185979087 cites W3102308370 @default.
• W2185979087 cites W3102538720 @default.
• W2185979087 cites W3102870872 @default.
• W2185979087 cites W3102903826 @default.
• W2185979087 cites W3103056658 @default.
• W2185979087 cites W3103292009 @default.
• W2185979087 cites W3103596053 @default.
• W2185979087 cites W3103635592 @default.
• W2185979087 cites W3103868583 @default.
• W2185979087 cites W3104123668 @default.
• W2185979087 cites W3104345759 @default.

• next