There is still a great deal to be learnt from CMB measurements. I will give an overview of science that the community hope to do with new data, from testing initial conditions of the universe to probing the dark sector and better understanding cosmic reionization and galaxy evolution. I will also describe some of the rich millimeter-wave science that can be done with these datasets, including...

104. Invited talk by Tomotake Matsumura (Kavli IPMU Tokyo) on "Scientific challenges expected from future space experiments"

5/23/22, 11:25 AM

Science Challenges

The measurement of cosmic microwave background (CMB) from space is ideal for the entire sky access and broad observational frequency coverage. The past CMB satellite missions, COBE, WMAP, and Planck, play crucial roles in establishing modern cosmology. Now next-generation satellite missions will aim for even more demanding scientific goals, and the various corresponding requirements on the...

105. Invited talk by Suzanne Staggs (Princeton University) on "Scientific challenges expected from future ground experiments"

5/23/22, 11:55 AM

Science Challenges

106. Invited talk by Paolo de Bernardis (Rome Sapienza University) on "Scientific challenges expected from future balloon experiments"

5/23/22, 12:25 PM

Science Challenges

107. Invited talk by Anthony Challinor (Cambridge University) on "CMB probes of cosmological inflation: current status and future prospects"

5/23/22, 2:00 PM

CMB, Cross-Correlation and Galactic Science

The temperature and polarisation anisotropies of the CMB offer our most direct view of the early universe and their observation has, and continues to be, critical in constraining early-universe models. In this talk, I will review the key ways that the CMB constrains the properties of the primordial fluctuations, which were likely produced during an early period of cosmological inflation, and...

108. Invited talk by Jon Gudmundsson (Stockholm University) on "Knowing your beams"

5/23/22, 2:40 PM

Beams

The cosmic microwave background (CMB) has played a foundational role in the establishment of the standard model of cosmology. Driven by significant technological advances, future CMB experiments aim to make dramatic strides in our understanding of the universe. Some of our most ambitious efforts, however, run the risk of being hamstrung by poorly-understood instrument effects, systematics. A...

109. Clara Vergès (Harvard CfA) "Beam calibration campaign requirements to control temperature-to-polarisation leakage for CMB-Stage 4"

5/23/22, 3:20 PM

Beams

110. Clément Leloup (APC Paris) "Study of beam side-lobes systematics and calibration for the LiteBIRD mission"

5/23/22, 3:40 PM

Beams

111. Emilie Storer (Princeton University) "Map-making and Beams for the Atacama Cosmology Telescope"

5/23/22, 4:00 PM

Beams

112. Invited talk by Hannes Hubmayr (NIST Boulder) on "The shape of CMB focal planes to come"

5/23/22, 4:40 PM

Detectors and Beams

The tantalizing science reach of CMB observations has driven remarkable innovation in superconducting detectors. Roughly two decades ago, CMB focal planes consisted of a few individually assembled detection channels. By use of modern micro-fabrication equipment and improved microwave design tools, today’s imaging focal planes consist of multiple-tiled, large-format wafers. A wafer may...

113. Guillermo Pascual Cisneros (IFCA Santander) "Optimization of a microwave polarimeter for astronomy with optical correlation and detection"

5/23/22, 5:20 PM

Detectors and Beams

114. Nadia Dachlythra (Oskar Klein Stockholm) "Optical calibration simulations for the Simons Observatory"

5/23/22, 5:40 PM

Detectors and Beams

115. Discussion (Jon Gudmundsson, Hannes Hubmayr)

5/23/22, 6:00 PM

Detectors and Beams

116. Invited talk by Charles R. Lawrence (NASA/JPL) on "Lessons from Planck Calibration for Future CMB Experiments"

5/24/22, 9:00 AM

Data Calibration and Characterization

Planck set new standards for calibration of CMB experiments. That was hard. Calibration of future experiments, which will require map noise levels of nanokelvin or better, will be much harder. I will discuss lessons learned in calibrating Planck for future experiments.

117. Nicholas Galitzki (UCSD) "The Characterization and Calibration of the Simons Observatory Small Aperture Telescope: Status and future plans"

5/24/22, 9:40 AM

Data Calibration and Characterization

118. Kirit Karkare (Chicago University) "Calibration and Systematics for the CMB-S4 Inflation Survey Small Aperture Telescopes"

5/24/22, 10:00 AM

Data Calibration and Characterization

119. Enrique Martínez-González (IFCA Santander) "Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite"

5/24/22, 10:20 AM

Data Calibration and Characterization

120. Gabriele Coppi (INFN Milan) "PROTOCALC: Design and Simulation of a Calibration Source for mm Telescopes"

5/24/22, 11:00 AM

Data Calibration and Characterization

122. Discussion (Daniele Mennella, Tomotake Matsumura)

5/24/22, 11:20 AM

Data Calibration and Characterization

121. Invited talk by Stephan Ilic (IJC Lab Paris) on "The history of reionisation : peering through the dark ages with the CMB"

5/24/22, 11:50 AM

CMB, Cross-Correlation and Galactic Science

Observations of the cosmic microwave background provide us with a unique window on the early Universe, and great new insights are expected from the next generation of dedicated ground and space telescopes. While probing the elusive inflationary epoch may be the most sought-after objective of those missions, they will also shed some light on another poorly-known era of the early Universe: the...

