4th ASI/COSMOS Workshop: Ground-based CMB experiments

Contribution List

1. welcome

04/03/2019, 09:00

2. The COSMOS program

Nicola Vittorio (ROMA2)

04/03/2019, 09:05

Introduction

3. CMB ground-based experiments: European and International context

Marco Bersanelli (MI)

04/03/2019, 09:30

Introduction

4. Foregrounds at low frequencies

Nicoletta Krachmalnicoff (Sissa)

04/03/2019, 09:55

Introduction

5. STRIP: the ground-based instrument of LSPE

Fabrizio Villa (INAF / IASF-Bologna)

04/03/2019, 10:50

Ground-based experiments in Italy and in Europe

6. QUBIC: status and perspectives

Stephen Torchinski

04/03/2019, 11:15

Ground-based experiments in Italy and in Europe

7. QUIJOTE and TMS

José Alberto Rubiño-Martin

04/03/2019, 11:40

Ground-based experiments in Italy and in Europe

8. C-BASS

Angela Taylor

04/03/2019, 12:05

Ground-based experiments in Italy and in Europe

9. Low frequency efforts in Germany

Aritra Basu

04/03/2019, 14:00

Ground-based experiments in Italy and in Europe

10. SPASS & future prospects

Ettore Carretti

04/03/2019, 14:25

Ground-based experiments in Italy and in Europe

11. COSMO: spectral measurements from Dome C

Paolo De Bernardis (ROMA1)

04/03/2019, 14:50

Ground-based experiments in Italy and in Europe

12. Short-Mid Term (2023): STRIP-2

Cristian Franceschet, Stefano Mandelli

04/03/2019, 15:40

Future Perspectives

• STRIP2 design options (KIDs or TES at W band)
• Atmospheric monitor

13. Long Term (2027): European Low Frequency Survey (ELFS)

Mike Jones, Carlo Baccigalupi (TS), Marco Bersanelli (MI), Aniello Mennella (MI), José Alberto Rubiño-Martin

04/03/2019, 16:05

Future Perspectives

• Full sky, 5-120GHz, HEMTs + KIDs
• Two large Aperture Telescope (6-m class)
• Sites: Tenerife (North) and TBC [Lliama, Atacama, SP] (South)

14. Participation in US-led efforts

Federico Nati

04/03/2019, 16:30

Future Perspectives

• Simons Array, Simons Observatory, Stage IV s
• Low frequency array for South Pole LAT to observe Bicep2 region?
• STRIP focal plane to be re-used at SP (SPT or Euro LAT)

15. SRT as follow up of CMB measurements

Alessandro Navarrini

04/03/2019, 16:55

Future Perspectives

16. HEMTS in Europe

Ernesto Limiti

05/03/2019, 09:00

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

17. TES: applications to W band and below

Flavio Gatti (GE)

05/03/2019, 09:25

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

18. KIDs for W band in Italy

Alessandro Paiella (ROMA1)

05/03/2019, 09:50

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

19. KIDs for W band in France

Alessandro Monfardini (CNRS Grenoble)

05/03/2019, 10:15

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

21. Antenna systems and characterization through UAV

Giuseppe Virone, Oscar Peverini (IEIIT - CNR)

05/03/2019, 11:10

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

22. Optical design

Sabrina Realini, Maura Sandri (INAF - IASF Bologna)

05/03/2019, 11:35

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

23. Calibration and testing

Mario Zannoni (MIB), Francesco Cuttaia (INAF - IAFS - Bologna), Cristian Franceschet

05/03/2019, 12:00

Technology to support future CMB experiments (focus on STRIP2 and ELFS)

24. Computing infrastructure in Europe, challenges in data analysis

Francesco Piacentini (ROMA1), Paolo Natoli (FE), Maurizio Tomasi (MI), Andrea Zacchei (INAF-OATs)

05/03/2019, 14:30

Data analysis and performance forecast

25. Defining the Scientific Requirements for ELFS

Carlo Baccigalupi (Sissa)

05/03/2019, 14:55

Data analysis and performance forecast

-Preliminary requirements (present status)
-Coordination of future work to fully establish ELFS requirements