Significant progress by experiments trying to detect the Global 21cm signal from neutral hydrogen in the intergalactic medium during the Dark Ages, Cosmic Dawn, and the Epoch of Reionization (z>6) has increased the attention on this measurement from the Astrophysics, Particle Physics, and Cosmology communities. In particular, the EDGES experiment has reported an absorption feature that could correspond to the Global 21cm signal, but which is significantly deeper than theoretical models and has other characteristics that depart from expectations. Instrumental calibration, foreground removal, radio-frequency interference, and ionospheric effects remain as issues that transform this measurement into a daunting experimental effort.
In light of the above, we will host the Second Global 21cm Workshop at McGill University on October 7th-9th, 2019. This workshop will serve as a forum to discuss recent progress from all the Global 21cm experiments. We will have talks about theory, data analysis, and, above all, instrumental development and field work. We will also host several discussion sessions expecting the most important aspects and concerns being raised and addressed.
We look forward to great updates and enlightening interactions, debates, and lessons.
Date | Message |
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2019-03-26 | Preliminary communication with different global 21cm experiments and researchers. |
2019-04-12 | First announcement sent out to invitees. |
2019-06-21 | Reminders sent out to invitees who had not replied. |
2019-07-14 | Asked invitees if invitation letter is needed. |
2019-08-05 | Logistics information uploaded to webpage. |
2019-09-07 | Email sent out to ask for talk titles and dietary restrictions. |
2019-09-24 | Reminder email sent out to ask for talk titles and dietary restrictions. |
2019-10-01 | Workshop agenda emailed and posted on the website. |
2019-10-03 | Agenda updated with modifications on Oct 9th. |
2019-10-04 | Email sent out with logistics details and agenda updates. |
2019-10-16 | Talks uploaded to webpage. |
Name | Institution |
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Dominic Anstey | Cambridge |
John Barrett | Haystack |
Joelle Bégin | McGill |
Gianni Bernardi | INAF Bologna |
Judd Bowman | ASU |
Robert Brandenberger | McGill |
Paula Boubel | McGill |
Ricardo Bustos | U.C. Santísima Concepción |
H. Cynthia Chiang | McGill |
Bryce Cyr | McGill |
Abhirup Datta | IIT Indore |
Mauricio Díaz | U.C. Santísima Concepción |
Taj Dyson | McGill |
Eloy de Lera Acedo | Cambridge |
Matt Dobbs | McGill |
Aaron Ewall-Wice | U. Berkeley |
Anastasia Fialkov | Cambridge |
Samuel Gagnon-Hartman | McGill |
Vera Gluscevic | U. Southern California |
Oscar Hernández | McGill |
José Miguel Jáuregui | CITA |
Zarif Kader | McGill |
Alexander Kaurov | IAS |
Girish Kulkarni | Tata Institute of Fundamental Research |
Adam Lidz | U. Pennsylvania |
Adrian Liu | McGill |
Colin Lonsdale | Haystack |
Nivedita Mahesh | ASU |
Tristan Menard | McGill |
Ben McKinley | Curtin U. |
Jordan Mirocha | McGill |
Raul Monsalve | McGill |
Julian Muñoz | Harvard |
Steven Murray | ASU |
Olga Navros | Carnegie Mellon |
Bang Nhan | NRAO Charlottesville |
Deniz Ölçek | McGill |
Matheus Pessôa | McGill |
Jeff Peterson | Carnegie Mellon |
David Rapetti | U. Colorado Boulder |
Nima Razavi-Ghods | Cambridge |
Alan Rogers | Haystack |
Seth Siegel | McGill |
Jonathan Sievers | McGill |
Peter Sims | Brown U. |
Saurabh Singh | McGill |
Marta Spinelli | INAF Trieste |
Mayuri S. Rao | Raman Research Institute |
Ravi Subrahmanyan | Raman Research Institute |
Keith Tauscher | U. Colorado Boulder |
Fernando Zago | McGill |
French is the official language in Quebec but Montreal is very much a bilingual city, with English being widely spoken. You are likely to be greeted with "Bonjour hi" or "Salut hi" and your response will dictate the language you prefer to communicate in.
The Montreal Trudeau International Airport is located ~20 km from McGill.
Airbnb is another possibility, with good options in the ~$100/night range. If you venture outside of downtown to The Plateau, Mile End, or Gay Village neighborhoods (just north/northwest of downtown), McGill is a longer walk (~30-40 min) but still easily accessible by bus or Metro.
