FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4293791195> ?p ?o ?g. }

• W4293791195 endingPage "2970" @default.
• W4293791195 startingPage "2947" @default.
• W4293791195 abstract "We present the results of a search for associated 21 cm HI absorption at redshift 0.42 < z < 1.00 in radio-loud galaxies from three Galaxy And Mass Assembly (GAMA) survey fields. These observations were carried out as part of a pilot survey for the ASKAP First Large Absorption Survey in HI (FLASH). From a sample of 326 radio sources with 855.5 MHz peak flux density above 10 mJy we detected two associated HI absorption systems, in SDSS J090331+010847 at z= 0.522 and SDSS J113622+004852 at z= 0.563. Both galaxies are massive (stellar mass > 10$^{11}$ M$_{sun}$) and have optical spectra characteristic of luminous red galaxies,though SED fitting implies that SDSS J113622+004852 contains a dust-obscured starburst with SFR ~ 69 M$_{sun}$ yr$^{-1}$. The HI absorption lines have a high optical depth, with $tau_{pk}$ of 1.77 $pm$ 0.16 for SDSS J090331+010847 (the highest value for any z > 0.1 associated system found to date) and 0.14 $pm$ 0.01 for SDSS J113622+004852. In the redshift range probed by our ASKAP observations, the detection rate for associated HI absorption lines (with $tau_{pk}$ > 0.1 and at least 3$sigma$ significance) is 2.9 (+9.7 -2.6) percent. Although the current sample is small, this rate is consistent with a trend seen in other studies for a lower detection rate of associated 21 cm HI absorption systems at higher redshift. We also searched for OH absorption lines at 0.67 < z < 1.34, but no detection was made in the 145 radio sources searched." @default.
• W4293791195 created "2022-08-31" @default.
• W4293791195 creator A5002092890 @default.
• W4293791195 creator A5040415300 @default.
• W4293791195 creator A5043531190 @default.
• W4293791195 creator A5043877824 @default.
• W4293791195 creator A5052703931 @default.
• W4293791195 creator A5054995116 @default.
• W4293791195 creator A5057384888 @default.
• W4293791195 creator A5064202595 @default.
• W4293791195 creator A5066897090 @default.
• W4293791195 creator A5071642172 @default.
• W4293791195 creator A5072524896 @default.
• W4293791195 creator A5077432294 @default.
• W4293791195 creator A5089501032 @default.
• W4293791195 creator A5090755551 @default.
• W4293791195 creator A5090939849 @default.
• W4293791195 date "2022-08-18" @default.
• W4293791195 modified "2023-10-17" @default.
• W4293791195 title "FLASH pilot survey: detections of associated 21 cm H <scp>i</scp> absorption in GAMA galaxies at 0.42 &lt; <i>z</i> &lt; 1.00" @default.
• W4293791195 cites W1847272642 @default.
• W4293791195 cites W1926882107 @default.
• W4293791195 cites W1943306457 @default.
• W4293791195 cites W1948511999 @default.
• W4293791195 cites W1966667130 @default.
• W4293791195 cites W1970058472 @default.
• W4293791195 cites W1972667386 @default.
• W4293791195 cites W1975549325 @default.
• W4293791195 cites W1977637580 @default.
• W4293791195 cites W1978552873 @default.
• W4293791195 cites W1979088966 @default.
• W4293791195 cites W1985584747 @default.
• W4293791195 cites W1985706855 @default.
• W4293791195 cites W1986643693 @default.
• W4293791195 cites W1988239806 @default.
• W4293791195 cites W2007975728 @default.
• W4293791195 cites W2015492754 @default.
• W4293791195 cites W2020623222 @default.
• W4293791195 cites W2022429079 @default.
• W4293791195 cites W2023873184 @default.
• W4293791195 cites W2029901638 @default.
• W4293791195 cites W2033003110 @default.
• W4293791195 cites W2044137421 @default.
• W4293791195 cites W2052937506 @default.
• W4293791195 cites W2061512713 @default.
• W4293791195 cites W2064174775 @default.
• W4293791195 cites W2064922940 @default.
• W4293791195 cites W2065973509 @default.
• W4293791195 cites W2069807023 @default.
• W4293791195 cites W2082671134 @default.
• W4293791195 cites W2084147024 @default.
• W4293791195 cites W2089151099 @default.
• W4293791195 cites W2091651313 @default.
• W4293791195 cites W2095363617 @default.
• W4293791195 cites W2096438709 @default.
• W4293791195 cites W2099351385 @default.
• W4293791195 cites W2101841715 @default.
• W4293791195 cites W2106246367 @default.
• W4293791195 cites W2106578604 @default.
• W4293791195 cites W2111817932 @default.
• W4293791195 cites W2114232018 @default.
• W4293791195 cites W2127490819 @default.
• W4293791195 cites W2127710072 @default.
• W4293791195 cites W2130848063 @default.
• W4293791195 cites W2131162049 @default.
• W4293791195 cites W2132459235 @default.
• W4293791195 cites W2138169438 @default.
• W4293791195 cites W2138759791 @default.
• W4293791195 cites W2139247602 @default.
• W4293791195 cites W2146660402 @default.
• W4293791195 cites W2148024523 @default.
• W4293791195 cites W2148719886 @default.
• W4293791195 cites W2155630450 @default.
• W4293791195 cites W2159883804 @default.
• W4293791195 cites W2166225242 @default.
• W4293791195 cites W2168912860 @default.
• W4293791195 cites W2209241523 @default.
• W4293791195 cites W2212386031 @default.
• W4293791195 cites W2223095747 @default.
• W4293791195 cites W2231870811 @default.
• W4293791195 cites W2253597312 @default.
• W4293791195 cites W2255673326 @default.
• W4293791195 cites W2277885298 @default.
• W4293791195 cites W2467658441 @default.
• W4293791195 cites W2520740623 @default.
• W4293791195 cites W2522408454 @default.
• W4293791195 cites W2546745436 @default.
• W4293791195 cites W2560093780 @default.
• W4293791195 cites W2581955329 @default.
• W4293791195 cites W2629929376 @default.
• W4293791195 cites W2724593991 @default.
• W4293791195 cites W2760131850 @default.
• W4293791195 cites W2761862871 @default.
• W4293791195 cites W2766288343 @default.
• W4293791195 cites W2769452099 @default.
• W4293791195 cites W2783332169 @default.
• W4293791195 cites W2786879317 @default.
• W4293791195 cites W2788385650 @default.

• next