123. Invited talk by Massimiliano Lattanzi (INFN Ferrara) on "Particle and energy composition of the Universe: Neutrinos, Light relics and Dark Matter"

5/24/22, 2:00 PM

CMB, Cross-Correlation and Galactic Science

The interaction between cosmology and particle physics has always been very fruitful. Cosmological observations provide a powerful mean to test particle physics theories, and to measure the properties of existing particles like neutrinos. At the same time, the solution to two long-standing mysteries in cosmology - the origin of dark matter and dark energy - might lie in physics beyond the...

124. Invited talk by Loris Colombo (Milan University) on "Lessons learned from Planck for cosmology from large angle polarization"

5/24/22, 2:40 PM

Systematics impact on large angular scale science

125. Roger de Belsunce (Cambridge University) "Cosmological inference from large-angular scale CMB data"

5/24/22, 3:20 PM

Systematics impact on large angular scale science

126. Dominic Beck (Stanford University) "Cosmological constraints and instrumental systematics studies using line-of-sight distortion fields with BICEP/Keck and beyond"

5/24/22, 3:40 PM

Systematics impact on large angular scale science

127. Sofia Fatigoni (UBC) "High Resolution analysis of the South Pole Atmosphere for CMB observations"

5/24/22, 4:00 PM

Systematics impact on large angular scale science

128. Giulio Fabbian (CCA Flatiron Institute) "Challenges for high precision lensing reconstruction"

5/24/22, 4:40 PM

Systematics impact on large angular scale science

129. Baptiste Jost (APC Paris) "Novel method for joint systematic correction and foreground cleaning and its application to the estimation of cosmic birefringence in Simons Observatory"

5/24/22, 5:00 PM

Systematics impact on large angular scale science

130. Patricia Diego-Palazuelos (IFCA Santander) "Simultaneous determination of miscalibrated polarization angles and cosmic birefringence from Planck PR4"

5/24/22, 5:20 PM

Systematics impact on large angular scale science

131. Discussion (Matthieu Tristram, Loris Colombo)

5/24/22, 5:40 PM

Systematics impact on large angular scale science

132. Invited talk by Nicoletta Krachmalnicoff (SISSA) on "Characterization of Foreground emission for CMB experiments: current status and future prospective"

5/25/22, 9:00 AM

Foregrounds

In the recent years it has become clear how the contamination coming from Galactic and extra-Galactic emissions represents one of the main limiting factor for any new science achievable with Cosmic Microwave Background observations. Having a thorough understanding of the foreground properties is therefore fundamental in order to achieve a reliable reconstruction of the clean CMB signal and to...

133. Invited talk by Mathieu Remazeilles (IFCA Santander) on "Next steps in component separation for new CMB observables"

5/25/22, 9:30 AM

Foregrounds

Beyond the significant legacy of the ESA's Planck mission, the cosmic microwave background (CMB) radiation carries much more information that remains to be exploited in the coming decades. Next-generation CMB experiments of unprecedented sensitivity are being planned to extract and interpret new cosmological observables out of future CMB data. Among these new, yet undetected, cosmological...

134. Niall Jeffrey (UCL) "Single frequency CMB B-mode inference with realistic foregrounds from a single training image"

5/25/22, 10:00 AM

Foregrounds

135. Elena de la Hoz (IFCA Santander) "Diffuse polarized foregrounds from component separation with QUIJOTE-MFI"

5/25/22, 10:20 AM

Foregrounds

168. Benjamin Beringue (Cardiff University) "Component separation for the Simons Observatory Large Aperture Telescope"

5/25/22, 11:00 AM

Foregrounds

137. Alessia Ritacco (INAF OAC) "First low latitudes reconstruction of the dust polarization spectral energy distribution variation"

5/25/22, 11:20 AM

Foregrounds

138. Giuseppe Puglisi (Tor Vergata University) "Foreground Removal for B-Modes Detection with Clustering Methods"

5/25/22, 11:40 AM

Foregrounds

172. Brandon Hensley (Princeton University) "Beyond Foregrounds: Galactic Science in the 2020s"

5/25/22, 12:00 PM

Foregrounds

139. Discussion (Carlo Baccigalupi, Nicoletta Krachmalnicoff, Mathieu Remazeilles)

5/25/22, 12:20 PM

Foregrounds

140. Invited talk by Reijo Keskitalo (LBNL) on "Integrated data analysis and end-to-end simulations"

5/26/22, 9:00 AM

Data Analysis Interdependencies

All data analysis for an experiment is, at least implicitly, integrated. It all aims to distill scientific knowledge from a common data set. Whether the architects of the data reduction pipelines make the integration explicit is influenced by external constraints (processing power, availability of accurate models) and design strategy (highly modular or tightly coupled). Regardless of the case,...

