Cosmic Cartography 2022: Exploring the Cosmic Web and Large-Scale Structure

Session

Day 2 Morning

2.1

8 Mar 2022, 09:00

Lecture Hall (Kavli IPMU, Kashiwa, Japan)

10. Large Scale Structure with the Prime Focus Spectrograph

Jenny Green (Princeton University)

08/03/2022, 09:00

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The Prime Focus Spectrograph will be an incredibly powerful instrument for large-area surveys of galaxies over most of cosmic time. With its wide wavelength coverage and multiplexing capabilities, it will be a powerful redshift machine. I will briefly describe the Strategic Survey Plan, and then focus on the Galaxy Evolution survey. With our Main survey, we will define the anisotropic...

11. Chrono-Cosmographic Analysis of the Cosmic Web with TARDIS

Benjamin Horowitz (Princeton University)

08/03/2022, 09:30

Recent Lyman-α forest tomography measurements of the intergalactic medium (IGM) have revealed a wealth of cosmic structures at high redshift (z ∼ 2.5), including detection of large voids and protoclusters. In this talk, I will discuss ongoing work on the Tomographic Absorption Reconstruction and Density Inference Scheme (TARDIS), a chrono-cosmographic analysis tool for understanding the...

12. Cartography of the Forming Galaxy Clusters: Proposal for a NIR spectroscopic campaign on IGM tomography map by PFS-SSP

Rhythm Shimakawa (NAOJ)

08/03/2022, 10:00

We will present highlights of our past deep Hα imaging and follow-up spectroscopy to dense forming proto-clusters at the cosmic noon (Shimakawa et al. 2014-18). We found enhanced star formation and gas-phase metallicity in low-mass galaxies in the protocluster cores at z=2-3. Combined with Lyα deficits therein, we suggest the forming cluster cores are associated with lavish gas reservoirs and...

13. The Cosmic Web and Galaxy Ecosystems Revealed by Slime Mold

Joseph Burchett (New Mexico State University)

08/03/2022, 10:40

Gas in the Cosmic Web, long associated with the IGM on large scales and CGM on small scales must fuel galaxy reservoirs and bear the imprint of galaxy feedback and structure formation. However, empirically connecting galaxies, their CGM, and the IGM within a Cosmic Web context has proven elusive. I will present our Cosmic Web reconstruction method Monte Carlo Physarum Machine (MCPM), inspired...

14. The Absorption and Emission of Neutral Hydrogen around Star-Forming Galaxies at Cosmic Noon

Yuguang Chen (University of California, Davis)

08/03/2022, 11:00

HI is an important component of the CGM/IGM gas. I will present two powerful samples from the KBSS Survey that focus on the Lya absorption and emission around z~2 star-forming galaxies. For absorption, we use the spectra of ~3000 galaxies to assemble ~200,000 foreground-background galaxy pairs. The ensemble is used to construct a 2D map of Lya absorption at 20-4000 kpc. The map suggests that...

15. Constraining the Cosmic Baryon Distribution with FRB Foreground Mapping

Ilya Khrykin (Kavli IPMU)

08/03/2022, 11:20

The FRB can shed light on the ‘missing’ baryons problem, because the dispersion of the FRB signals encodes information about the ionized gas along the line-of-sight. The majority of this dispersion is expected to come from the diffuse IGM tracing the cosmic web. However, the cosmic variance significantly decreases the sensitivity of the FRB. We introduce a technique to estimate the density...

16. Foreground halo contributions to FRB dispersion measures: Preliminary constraints from the FLIMFLAM Survey

Sunil Simha (University of California Santa Cruz)

08/03/2022, 11:40

Fast radio burst (FRB) dispersion measures (DMs) from radio observations record the presence of ionized baryons that are otherwise invisible to effectively all other techniques. Therefore, with FRBs, we may resolve the matter distribution in the cosmic web offering unique constraints on our cosmological paradigm. The number of FRBs localized to their host galaxies has steadily increased to the...