The 3rd Shanghai Assembly on Cosmology and Structure Formation

Session

Cosmology 6

Nov 20, 2025, 3:50 PM

Tianwen Hall

Conveners

Cosmology 6

• Kwan Chuen Chan (Sun-Yat Sen University)

Description

systematics

58. Enhancing DESI DR1 Full-Shape Analysis

Hanyu Zhang (University of Waterloo)

11/20/25, 3:50 PM

Cosmology and Large-scale Structure

Talk

DESI DR1 full-shape clustering constrains cosmology from linear to quasi-nonlinear scales but is vulnerable to projection effects from broad nuisance priors. We strengthen the analysis along three axes: (i) HOD-informed priors (HIP), calibrated on high-fidelity mocks, to anchor nuisance parameters to realistic galaxy–halo connections; (ii) nonlinear reparameterization of the nuisance sector...

64. Will ignoring PNG in the covariance affect the measurement of $f_{NL}$ ?

Zhuoyang Li (Tsinghua University)

11/20/25, 4:10 PM

Cosmology and Large-scale Structure

Talk

Primordial non-Gaussianity​ is one of the most important signals for probing the physics of the early universe. Over the past decade, constraints on primordial non-Gaussianity (quantified by the parameter fNL​) from the Planck experiment have ruled out a number of simple inflationary models. In the coming years, ongoing and upcoming large-scale structure (LSS) surveys (e.g., SPHEREx) will...

45. Reconstructing redshift distributions with photometric galaxy clustering

Hui Peng (Shanghai Jiao Tong University)

11/20/25, 4:25 PM

Cosmology and Large-scale Structure

Talk

The accurate determination of the true redshift distributions in tomographic bins is critical for cosmological constraints from photometric surveys. We developed a redshift self-calibration method, which utilizes the photometric galaxy clustering alone, is highly convenient and avoids the challenges from incomplete or unrepresentative spectroscopic samples in external calibration. By refining...

10. Clustering redshifts with Lyman-alpha forest: calibrating the high redshift tail with DESI for Stage IV photometric surveys

Qianjun Hang

11/20/25, 4:40 PM

Cosmology and Large-scale Structure

Talk

Stage IV surveys such as Euclid and LSST will have unprecedented constraining power in cosmological parameters. To achieve this scientific goal, one of the major sources of uncertainties, photometric redshifts of the galaxy sample, needs to be under control. Clustering redshift has been a promising method for photometric redshift calibration, as have been adopted in many stage III surveys, but...

56. KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects

Ziang Yan (Ruhr University Bochum)

11/20/25, 4:55 PM

Cosmology and Large-scale Structure

Talk

Photometric galaxy surveys, despite their limited resolution along the line of sight, encode rich information about the large-scale structure (LSS) of the Universe thanks to the high number density and extensive depth of the data. However, the complicated selection effects in wide and deep surveys can potentially cause significant bias in the angular two-point correlation function (2PCF)...

88. Probing Light Dark Matter with Cosmic Gravitational Focusing

Liang Tan (Tsung-Dao Lee Institute)

11/20/25, 5:10 PM

Cosmology and Large-scale Structure

Talk

We investigate the possibility of using the cosmic gravitational focusing (CGF) to probe the minor light dark matter (DM) component whose mass is in the range of $(0.1 \sim 100)$\,eV. Being a purely gravitational effect, the CGF offers a mode-independent probe that is complementary to the existing ways such as Lyman-$\alpha$ and $\Delta N_{\rm eff}$. Such effect finally leads to a dipole...