141. Mathew Galloway (Oslo University) "BeyondPlanck – Bayesian end-to-end Analysis of Planck LFI"

5/26/22, 9:40 AM

Data Analysis Interdependencies

142. Ian Harrison (Cardiff University) "SO Likelihood Codes for CMB Combined Probes"

5/26/22, 10:00 AM

Data Analysis Interdependencies

143. Erik Rosenberg (Cambridge University) "CMB power spectra and cosmological parameters from Planck PR4 (NPIPE) with CamSpec"

5/26/22, 10:20 AM

Data Analysis Interdependencies

144. Gabriel Jung (Padova University) "The integrated angular bispectrum of the CMB"

5/26/22, 11:00 AM

Data Analysis Interdependencies

145. Adriaan Duivenvoorden (Princeton University) "The Atacama Cosmology Telescope: science and analysis pipeline"

5/26/22, 11:20 AM

Data Analysis Interdependencies

146. Etienne Camphuis (IAP Paris) "Building an accurate analytical power spectrum covariance matrix on a small survey area"

5/26/22, 11:40 AM

Data Analysis Interdependencies

147. Discussion (Paolo Natoli, Reijo Keskitalo)

5/26/22, 12:00 PM

Data Analysis Interdependencies

150. Invited talk by Jia Liu (Kavli IPMU Tokyo) on "Simulating correlated CMB and large-scale structure observables"

5/26/22, 2:00 PM

CMB, Cross-Correlation and Galactic Science

We are expecting high-precision observations from upcoming CMB surveys, such as the Simons Observatory, CMB-S4, and LiteBIRD, as well as from future surveys of the large-scale structure, such as Euclid, Rubin LSST, SPHEREx, PSF, and Roman Space Telescope. Most of the observables from these independent surveys will be correlated due to their large overlaps in sky and redshift coverage. Joint...

152. Mathew Madhavacheril (USC) "Cosmology with CMB Lensing: ACT, SO and beyond"

5/26/22, 2:40 PM

CMB, Cross-Correlation and Galactic Science

148. Laura Salvati (IAS Orsay) "Galaxy clusters in the mm wavelengths: cosmological analysis and future perspectives"

5/26/22, 3:00 PM

CMB, Cross-Correlation and Galactic Science

151. Federica Guidi (IAP Paris) "Cosmology from SPT-3G"

5/26/22, 3:20 PM

CMB, Cross-Correlation and Galactic Science

149. Vincent Pelgrims (Crete University) "Pasiphae: Goal and overview of current status"

5/26/22, 3:40 PM

CMB, Cross-Correlation and Galactic Science

153. Invited talk by Aditya Rotti (Manchester University) on "Spectral distortion science and measurement challenges"

5/26/22, 4:20 PM

CMB, Cross-Correlation and Galactic Science

165. Angela Taylor (Oxford University) "The C-Band All-Sky Survey: Northern sky-survey results"

5/26/22, 5:00 PM

Experimental results

166. Kirit Karkare (Chicago University) "The BICEP/Keck program: latest results and progress update on the upcoming BICEP Array receiver deployments"

5/26/22, 5:20 PM

Experimental results

155. Jose Alberto Rubino-Martin (IAC Tenerife) "The QUIJOTE MFI wide survey: A northern sky survey in intensity and polarization at 10–20GHz"

5/26/22, 5:40 PM

Experimental results

167. Elle Shaw (UIUC) "Limits on Cosmological B-mode Polarization in the CMB from Spider"

5/26/22, 6:00 PM

Experimental results

157. Invited talk by François R. Bouchet (IAP Paris) on "Introduction to future experiments"

5/27/22, 9:00 AM

Future Plans

158. Invited talk by Masashi Hazumi (KEK Tsukuba) on "LiteBIRD"

5/27/22, 9:30 AM

Future Plans

159. Invited talk by Jens Chluba (Manchester University) on "Ongoing and planned CMB spectrometers and what we still need to make this happen"

5/27/22, 9:50 AM

Future Plans

CMB spectral distortion measurements are going to be challenging and multiple groups are considering experimental approaches that might allow us to target these small signals in the near and distant future. In my talk I will give a brief overview of all the ongoing and planned CMB spectrometer concepts and initiatives trying in particular to highlight synergies and individual strengths. I will...

160. Invited talk by Julian Borrill (LBNL) on "From Stage 3 to Stage 4 - South Pole Observatory, Simons Observatory and CMB-S4"

5/27/22, 10:10 AM

Future Plans

Ground-based CMB experiments are evolving from fielding thousands of detectors on telescope(s) of a single size at a single observing site in the last decade (eg. the Atacama Cosmology Telescope, BICEP/Keck, Polarbear/Simons Array, and South Pole Telescope), through tens of thousands of detectors on telescopes of multiple sizes at a single observing site in this decade (the South Pole...

161. Invited talk by Mark Devlin (UPenn) on "All the Way from Earth to Space. How Earth-based, sub-orbital, and space missions are complimenting each other with precision measurements of the millimeter sky"

5/27/22, 10:50 AM

Future Plans

164. Discussion EOM (Charles R. Lawrence, Francois R. Bouchet)

5/27/22, 11:10 AM

Future Plans

Choose timezone

From Planck to the future of CMB