A typical day in October has low temperatures around 5°C and highs around 15°C (40°F-60°F). Rain is common but snow is unlikely.
You are free for breakfast each day, as well as dinner on Monday and Wednesday.
Click HERE for an interactive map of Restaurants and Sightseeing around McGill and in MontrealWe also list these spots below.
Coffee Shops:
Lunch (quick):
Lunch/Dinner:
Bars/Pubs/Cocktails:
Famous Montreal Establishments:
Sightseeing:
Mount-Royal (Mont-Royal) is a large hill located in the middle of Montreal. The city is named after this 761 foot hill, which also houses the famous Mount-Royal Park (Parc du Mont-Royal), one of Montreal's largest green spaces. From the top of Mount-Royal, you will get some impressive views of downtown Montreal and the surrounding area.
The church features two soaring towers and stands as a dramatic example of the Gothic Revival style. Its grand interior is filled with hundreds of intricate wooden carvings and religious statues, as well as a Casavant Freres pipe organ that dates back to 1891.
Old Montreal is a part of downtown Montreal that has been preserved in much of its original state, with the oldest buildings dating back to the 1600's. Visitors can appreciate Old Montreal by merely wandering the streets and stumbling upon its delightful nooks and crannies. The Old Montreal website has a well laid out and thorough self-guided walking tour of Old Montreal, complete with photos and maps.
Founded in 1860, it has grown into one of the most visited museums in North America; it hosts around 43,000 works from antiquity to today, much of it on display throughout five pavilions. The enormous institution also hosts seasonal blockbuster exhibitions.
Pointe-a-Calliere is the largest archaeology museum in Canada, and is built atop the historic Old Montreal sites. It hosts an impressive collection of excavated remains of the original settlement. Pointe-a-Calliere also presents three to four temporary exhibitions every year.
It is Canada's largest church and claims to have one of the largest domes in the world. The shrine includes a majestic building, the small original chapel, a votive chapel, a crypt, gardens of the way of the cross, and a basilica that can accommodate close to 2,000 people.
The Montreal Space for Life, home to the Biodome, Insectarium, Rio Tinto Alcan Planetarium, and Botanical Garden, is the largest natural science museum complex in Canada. Don't miss the "Gardens of Light" lantern festival held annually at the Botanical Garden.
It is one of the largest open-air markets in North America. The market, which consists of small shopkeepers, bustles with activity year-round; you'll find local fruit and vegetable growers, butchers, bakers, fishmongers, grocers, and restaurateurs.
Please click here to view and download the workshop agenda.
SESSION 1 9:00am-10:40am | |
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Vera Gluscevic | Dark matter throughout cosmic history |
Adam Lidz | The 21 cm signal and fuzzy dark matter |
Jordan Mirocha | The global 21-cm signal in the context of high-z galaxy surveys |
Girish Kulkarni | Hints of a concordant reionization model from the Lyman-alpha forest |
SESSION 2 11:00am-12:20pm | |
Saurabh Singh | SARAS: evolution of system design and related challenges |
Ravi Subrahmanyan | SARAS 3 |
SESSION 3 1:40pm-3:20pm | |
Judd Bowman | EDGES overview |
Nivedita Mahesh | EDGES beam modelling and data comparison |
Raul Monsalve | EDGES Mid-Band analysis |
Alan Rogers | Update on EDGES-3 |
SESSION 4 3:40pm-5:20pm | |
Steven Murray | Making EDGES bayesian |
Peter Sims | The impact of calibration errors on 21 cm global experiments: a bayesian case study with EDGES |
Keith Tauscher | Moving away from analytical a priori foreground models in signal extraction |
David Rapetti | Rigorously extracting and constraining global 21-cm signal model parameters |
Abhirup Datta | Global 21cm signal estimation using neural networks |
SESSION 5 9:00am-10:20am | |
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Julian Muñoz | Dark matter and the 21-cm global signal |
Aaron Ewall-Wice | Can we explain the EDGES Feature with Black Holes? |
Alexander Kaurov | Implication of the shape of the EDGES signal for the 21 cm power spectrum |
SESSION 6 11:00am-12:20pm | |
H. Cynthia Chiang | Observing the < 100 MHz radio sky from the sub-Antarctic and Arctic |
José Miguel Jáuregui | HIBiscus and Mango-Peel antennas |
Jonathan Sievers | Beam chromaticity with gaussian random fields |
SESSION 7 1:40pm-3:20pm | |
O. Navros | High-Z |
Jeff Peterson | Test of long dipole on the soil at Karoo |
Gianni Bernardi | LEDA status update |