Matches in SemOpenAlex for { <https://semopenalex.org/work/W2969324246> ?p ?o ?g. }
- W2969324246 abstract "This paper outlines the science case for line-intensity mapping with a space-borne instrument targeting the sub-millimeter (microwaves) to the far-infrared (FIR) wavelength range. Our goal is to observe and characterize the large-scale structure in the Universe from present times to the high redshift Epoch of Reionization. This is essential to constrain the cosmology of our Universe and form a better understanding of various mechanisms that drive galaxy formation and evolution. We argue that the proposed frequency range would make it possible to probe important metal cooling lines such as [CII] up to very high redshift as well as a large number of rotational lines of the CO molecule. These can be used to trace molecular gas and dust evolution and constrain the buildup in both the cosmic star formation rate density and the cosmic infrared background (CIB). Moreover, surveys at the highest frequencies will detect FIR lines which are used as diagnostics of galaxies and AGN. Tomography of these lines over a wide redshift range will enable invaluable measurements of the cosmic expansion history at epochs inaccessible to other methods, competitive constraints on the parameters of the standard model of cosmology, and numerous tests of dark matter, dark energy, modified gravity and inflation. To reach these goals, large-scale structure must be mapped over a wide range in frequency to trace its time evolution over a reasonable fraction of the volume of the observable Universe. In addition, the surveyed area needs to be very large to beat cosmic variance and to probe the largest scales where its easier to separate the astrophysical and cosmological contributions to the observed signal. Only, a space-borne mission can properly meet these requirements." @default.
- W2969324246 created "2019-08-29" @default.
- W2969324246 creator A5006341437 @default.
- W2969324246 creator A5015970622 @default.
- W2969324246 creator A5018395981 @default.
- W2969324246 creator A5025321333 @default.
- W2969324246 creator A5035557169 @default.
- W2969324246 creator A5047971920 @default.
- W2969324246 creator A5051524423 @default.
- W2969324246 creator A5054190787 @default.
- W2969324246 creator A5066518636 @default.
- W2969324246 date "2019-10-22" @default.
- W2969324246 modified "2023-09-27" @default.
- W2969324246 title "Mapping Large-Scale-Structure Evolution over Cosmic Times" @default.
- W2969324246 cites W1037667007 @default.
- W2969324246 cites W1496460803 @default.
- W2969324246 cites W1534648590 @default.
- W2969324246 cites W1558798502 @default.
- W2969324246 cites W1667726566 @default.
- W2969324246 cites W1793882623 @default.
- W2969324246 cites W1830746653 @default.
- W2969324246 cites W1994981447 @default.
- W2969324246 cites W2013997547 @default.
- W2969324246 cites W2027635416 @default.
- W2969324246 cites W2028757778 @default.
- W2969324246 cites W2067649418 @default.
- W2969324246 cites W2068577843 @default.
- W2969324246 cites W2073938066 @default.
- W2969324246 cites W2081852959 @default.
- W2969324246 cites W2082674267 @default.
- W2969324246 cites W2097835815 @default.
- W2969324246 cites W2102336972 @default.
- W2969324246 cites W2119131940 @default.
- W2969324246 cites W2130563989 @default.
- W2969324246 cites W2135307561 @default.
- W2969324246 cites W2135335133 @default.
- W2969324246 cites W2144910248 @default.
- W2969324246 cites W2147626801 @default.
- W2969324246 cites W2233026052 @default.
- W2969324246 cites W2240612907 @default.
- W2969324246 cites W2268048116 @default.
- W2969324246 cites W2285875586 @default.
- W2969324246 cites W2333082371 @default.
- W2969324246 cites W2470245986 @default.
- W2969324246 cites W2515638351 @default.
- W2969324246 cites W2558514382 @default.
- W2969324246 cites W2586531505 @default.
- W2969324246 cites W2597412078 @default.
- W2969324246 cites W2607228707 @default.
- W2969324246 cites W2728482766 @default.
- W2969324246 cites W2754959546 @default.
- W2969324246 cites W2756473891 @default.
- W2969324246 cites W2760594049 @default.
- W2969324246 cites W2762741961 @default.
- W2969324246 cites W2764096479 @default.
- W2969324246 cites W2788258268 @default.
- W2969324246 cites W2792686445 @default.
- W2969324246 cites W2799088967 @default.
- W2969324246 cites W2802270478 @default.
- W2969324246 cites W2803801964 @default.
- W2969324246 cites W2804669945 @default.
- W2969324246 cites W2807009254 @default.
- W2969324246 cites W2808302137 @default.
- W2969324246 cites W2809759060 @default.
- W2969324246 cites W2812623185 @default.
- W2969324246 cites W2884028096 @default.
- W2969324246 cites W2888035497 @default.
- W2969324246 cites W2893595334 @default.
- W2969324246 cites W2900304263 @default.
- W2969324246 cites W2902092047 @default.
- W2969324246 cites W2920866920 @default.
- W2969324246 cites W2921866506 @default.
- W2969324246 cites W2949460745 @default.
- W2969324246 cites W2950838963 @default.
- W2969324246 cites W2961457169 @default.
- W2969324246 cites W2962961900 @default.
- W2969324246 cites W2963045701 @default.
- W2969324246 cites W2963122279 @default.
- W2969324246 cites W2964330856 @default.
- W2969324246 cites W2964341266 @default.
- W2969324246 cites W2995509084 @default.
- W2969324246 cites W3098285627 @default.
- W2969324246 cites W3098522964 @default.
- W2969324246 cites W3098967230 @default.
- W2969324246 cites W3100139394 @default.
- W2969324246 cites W3101475091 @default.
- W2969324246 cites W3102034977 @default.
- W2969324246 cites W3102449281 @default.
- W2969324246 cites W3103107149 @default.
- W2969324246 cites W3103494697 @default.
- W2969324246 cites W3103714828 @default.
- W2969324246 cites W3103730211 @default.
- W2969324246 cites W3104404122 @default.
- W2969324246 cites W3104405069 @default.
- W2969324246 cites W3104728800 @default.
- W2969324246 cites W3104860562 @default.
- W2969324246 cites W3104984377 @default.
- W2969324246 cites W3123046296 @default.
- W2969324246 cites W569873724 @default.
- W2969324246 cites W608922738 @default.