Typo in institution name

docs/papers.yml

@@ -166,7 +166,7 @@ papers:
       4: Columbia University
       5: Cornell University
       6: University of Connecticut
-      7: Havard University
+      7: Harvard University
     link: https://arxiv.org/abs/2201.01305
     abstract: "Complex systems (stars, supernovae, galaxies, and clusters) often exhibit low scatter relations between observable properties (e.g., luminosity, velocity dispersion, oscillation period, temperature). These scaling relations can illuminate the underlying physics and can provide observational tools for estimating masses and distances. Machine learning can provide a fast and systematic way to search for new scaling relations (or for simple extensions to existing relations) in abstract high-dimensional parameter spaces. We use a machine learning tool called symbolic regression (SR), which models the patterns in a given dataset in the form of analytic equations. We focus on the Sunyaev-Zeldovich flux-cluster mass relation (Y-M), the scatter in which affects inference of cosmological parameters from cluster abundance data. Using SR on the data from the IllustrisTNG hydrodynamical simulation, we find a new proxy for cluster mass which combines $Y_{SZ}$ and concentration of ionized gas (cgas): $M \\propto Y_{\\text{conc}}^{3/5} \\equiv Y_{SZ}^{3/5} (1 - A c_\\text{gas})$. Yconc reduces the scatter in the predicted M by ~ 20 - 30% for large clusters ($M > 10^{14} M_{\\odot}/h$) at both high and low redshifts, as compared to using just $Y_{SZ}$. We show that the dependence on cgas is linked to cores of clusters exhibiting larger scatter than their outskirts. Finally, we test Yconc on clusters from simulations of the CAMELS project and show that Yconc is robust against variations in cosmology, astrophysics, subgrid physics, and cosmic variance. Our results and methodology can be useful for accurate multiwavelength cluster mass estimation from current and upcoming CMB and X-ray surveys like ACT, SO, SPT, eROSITA and CMB-S4."
     image: SyReg_GasConc.png
@@ -192,7 +192,7 @@ papers:
       5: Flatiron Institute
       6: Yale University
       7: University of Connecticut
-      8: Havard University
+      8: Harvard University
     link: https://arxiv.org/abs/2209.02075
     abstract: "Ionized gas in the halo circumgalactic medium leaves an imprint on the cosmic microwave background via the thermal Sunyaev-Zeldovich (tSZ) effect. Feedback from active galactic nuclei (AGN) and supernovae can affect the measurements of the integrated tSZ flux of halos ($Y_{SZ}$) and cause its relation with the halo mass ($Y_{SZ}-M$) to deviate from the self-similar power-law prediction of the virial theorem. We perform a comprehensive study of such deviations using CAMELS, a suite of hydrodynamic simulations with extensive variations in feedback prescriptions. We use a combination of two machine learning tools (random forest and symbolic regression) to search for analogues of the $Y-M$ relation which are more robust to feedback processes for low masses ($M \\leq 10^{14} M_{\\odot}/h$); we find that simply replacing $Y \\rightarrow Y(1+M_\\ast/M_{\\text{gas}})$ in the relation makes it remarkably self-similar. This could serve as a robust multiwavelength mass proxy for low-mass clusters and galaxy groups. Our methodology can also be generally useful to improve the domain of validity of other astrophysical scaling relations. We also forecast that measurements of the Y-M relation could provide percent-level constraints on certain combinations of feedback parameters and/or rule out a major part of the parameter space of supernova and AGN feedback models used in current state-of-the-art hydrodynamic simulations. Our results can be useful for using upcoming SZ surveys (e.g. SO, CMB-S4) and galaxy surveys (e.g. DESI and Rubin) to constrain the nature of baryonic feedback. Finally, we find that the an alternative relation, $Y-M_{\\ast}$, provides complementary information on feedback than $Y-M$."
     image: Y_Mgal_Simba.png