• All Publications (ADS, PDF)
• Total Publications: 111
• Total Cititations: >8400
• h-index: 42

First (12) and Second (10) Authored Publications:

  1. Jin, Xiangyu; Yang, Jinyi; Fan, Xiaohui et al., 2024, ApJ, A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [OIII] Emitters (first author is grad student working with J. Yang)

  2. Wang, Feige; Yang, Jinyi; Hennawi, Joseph F., et al., 2024, ApJL, A Massive Protocluster Anchored by a Luminous Quasar at z = 6.63

  3. Wang, Feige; Yang, Jinyi; Fan, Xiaohui et al., 2024, ApJ, A Spatially Resolved [C II] Survey of 31 z ∼ 7 Massive Galaxies Hosting Luminous Quasars

  4. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2023, ApJL, A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars using JWST

  5. Wang, Feige; Yang, Jinyi; Hennawi, Joseph F. et al., 2023, ApJL, A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar

  6. Yang, Jinyi; Fan, Xiaohui; Gupta, Ansh et al., 2023, ApJS, Accepted, DESI z ≳ 5 Quasar Survey. I. A First Sample of 400 New Quasars at z ∼ 4.7 - 6.6

  7. Jin, Xiangyu; Yang, Jinyi; Fan, Xiaohui et al., 2023, ApJ, (Nearly) Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at z ∼ 5 - 7 Using Dark Pixel Fractions in Ly-alpha and Ly-beta Forests (first author is grad student working with J. Yang)

  8. Yang, Jinyi; Fan, Xiaohui; Wang, Feige et al., 2022, ApJL Deep XMM-Newton Observation of a X-ray Weak, Broad Absorption Line Quasar at z=6.5

  9. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2021, ApJ Probing Early Super-massive Black Hole Growth and Quasar Evolution with Near-infrared Spectroscopy of 37 Reionization-era Quasars at 6.3 < z ≤ 7.64

  10. Yue, Minghao; Yang, Jinyi; Fan, Xiaohui et al., 2021, ApJ ALMA Observations of the Sub-kpc Structure of the Host Galaxy of a z = 6.5 Lensed Quasar: A Rotationally-Supported Hyper-Starburst System at the Epoch of Reionization (first author is grad student working with J. Yang)

  11. Wang, Feige; Yang, Jinyi; Fan, Xiaohui et al., 2021, ApJL A Luminous Quasar at Redshift 7.642

  12. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2020, ApJL Pōnuiā‘ena: A Luminous z=7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole

  13. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2020, ApJ Measurements of the z ~ 6 Intergalactic Medium Optical Depth and Transmission Spikes Using a New z > 6.3 Quasar Sample

  14. Yang, Jinyi; Venemans, Bram; Wang, Feige et al., 2019, ApJ Far-infrared Properties of the Bright, Gravitationally Lensed Quasar J0439+1634 at z = 6.5

  15. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2019, AJ Exploring Reionization-era Quasars. IV. Discovery of Six New z ≳ 6.5 Quasars with DES, VHS, and unWISE Photometry

  16. Wang, Feige; Yang, Jinyi; Fan, Xiaohui et al., 2019, ApJ Exploring Reionization-Era Quasars III: Discovery of 16 Quasars at 6.4≲z≲6.9 with DESI Legacy Imaging Surveys and UKIRT Hemisphere Survey and Quasar Luminosity Function at z∼6.7

  17. Yang, Jinyi; Wang, Feige; Fan, Xiaohui et al., 2019, ApJ Filling in the Quasar Redshift Gap at z ∼ 5.5. II. A Complete Survey of Luminous Quasars in the Post-reionization Universe

  18. Wang, Feige; Yang, Jinyi; Fan, Xiaohui et al., 2018, ApJ The Discovery of a Luminous Broad Absorption Line Quasar at a Redshift of 7.02

  19. Yang, Jinyi; Wu, Xue-Bing; Liu, Dezi et al., 2018, AJ Deep CFHT Y-band Imaging of VVDS-F22 Field. II. Quasar Selection and Quasar Luminosity Function

  20. Liu, Dezi; Yang, Jinyi; Yuan, Shuo et al., 2017, AJ Deep CFHT Y-band Imaging of VVDS-F22 Field. I. Data Products and Photometric Redshifts

  21. Yang, Jinyi; Fan, Xiaohui; Wu, Xue-Bing et al., 2017, AJ Discovery of 16 New z ∼ 5.5 Quasars: Filling in the Redshift Gap of Quasar Color Selection

  22. Yang, Jinyi; Wang, Feige; Wu, Xue-Bing et al., 2016, ApJ A Survey of Luminous High-redshift Quasars with SDSS and WISE. II. the Bright End of the Quasar Luminosity Function at z ≈ 5