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1. The DESI One-Percent Survey: A Concise Model for the Galactic Conformity of Emission-line Galaxies

2. Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

3. Photometric Objects Around Cosmic Webs (PAC). VI. High Satellite Fraction of Quasars

4. PAC. V. The Roles of Mass and Environment in the Quenching of Galaxies

5. The Early Data Release of the Dark Energy Spectroscopic Instrument

6. Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter

7. Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High-precision Constraints on the Evolution of the Stellar–Halo Mass Relation at Redshift z < 0.7

8. Mass Dependence of Galaxy–Halo Alignment in LOWZ and CMASS

9. Physical Evolution of Dark Matter Halo around the Depletion Boundary

10. The DESI One-Percent Survey: Constructing Galaxy–Halo Connections for ELGs and LRGs Using Auto and Cross Correlations

11. Toward a Physical Understanding of Galaxy–Halo Alignment

12. Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument

13. Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys

14. Construct the emission line galaxy-host halo connection through auto and cross correlations

15. Environmental dependence of cold dark matter halo formation

16. Semianalytical Model of Galaxy Formation with High‐ResolutionN‐Body Simulations

17. The Nonlinear Evolution of the Bispectrum in Scale‐freeN‐Body Simulations

18. What X-rays tell us about dark matter halos

19. Formation time-distribution of dark matter haloes: theories versus N-body simulations

20. Substructures and density profiles of clusters in models of galaxy formation

21. Effects of dark sectors' mutual interaction on the growth of structures

22. Merger time scale of galaxies

23. The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models

24. Velocity of galaxies with different luminosity

25. Warm Dark Matter Model of Galaxy Formation

26. Scaling properties of the redshift power spectrum: theoretical models

27. Large Cosmological N-Body Simulations and Clustering of Dark Matter Halos

28. Three-point correlation function of galaxy clusters in cosmological models: a strong dependence on triangle shape

29. PHOTOMETRIC PROPERTIES AND LUMINOSITY FUNCTION OF NEARBY MASSIVE EARLY-TYPE GALAXIES.

31. PURIFICATION AND CHARACTERIZATION OF A THERMAL STABLE ANTIMICROBIAL PROTEIN FROM HOUSEFLY LARVAE, MUSCA DOMESTICA, INDUCED BY ULTRASONIC WAVE.

32. The dependence of the galaxy luminosity function on large-scale environment.

33. The cluster-cluster correlation in hybrid models

34. The power spectra of IRAS galaxies and of Abell clusters

35. On the error estimates of correlation functions

36. Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys. I. Tests with Mock Catalogs.

37. Determination of Dark Matter Halo Mass from Dynamics of Satellite Galaxies.

38. Constraining the H i–Halo Mass Relation from Galaxy Clustering.

39. ELUCID—Exploring the Local Universe with the reConstructed Initial Density Field. II. Reconstruction Diagnostics, Applied to Numerical Halo Catalogs.

40. MEASUREMENT OF A REDSHIFT-SPACE POWER SPECTRUM FOR BOSS GALAXIES AND THE GROWTH RATE AT REDSHIFT 0.57.

41. ELUCID—EXPLORING THE LOCAL UNIVERSE WITH RECONSTRUCTED INITIAL DENSITY FIELD. III. CONSTRAINED SIMULATION IN THE SDSS VOLUME.

42. CLUSTERING PROPERTIES AND HALO MASSES FOR CENTRAL GALAXIES IN THE LOCAL UNIVERSE.

43. AN EXTENDED VIEW OF THE PISCES OVERDENSITY FROM THE SCUSS SURVEY.

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