Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100462550> ?p ?o ?g. }
- W3100462550 endingPage "16" @default.
- W3100462550 startingPage "1" @default.
- W3100462550 abstract "The C III] λλ 1907, 1909 emission doublet has been proposed as an alternative to Lyman-α in redshift confirmations of galaxies at z ≳ 6 since it is not attenuated by the largely neutral intergalactic medium at these redshifts and is believed to be strong in the young, vigorously star-forming galaxies present at these early cosmic times. We present a statistical sample of 17 C III]-emitting galaxies beyond z ~ 1.5 using ~30 h deep VLT/MUSE integral field spectroscopy covering 2 square arcminutes in the Hubble Deep Field South (HDFS) and Ultra Deep Field (UDF), achieving C III] sensitivities of ~ 2 × 10-17 erg s-1 cm-2 in the HDFS and ~ 7 × 10-18 erg s-1 cm-2 in the UDF. The rest-frame equivalent widths range from 2 to 19 A. These 17 galaxies represent ~3% of the total sample of galaxies found between 1.5 ≲ z ≲ 4. They also show elevated star formation rates, lower dust attenuation, and younger mass-weighted ages than the general population of galaxies at the same redshifts. Combined with deep slitless grism spectroscopy from the HST/WFC3 in the UDF, we can tie the rest-frame ultraviolet C III] emission to rest-frame optical emission lines, namely [O III] λ 5007, finding a strong correlation between the two. Down to the flux limits that we observe (~ 1 × 10-18 erg s-1 cm-2 with the grism data in the UDF), all objects with a rest-frame [O III] λλ 4959, 5007 equivalent width in excess of 250 A, the so-called extreme emission line galaxies, have detections of C III] in our MUSE data. More detailed studies of the C III]-emitting population at these intermediate redshifts will be crucial to understand the physical conditions in galaxies at early cosmic times and to determine the utility of C III] as a redshift tracer." @default.
- W3100462550 created "2020-11-23" @default.
- W3100462550 creator A5001016126 @default.
- W3100462550 creator A5013271839 @default.
- W3100462550 creator A5014596652 @default.
- W3100462550 creator A5020050534 @default.
- W3100462550 creator A5022894838 @default.
- W3100462550 creator A5028898239 @default.
- W3100462550 creator A5032025507 @default.
- W3100462550 creator A5046181082 @default.
- W3100462550 creator A5053677091 @default.
- W3100462550 creator A5055513022 @default.
- W3100462550 creator A5055826068 @default.
- W3100462550 creator A5060806863 @default.
- W3100462550 creator A5077065356 @default.
- W3100462550 creator A5079172029 @default.
- W3100462550 creator A5084269645 @default.
- W3100462550 date "2017-12-01" @default.
- W3100462550 modified "2023-10-01" @default.
- W3100462550 title "The MUSE Hubble Ultra Deep Field Survey - IV. Global properties of C III] emitters" @default.
- W3100462550 cites W1495243983 @default.
- W3100462550 cites W1525855014 @default.
- W3100462550 cites W1582953240 @default.
- W3100462550 cites W1610452254 @default.
- W3100462550 cites W1722819912 @default.
- W3100462550 cites W1742810195 @default.
- W3100462550 cites W1787231361 @default.
- W3100462550 cites W1875890127 @default.
- W3100462550 cites W1888590559 @default.
- W3100462550 cites W1891417619 @default.
- W3100462550 cites W1908085087 @default.
- W3100462550 cites W1912798299 @default.
- W3100462550 cites W1929287038 @default.
- W3100462550 cites W1964084977 @default.
- W3100462550 cites W1965353112 @default.
- W3100462550 cites W1968744481 @default.
- W3100462550 cites W1974288578 @default.
- W3100462550 cites W1976737607 @default.
- W3100462550 cites W1980488087 @default.
- W3100462550 cites W1985418880 @default.
- W3100462550 cites W1986510200 @default.
- W3100462550 cites W2006214076 @default.
- W3100462550 cites W2008228827 @default.
- W3100462550 cites W2008777327 @default.
- W3100462550 cites W2013741966 @default.
- W3100462550 cites W2018539983 @default.
- W3100462550 cites W2020648693 @default.
- W3100462550 cites W2025717087 @default.
- W3100462550 cites W2037878575 @default.
- W3100462550 cites W2040634438 @default.
- W3100462550 cites W2048136989 @default.
- W3100462550 cites W2055390206 @default.
- W3100462550 cites W2057816597 @default.
- W3100462550 cites W2067857092 @default.
- W3100462550 cites W2070829450 @default.
- W3100462550 cites W2076051966 @default.
- W3100462550 cites W2080624490 @default.
- W3100462550 cites W2081220046 @default.
- W3100462550 cites W2082377112 @default.
- W3100462550 cites W2088723553 @default.
- W3100462550 cites W2093520301 @default.
- W3100462550 cites W2094871238 @default.
- W3100462550 cites W2103267716 @default.
- W3100462550 cites W2115967849 @default.
- W3100462550 cites W2118229083 @default.
- W3100462550 cites W2124199755 @default.
- W3100462550 cites W2129619027 @default.
- W3100462550 cites W2131303567 @default.
- W3100462550 cites W2133581151 @default.
- W3100462550 cites W2135400154 @default.
- W3100462550 cites W2135625048 @default.
- W3100462550 cites W2150819820 @default.
- W3100462550 cites W2151062050 @default.
- W3100462550 cites W2153610806 @default.
- W3100462550 cites W2157917411 @default.
- W3100462550 cites W2166365370 @default.
- W3100462550 cites W2184399044 @default.
- W3100462550 cites W2231005101 @default.
- W3100462550 cites W2235062852 @default.
- W3100462550 cites W2286156139 @default.
- W3100462550 cites W2290750753 @default.
- W3100462550 cites W2413278594 @default.
- W3100462550 cites W2522290439 @default.
- W3100462550 cites W2573999096 @default.
- W3100462550 cites W2594398567 @default.
- W3100462550 cites W2950015636 @default.
- W3100462550 cites W2951323278 @default.
- W3100462550 cites W2990150359 @default.
- W3100462550 cites W3021809919 @default.
- W3100462550 cites W3098475011 @default.
- W3100462550 cites W3098927306 @default.
- W3100462550 cites W3099024504 @default.
- W3100462550 cites W3099774793 @default.
- W3100462550 cites W3100077317 @default.
- W3100462550 cites W3100387168 @default.
- W3100462550 cites W3100564066 @default.
- W3100462550 cites W3101455189 @default.
- W3100462550 cites W3101548371 @default.