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Constraining gravity at the largest scales through CMB lensing and galaxy velocities

Monthly notices of the Royal Astronomical Society, 2016-08, Vol.460 (4), p.4098-4108

2016

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CROSS-CORRELATIONS AS A COSMOLOGICAL CARBON MONOXIDE DETECTOR

The Astrophysical journal, 2013-05, Vol.768 (1), p.1-15

2013

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Calibrating magnification bias for the EG statistic to test general relativity

Monthly notices of the Royal Astronomical Society, 2018-12, Vol.481 (2), p.1441-1454

2018

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Probing gravity at large scales through CMB lensing

Monthly notices of the Royal Astronomical Society, 2015-06, Vol.449 (4), p.4326-4335

2015

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Characterizing the Conditional Galaxy Property Distribution Using Gaussian Mixture Models

The Astrophysical journal, 2023-06, Vol.950 (2), p.159

2023

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Evidence for C ii diffuse line emission at redshift z ∼ 2.6

Monthly notices of the Royal Astronomical Society. Letters, 2019-10, Vol.489 (1), p.L53-L57

2019

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Removing interlopers from intensity mapping probes of primordial non-Gaussianity

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.512 (3), p.4262-4271

2022

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INTENSITY MAPPING ACROSS COSMIC TIMES WITH THE Lyα LINE

The Astrophysical journal, 2014-05, Vol.786 (2), p.1-16

2014

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Non-detection of a statistically anisotropic power spectrum in large-scale structure

Journal of cosmology and astroparticle physics, 2010-05, Vol.2010 (5), p.27-27

2010

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New Probe of the High-z Baryon Acoustic Oscillation Scale: BAO Tomography with CMB×LIM-Nulling Convergence

Physical review letters, 2024-06, Vol.132 (24), p.241001, Article 241001

2024

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Full-sky lensing reconstruction of 21 cm intensity maps

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.488 (2), p.1828-1845

2019

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Constraining the star formation rate using joint CIB continuum and C ii intensity mapping

Monthly notices of the Royal Astronomical Society, 2023-10, Vol.524 (4), p.5254-5265

2023

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An Empirical Representation of a Physical Model for the ISM [C ii], CO, and [C i] Emission at Redshift 1 ≤ z ≤ 9

The Astrophysical journal, 2022-04, Vol.929 (2), p.140

2022

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A new calibration method of sub-halo orbital evolution for semi-analytic models

Monthly notices of the Royal Astronomical Society, 2020-11, Vol.498 (3), p.3902-3913

2020

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Multitracer Cosmological Line Intensity Mapping Mock Light-cone Simulation

The Astrophysical journal, 2021-04, Vol.911 (2), p.132

2021

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Systematic Effects in Large-Scale Angular Power Spectra of Photometric Quasars and Implications for Constraining Primordial Non-Gaussianity

Publications of the Astronomical Society of the Pacific, 2013-06, Vol.125 (928), p.705-718

2013

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Quantifying the power spectrum of small-scale structure in semi-analytic galaxies

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.488 (4), p.5085-5092

2019

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On Estimating the Cosmic Molecular Gas Density from CO Line Intensity Mapping Observations

The Astrophysical journal, 2022-04, Vol.929 (1), p.30

2022

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Testing general relativity on cosmological scales at redshift z ∼ 1.5 with quasar and CMB lensing

Monthly notices of the Royal Astronomical Society, 2021-02, Vol.501 (1), p.1013-1027

2021

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Extragalactic science with the experiment for cryogenic large-aperture intensity mapping

Monthly notices of the Royal Astronomical Society, 2023-06, Vol.521 (4), p.6124-6142

2023

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Systematic error mitigation for the PIXIE Fourier transform spectrometer

Journal of cosmology and astroparticle physics, 2023-07, Vol.2023 (7), p.57

2023

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Interloper bias in future large-scale structure surveys

Publications of the Astronomical Society of Japan, 2016-02, Vol.68 (1)

2016

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New probe of the high-redshift Universe: Nulling CMB lensing with interloper-free line intensity mapping pair lensing

Physical review. D, 2022-04, Vol.105 (8), Article 083509

2022

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Search for CII emission on cosmological scales at redshift Z ~ 2.6

Monthly notices of the Royal Astronomical Society, 2018-08, Vol.478 (2)

2018

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Constraining cosmology with the CMB × line intensity mapping-nulling convergence

Physical review. D, 2024-06, Vol.109 (12), Article 123518

2024

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Constraining gravity at the largest scales through CMB lensing and galaxy velocities

CROSS-CORRELATIONS AS A COSMOLOGICAL CARBON MONOXIDE DETECTOR

Calibrating magnification bias for the EG statistic to test general relativity

Probing gravity at large scales through CMB lensing

Characterizing the Conditional Galaxy Property Distribution Using Gaussian Mixture Models

Evidence for C ii diffuse line emission at redshift z ∼ 2.6

Removing interlopers from intensity mapping probes of primordial non-Gaussianity

INTENSITY MAPPING ACROSS COSMIC TIMES WITH THE Lyα LINE

Non-detection of a statistically anisotropic power spectrum in large-scale structure

New Probe of the High-z Baryon Acoustic Oscillation Scale: BAO Tomography with CMB×LIM-Nulling Convergence

Full-sky lensing reconstruction of 21 cm intensity maps

Constraining the star formation rate using joint CIB continuum and C ii intensity mapping

An Empirical Representation of a Physical Model for the ISM [C ii], CO, and [C i] Emission at Redshift 1 ≤ z ≤ 9

A new calibration method of sub-halo orbital evolution for semi-analytic models

Multitracer Cosmological Line Intensity Mapping Mock Light-cone Simulation

Systematic Effects in Large-Scale Angular Power Spectra of Photometric Quasars and Implications for Constraining Primordial Non-Gaussianity

Quantifying the power spectrum of small-scale structure in semi-analytic galaxies

On Estimating the Cosmic Molecular Gas Density from CO Line Intensity Mapping Observations

Testing general relativity on cosmological scales at redshift z ∼ 1.5 with quasar and CMB lensing

Extragalactic science with the experiment for cryogenic large-aperture intensity mapping

Systematic error mitigation for the PIXIE Fourier transform spectrometer

Interloper bias in future large-scale structure surveys

New probe of the high-redshift Universe: Nulling CMB lensing with interloper-free line intensity mapping pair lensing

Search for CII emission on cosmological scales at redshift Z ~ 2.6

Constraining cosmology with the CMB × line intensity mapping-nulling convergence

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