IGM2018: Revealing Cosmology and Reionization History with the Intergalactic Medium

Asia/Tokyo
Kavli IPMU, Kashiwa, Japan

Kavli IPMU, Kashiwa, Japan

Kashiwa, Japan
Description

Overview: As the dominant reservoir of baryons in the Universe, the intergalactic medium (IGM) plays a crucial role in the history and evolution of cosmic structure. The stars and black holes in the first galaxies emitted copious amounts of ionizing radiation, singly ionizing hydrogen and helium at z~10, and later doubly ionizing Helium at z~3, thus reheating and reionizing the cosmos. The IGM evolves into the clumpy cosmic web, which is the source of gas that cools and accretes onto galaxies powering star-formation, and a sink for the metal enriched material, energy, and radiation which galaxies eject. The complex interplay of these processes determines the physical state of the intergalactic gas over cosmic time. Observations of absorption lines in quasar and galaxy spectra from the present until redshift 7 provide a thermal and chemical record of the IGM, enable precision measurements of density fluctuations and the geometry of the early Universe, and provide invaluable insights into the physical processes shaping galaxy formation. In the next few years, advances in telescope instrumentation, the emergence of massive spectroscopic surveys, as well as developments in theory and computation will deepen our understanding of the IGM as a probe of cosmology and the cosmic reionization events. This conference aims to bring together both theorists and observers working on the various astronomical passbands to discuss the latest developments in this exciting field.

Dates: September 18th - 21st, 2018

Deadlines: Abstract submission is now closed. You may still register to attend the meeting until September 1st, 2018.

Venue: Kavli IPMU, Kashiwa, Japan

Organizers: Khee-Gan Lee (Kavli IPMU), Nao Suzuki (Kavli IPMU)

Scientific Organizing Committee:

Piero Madau (UCSC) Valentina D'Odorico (INAF/OATS)
Matt McQuinn (Washington) Raghunathan Srianand (IUCAA)
Nathalie Palanque-Delabrouille (CEA Saclay) Martin Haehnelt (Cambridge)
Joe Hennawi (UCSB)  


Confirmed Speakers: 

Benedetta Ciardi (MPA) Daniel Stark (Arizona) Andreu Font-Ribera (UCL)
Andrei Mesinger (SNS) Laura Keating (CITA) Matteo Viel (INAF-OATS)
Andrea Ferrara (SNS) Masami Ouchi (Tokyo) Chen Heinrich (JPL)
Emma Ryan-Weber (Swinburne) Naoki Yoshida (Kavli IPMU) Michael Walther (UCSB)
Fred Davies (UCSB) Christina Eilers (MPIA) George Becker (UC Riverside)
Christophe Yèche (CEA Saclay) Raul Monsalve (Colorado/McGill)  

Address:

Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), the University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa City, Chiba 277-8583, Japan


