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Probabilistic Random Forest: A machine learning algorithm for noisy datasets
TLDR
Effectively using unsupervised machine learning in next generation astronomical surveys
- I. Reis, Michael Rotman, D. Poznanski, J. Prochaska, L. Wolf
- PhysicsAstron. Comput.
- 15 November 2019
The subtlety of Ly α photons: changing the expected range of the 21-cm signal
- I. Reis, A. Fialkov, R. Barkana
- PhysicsMonthly Notices of the Royal Astronomical Society
- 5 January 2021
We present the evolution of the 21-cm signal from cosmic dawn and the epoch of reionization (EoR) in an upgraded model including three subtle effects of Ly α radiation: Ly α heating, CMB heating…
Detecting outliers and learning complex structures with large spectroscopic surveys - a case study with APOGEE stars
- I. Reis, D. Poznanski, D. Baron, G. Zasowski, S. Shahaf
- Computer Science, Physics
- 31 October 2017
In this work we apply and expand on a recently introduced outlier detection algorithm that is based on an unsupervised random forest. We use the algorithm to calculate a similarity measure for…
Self-organized topological state in a magnetic chain on the surface of a superconductor
- I. Reis, D. Marchand, M. Franz
- Physics
- 19 June 2014
Electronic states associated with a chain of magnetic adatoms on the surface of an ordinary s- wave superconductor have been shown theoretically to form a one dimensional topological phase with…
HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization
- The Hera Collaboration Zara Abdurashidova, J. Aguirre, Haoxuan Zheng
- PhysicsThe Astrophysical Journal
- 16 August 2021
Recently, the Hydrogen Epoch of Reionization Array (HERA) has produced the experiment’s first upper limits on the power spectrum of 21 cm fluctuations at z ∼ 8 and 10. Here, we use several…
Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations
- I. Reis, R. Barkana, A. Fialkov
- PhysicsMonthly Notices of the Royal Astronomical Society
- 24 June 2021
The 21-cm signal from cosmic dawn and the epoch of reionization (EoR) probes the characteristics of the high redshift galaxy population. Many of the astrophysical properties of galaxies at high…
Redshifted broad absorption line quasars found via machine-learned spectral similarity
- I. Reis, D. Poznanski, P. Hall
- PhysicsMonthly Notices of the Royal Astronomical Society
- 24 May 2018
We report the discovery of 31 new redshifted broad absorption line quasars (RSBALs) from the Sloan Digital Sky Survey (SDSS). The number of previously known such objects is 19. The identification of…
High-redshift radio galaxies: a potential new source of 21-cm fluctuations
- I. Reis, A. Fialkov, R. Barkana
- Physics
- 10 August 2020
Radio sources are expected to have formed at high redshifts, producing an excess radiation background above the cosmic microwave background (CMB) at low frequencies. Their effect on the redshifted…
Effect of the cosmological transition to metal-enriched star-formation on the hydrogen 21-cm signal
- M. Magg, I. Reis, A. Schauer
- PhysicsMonthly Notices of the Royal Astronomical Society
- 29 October 2021
Mapping Cosmic Dawn with 21-cm tomography offers an exciting new window into the era of primordial star formation. However, self-consistent implementation of both the process of star formation and…
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