Universe after the first 200 million years
Cosmic Dawn, Reionization and Post reionization with 21cm
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11-13 December, 2017, Presidency University, Kolkata
Conference Schedule (Download the PDF version)
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Venue: A J C Seminar room, Main Building, Presidency University
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11th December (Monday)
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09.30-10.00: Inaugural Session
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Tea Break
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10.30-11.10: Global 21-cm signal from Cosmic Dawn and Epoch of Reionization
Ravi Subrahmanyan (IR) [Slides]
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11.10-11.35: Imprints of recombination history of the Universe on HI 21-cm signal during dark ages
Mayuri S. Rao (IT) [Slides]
11.35-11.55: Foreground Subtraction in redshifted 21cm Global Signal Experiments using Artificial Neural Networks
Madhurima Choudhury [Slides]
11.55-12.20: Simulations of the post-EoR HI signal
Nishikant Khandai (IT) [Slides]
12.20-12.45: Probing the post reionization epoch with Ooty Wide-Field Array: Challenges in detecting redshifted 21-cm signal
Visweshwar Ram Marthi (IT) [Slides]
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Lunch Break
1.40-2.20: Towards accurate modelling HI 21-cm signal from cosmic dawn and reionization: Current status and challenges
Tirthankar Roy Choudhury (IR) [Slides]
2.20-2.40: Reionization constraints after Planck
Sourav Mitra (IT) [Slides]
2.40-3.00: Measuring the reionization 21cm fluctuations using clustering wedges
Dinesh Raut [Slides]
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Break due to a University event (3.00-4.20pm)
A talk on "Mahalanobis & Fisher: Mathematical Statistics As A Global Enterprise" by
Prof. STEPHEN STIGLER (see here for details)
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Post Tea Session
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4.20-4.40: Analytically Modelling 21-cm Signal from Early Phase of Epoch of Reionization
Jankee Raste [Slides]
4.40-5.00: Enhanced 21cm Power Spectrum due to inhomogeneous CMB heating during Dark Ages
Sioree Ansar [Slides]
5.00-5.20: Impact of Non-Gaussianity for Parameter Estimation from the EoR 21cm Signal
Avinash K. Shaw [Slides]
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12th December (Tuesday)
9.30-9.55: Probing the epoch of reionization using Minkowski Tensors
Pravabati Chingangbam (IT) [Slides]
9.55-10.15: 3D Minkowski Tensors as a probe of Epoch of Reionization
Akanksha Kapahtia [Slides]
10.15-10.40: The epoch of reionization through HI 21-cm bispectrum
Suman Majumdar (IT) [Slides]
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Tea Break
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11.10-11.35: Probing epoch of reionization with SKA1-low: An Indian perspective
Abhirup Datta (IT) [Slides]
11.35-11.55: Searching for sources at the Cosmic Dawn using redshifted 21cm signal
Raghunath Ghara (IT) [Slides]
11.55-12.20: Extracting the HI power spectrum from the EoR using the MWA
Sourabh Paul (IT) [Slides]
12.20-12.40: On detecting EoR using drift scan data from MWA
Akash Kumar Patwa [Slides]
Lunch Break
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2.15-2.55: Interferometric detection of cosmological 21-cm signal: Challenges and prospects
Somnath Bharadwaj (IR) [Slides]
2.55-3.20: The Tapered Gridded Estimator (TGE): A novel technique to estimate power spectrum from radio-interferometric data
Samir Choudhuri (IT) [Slides]
3.20-3.45: Characterizing Foregrounds in 21 cm Cosmology Observation with the uGMRT at 300-500 MHz
Arnab Chackraborty [Slides]
Tea Break
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4.15-4.35: Probing the epoch of reionization with the galaxy luminosity function
Saumyadeep Samui (IT) [Slides]
4.35-4.55: Non-linear clustering of high-z dark matter halos and galaxies
Charles Jose (IT) [Slides]
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4.55-5.15 Conditional HI Mass Function and Clustering in the Local Universe
Saili Dutta [Slides]
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13th December (Wednesday)
9.30-9.55: Prospect for detecting of the cosmological HI signal with Ooty Wide-Field Array
Sk. Saiyad Ali (IT) [Slides]
9.55-10.15: A study of the effectiveness of the TGE in suppressing the point source contamination in detecting the 21-cm EoR signal
Srijita Pal [Slides]
10.15-10.35: Spherical Harmonic Analysis of HI 21-cm Visibility and Visibility Correlation
Suman Chatterjee [Slides]
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Tea Break
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11.30-11.55: Future Constraints on Dark Energy using 21cm observations with SKA1-mid
Bikash Dinda [Slides]
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11.55-12.15: Prospects of probing quintessence with H I 21-cm intensity mapping survey
Azam Hussain [Slides]
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12.15-12.35: Modelling redshift-space distortion (RSD) in the post-reionization HI 21-cm power spectrum
Debanjan Sarkar [Slides​]
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12.35-12.55: Predictions for detecting the cross correlation signal using OWFA
Anjan Sarkar [Slides]
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Lunch Break
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2.25 - 3.50: Discussion session on Future plans with GMRT, OWFA, SARAS, SKA India EoR/Cosmology
3.50 - 4.00: Vote of thanks
IR: Invited Review talk
IT: Invited focussed talk