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Participants
  • Aaron Ewall-Wice
  • Aaron Parsons
  • Akio Inoue
  • Alexey Boyarsky
  • Ana Paulino-Afonso
  • Anastasia Fialkov
  • Andrei Mesinger
  • Andreu Font-Ribera
  • Andrew Bunker
  • Andrii Magalich
  • Anna-Christina Eilers
  • Anson D'Aloisio
  • Antonella Garzilli
  • Atsushi Nishizawa
  • Ben Horowitz
  • Benedetta Ciardi
  • Benjamin Saliwanchik
  • Chen Heinrich
  • Chris Pedersen
  • Christophe Yeche
  • Craig Douglass
  • Daniel Stark
  • David Stark
  • Debanjan Sarkar
  • Elisa Boera
  • Emma Ryan-Weber
  • Evgenii Vasiliev
  • Francesco Haardt
  • Frederick Davies
  • Gabor Worseck
  • George Becker
  • Hannah Ross
  • Harley Katz
  • Hayato Shimabukuro
  • Hector Hiss
  • Huanqing Chen
  • Hy Trac
  • Ilya Khrykin
  • J. Xavier Prochaska
  • Jiani Ding
  • John Silverman
  • Jordi Miralda-Escudé
  • Jose Monzon
  • Kana Moriwaki
  • Keir Rogers
  • Kenji Hasegawa
  • Kenji Kubota
  • Kentaro Nagamine
  • Keri Dixon
  • Khee-Gan Lee
  • Kirit Karkare
  • Laura Keating
  • Malte Schramm
  • Marc Rafelski
  • Martin Haehnelt
  • Masahiro Takada
  • Masami Ouchi
  • Masayuki Umemura
  • Matteo Viel
  • Matthew McQuinn
  • Matthew Wilde
  • Metin Ata
  • Michael Rauch
  • Michael Walther
  • Miftahul Hilmi
  • Miguel Folgado
  • Nao Suzuki
  • Naoki Yoshida
  • Nathalie Palanque-Delabrouille
  • Nicholas Kern
  • Nicolas Fagnoni
  • Nobunari Kashikawa
  • Oleg Ruchayskiy
  • Pablo Villanueva Domingo
  • Peter Laursen
  • Phoebe Upton Sanderbeck
  • Piero Madau
  • Priyanka Jalan
  • Raghunathan Srianand
  • Raul Monsalve
  • Rieko Momose
  • Rika Ando
  • Robin Kooistra
  • Romain Meyer
  • Ryan Endsley
  • Sarmadi Almecci
  • Sergei Balashev
  • Shohei Aoyama
  • Shoichiro Tanaka
  • Simeon Bird
  • Soumak Maitra
  • Sownak Bose
  • Stephanie Tonnesen
  • Surhud More
  • Taisuke Nakashima
  • Takanobu Kirihara
  • Ting-Wen Lan
  • Tobias Schmidt
  • Tomomi Sunayama
  • Tomoya Kaneuji
  • Toru Misawa
  • Toshiyuki Tanaka
  • Utane Sawangwit
  • Valentina D'Odorico
  • Xiaohui Fan
  • Yi Mao
  • Yongming Liang
  • Yuichi Harikane
  • Zarija Lukic
Contact
    • Introduction by Deputy Director Misao Sasaki: Preliminaries
    • 1
      Ciardi (30 mins): The heating and ionization of the IGM: theoretical modeling and observational probes (Session Chair: Haehnelt)
    • 2
      D'Aloisio (15 mins): How hot does the IGM get during reionization?
    • 3
      Mesinger (20 mins): Modeling reionization observables
    • 10:40
      Coffee Break
    • 4
      Heinrich (20 mins): Complete reionization constraints from Planck data
    • 5
      Trac (15 mins): Simulations and Constructions of the Reionization of Cosmic Hydrogen
    • 6
      Mao (15 mins): Antisymmetric cross power spectrum as a new probe of cosmic reionization
    • 7
      Lightning Talks I: Tanaka, Karkare, Aoyama, Ewall-Wice
    • 12:25
      Lunch Atelier Joel Robuchon

      Atelier Joel Robuchon

    • 8
      Stark (30 mins): Deep Spectroscopy of Lyman-alpha Emitters in the Reionization Era (Session Chair: Prochaska)
    • 9
      Bunker (15 mins): Exploring the IGM and Reionization with JWST
    • 10
      Ouchi (20 mins): Subaru Hyper Suprime-Cam Survey for High Redshift Galaxies: Interplay between Galaxies and IGM
    • 11
      Harikane (15 mins): Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC
    • 12
      Paulino-Afonso (15 mins): The end of the reionisation: what are the most luminous Lyman-a emitters telling us?

      The end of the reionisation: what are the most luminous Lyman-a emitters telling us?

    • 13
      Poster Presentations
    • 15:35
      Coffee Break
    • 14
      Walther (20 mins): New measurements of thermal evolution in the IGM based on absorption line analyses
    • 15
      Boera (15 mins): The impact of Reionization on the IGM thermal history: present and future constraints
    • 16
      Hiss (15 mins): A New Statistical Method for Measuring the Temperature-Density Relation in the IGM using the b-N Distribution
    • 17
      Worseck (15 mins): Constraints on the High-Redshift Quasar Population from Ongoing HeII Reionization at z~4
    • 18
      Khrykin (15 mins): The He II proximity effect at z~4: evidence for short quasar lifetime
    • 19
      D'Odorico (30 mins): Constraints on reionization and the first sources from quasar absorption spectra (Session Chair: Ryan-Weber)
    • 20
      Fan (15 mins): New Surveys of Luminous z~7 Quasars: Mapping Reionization History
    • 21
      Davies (20 mins): Measuring the Reionization History with Quasar Damping Wings
    • 22
      Keating (20 mins): The IGM at the end of reionization
    • 10:45
      Coffee Break
    • 23
      Lee (20 mins): Mapping the z~2 Cosmic Web with IGM Tomography
      Lee
    • 24
      Nagamine (15 mins): Subaru PFS survey and IGM tomography using Cosmological Hydrodynamic Simulations
    • 25
      Schmidt (15 mins): Mapping quasar light echos in three dimensions with Lya forest tomography
    • 26
      Maitra (15 mins): Three point correlation of the IGM
    • 12:30
      Lunch Sukiyabashi Jiro

