3D Gas Tomography of Cosmic Large Scale Structure 10 Billion years Ago
| Project/Area Number |
18H05868
|
|---|
| Research Category |
Grant-in-Aid for Research Activity Start-up
|
| Allocation Type | Single-year Grants |
|---|
| Review Section |
0204:Astronomy, earth and planetary science, and related fields
|
|---|
| Research Institution | The University of Tokyo |
|---|
Principal Investigator |
Lee KheeGan 東京大学, カブリ数物連携宇宙研究機構, 特任講師 (10822091)
|
|---|
| Project Period (FY) |
2018-08-24 – 2020-03-31
|
| Project Status |
Completed (Fiscal Year 2018)
|
| Budget Amount *help |
¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2018: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
|
|---|
| Keywords | astronomy / astrophysics / cosmic web / large-scale structure / cosmology |
|---|
| Outline of Annual Research Achievements |
In FY2018, we published the first data release of the CLAMATO absorption tomography survey probing the 2.0<z<2.5 intergalactic medium (IGM), which I led and authored. This was accompanied by the detection of cosmic voids within this data at <z>~2.3, which marks the most distant sample of cosmic voids observed to-date. At the same time, we have also worked on theoretical methods to estimate the underlying dark matter density field using IGM tomography data. The initial paper describing the basic method has recently been completed, showing that this technique is able to recover well the cosmic web structure in the observational volume. Another application of IGM tomography is to target the volume near ultraluminous quasars to measure the effect of the intense quasar radiation on the nearby IGM structures - the first paper describing method has also been submitted.
Observationally, we managed to get additional telescope time to obtain more data in January and February 2019, which will increase our observational footprint by 25% and improving coverage of the large galaxy protoclusters in that volume. We are continuing to apply for more telescope time to further increase the coverage and maximize the scientific yield.
These results are feeding into the survey science definition for the Prime Focus Spectrograph on the Subaru Telescope, which will be Japan's next major astronomical survey facility starting from 2022.
|
| Research Progress Status |
平成30年度が最終年度であるため、記入しない。
|
| Strategy for Future Research Activity |
平成30年度が最終年度であるため、記入しない。
|
Report
(1 results)
Research Products
(8 results)