      Sukiyabashi Jiro

    • 27
      Srianand (20 mins): Influence of ionising UV Background on the inferred properties of metals in the IGM (Session Chair: Yoshida)
    • 28
      Haardt (15 mins): The cosmic ultraviolet background then and now
    • 29
      Upton Sanderbeck (15 mins): The impact of ultraviolet background fluctuations on galaxy clustering measurements
    • 30
      Bose (15 mins): How the present-day distribution of dwarf galaxies encodes the physics of reionisation
    • 15:10
      Coffee Break
    • 15:30
      Self-Organized Excursion to Asakusa Asakusa

      Asakusa

    • 18:30
      Conference Dinner on "Amitatsu" Banquet Boat Asakusa

      Asakusa

      Departing from Asakusa pier

    • 31
      Haehnelt (30 mins): The emergence of structure during the epoch of reionization (Session Chair: Miralda-Escude)
    • 32
      Yoshida (20 mins): Structure formation in the early universe
    • 33
      McQuinn (20 mins): The perturbation theory of everything (IGM)
    • 11:10
      Coffee Break
    • 34
      Monsalve (20 mins): An Absorption Profile in the Sky-Averaged Radio Spectrum
    • 35
      Parsons (15 mins): Prospects for Mapping the z~10 IGM with HERA
    • 36
      Kern (15 mins): Early Data Analysis and Power Spectrum Efforts from HERA
    • 37
      Fialkov (15 mins): Illuminating Dark Ages
    • 12:55
      Lunch Usukifugu Yamadaya

      Usukifugu Yamadaya

    • 38
      Ross (15 mins): Simulating the 21-cm signal from the Cosmic Dawn (Session Chair: McQuinn)
    • 39
      Dixon (15 mins): Reionization on the large scales
    • 40
      Katz (15 mins): The Sphinx Simulations: The Impact of Inhomogeneous Reionization on the IGM and Galaxy Formation
    • 41
      Lightning Talks II: Balashev, Laursen, Suzuki, Liang, Fagnoni
    • 15:30
      Coffee Break
    • 42
      Font-Ribera (30 mins): Studying the Expansion of the Universe with quasar spectra (Session Chair: McQuinn)
    • 43
      Yeche (20 mins): Neutrino masses and cosmology with Lyman-alpha forest power spectrum
    • 44
      Palanque-Delabrouille (20 mins): Sterile neutrinos in cosmology
    • 45
      Lightning Talks III: Rogers, Pedersen, Prochaska, Meyer, Shimabukuro
    • 46
      Tonnesen (15 mins): Probing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα Forest (Session Chair: D'Odorico)
    • 47
      Lukic (15 mins): WHIM in hydrodynamical simulations
    • 48
      Kooistra (15 mins): Probing the neutral IGM in filaments with SKA
    • 49
      Ando (15 mins): Redshift space distortion of 21cm line with cosmological hydrodynamic simulations
    • 50
      Saliwanchik (15 mins): Mapping BAO with the HIRAX Radio Array
    • 10:40
      Coffee Break
    • 51
      Becker (20 mins): Connecting IGM Opacity Fluctuations to Galaxies Near Reionization
    • 52
      Rauch (15 mins): Probing the Nature of Low Density Regions in the High Z IGM
    • 53
      Ding (15 mins): A new measurement on the effective optical depth of Lyman Series
    • 54
      Eilers (20 mins): The Intergalactic Medium at High Redshift and its Implications on the Epoch of Reionization
    • 12:30
      Lunch Azabu Yukimura

      Azabu Yukimura

    • 55
      Viel (20 mins): Intergalactic Medium constraints on dark matter properties (Session Chair: Palanque-Delabrouille)
    • 56
      Garzilli (15 mins): Lyman-alpha revisited: baryonic effects versus warm dark matter
    • 57
      Bird (15 mins):Is It Time to Stop Rescaling Spectra to Match the Observed Mean Flux?
    • 58
      Ryan-Weber (20 mins): Galaxies, Intergalactic and Circumgalatic Carbon at redshifts 4 to 6
    • 15:15
      Coffee Break
    • 59
      Miralda-Escudé (15 mins): Host halo masses of damped lyman alpha systems as a function of metal line strength (Session Chair: Hennawi)
    • 60
      Rafelski (15 mins): Evolution of the metallicity, incidence rate, and hydrogen mass density of damped Lyman-alpha systems out to z~5
    • 61
      Lan (15 mins): Metallicity and morphology of the circumgalactic medium
    • 62
      Conference Summary by Piero Madau (45 mins)