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1
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
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A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4

The Astrophysical journal, 2018-12, Vol.868 (2), p.92 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Dec 01, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aae8e0

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2
Fast Magnetic Reconnection: "Ideal" Tearing and the Hall Effect
Fast Magnetic Reconnection: "Ideal" Tearing and the Hall Effect
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Fast Magnetic Reconnection: "Ideal" Tearing and the Hall Effect

The Astrophysical journal, 2017-08, Vol.845 (1), p.25 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Aug 10, 2017 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa7b82

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3
The Imprint of Neutrinos on Clustering in Redshift Space
The Imprint of Neutrinos on Clustering in Redshift Space
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The Imprint of Neutrinos on Clustering in Redshift Space

The Astrophysical journal, 2018-07, Vol.861 (1), p.53 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jul 01, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aac6bf

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4
The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
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The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument

The Astronomical journal, 2023-04, Vol.165 (4), p.144 [Peer Reviewed Journal]

2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/acb212

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5
The Aemulus Project. III. Emulation of the Galaxy Correlation Function
The Aemulus Project. III. Emulation of the Galaxy Correlation Function
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The Aemulus Project. III. Emulation of the Galaxy Correlation Function

The Astrophysical journal, 2019-03, Vol.874 (1), p.95 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 20, 2019 ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab0d7b

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6
Atmospheric new particle formation and growth: review of field observations
Atmospheric new particle formation and growth: review of field observations
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Atmospheric new particle formation and growth: review of field observations

Environmental research letters, 2018-09, Vol.13 (10), p.103003 [Peer Reviewed Journal]

2018 The Author(s). Published by IOP Publishing Ltd ;2018. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 1748-9326 ;EISSN: 1748-9326 ;DOI: 10.1088/1748-9326/aadf3c ;CODEN: ERLNAL

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7
Research on the adjustment boundary of well pattern injection-production structure in the eastern area of South Second District
Research on the adjustment boundary of well pattern injection-production structure in the eastern area of South Second District
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Research on the adjustment boundary of well pattern injection-production structure in the eastern area of South Second District

IOP conference series. Earth and environmental science, 2021-08, Vol.831 (1), p.12019 [Peer Reviewed Journal]

Published under licence by IOP Publishing Ltd ;2021. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 1755-1307 ;EISSN: 1755-1315 ;DOI: 10.1088/1755-1315/831/1/012019

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8
The Effect of Supernova Convection On Neutron Star and Black Hole Masses
The Effect of Supernova Convection On Neutron Star and Black Hole Masses
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The Effect of Supernova Convection On Neutron Star and Black Hole Masses

The Astrophysical journal, 2022-06, Vol.931 (2), p.94 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac6ac9

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9
Disk Tearing: Numerical Investigation of Warped Disk Instability
Disk Tearing: Numerical Investigation of Warped Disk Instability
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Disk Tearing: Numerical Investigation of Warped Disk Instability

The Astrophysical journal, 2021-03, Vol.909 (1), p.81 [Peer Reviewed Journal]

Copyright IOP Publishing Mar 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abdc24

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10
Streaming Instability for Particle-size Distributions
Streaming Instability for Particle-size Distributions
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Streaming Instability for Particle-size Distributions

Astrophysical journal. Letters, 2019-06, Vol.878 (2), p.L30 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 20, 2019 ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/ab2596

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11
SIGNS OF EARLY-STAGE DISK GROWTH REVEALED WITH ALMA
SIGNS OF EARLY-STAGE DISK GROWTH REVEALED WITH ALMA
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SIGNS OF EARLY-STAGE DISK GROWTH REVEALED WITH ALMA

The Astrophysical journal, 2017-01, Vol.834 (2), p.178 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jan 10, 2017 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/834/2/178

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12
Plausible 2005–2050 emissions scenarios project between 2 °C and 3 °C of warming by 2100
Plausible 2005–2050 emissions scenarios project between 2 °C and 3 °C of warming by 2100
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Plausible 2005–2050 emissions scenarios project between 2 °C and 3 °C of warming by 2100

Environmental research letters, 2022-02, Vol.17 (2), p.24027 [Peer Reviewed Journal]

2022 The Author(s). Published by IOP Publishing Ltd ;2022 The Author(s). Published by IOP Publishing Ltd. This work is published under http://creativecommons.org/licenses/by/4.0 (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 1748-9326 ;EISSN: 1748-9326 ;DOI: 10.1088/1748-9326/ac4ebf ;CODEN: ERLNAL

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13
MODELING DUST EVOLUTION IN GALAXIES WITH A MULTIPHASE, INHOMOGENEOUS ISM
MODELING DUST EVOLUTION IN GALAXIES WITH A MULTIPHASE, INHOMOGENEOUS ISM
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MODELING DUST EVOLUTION IN GALAXIES WITH A MULTIPHASE, INHOMOGENEOUS ISM

The Astrophysical journal, 2016-11, Vol.831 (2), p.147 [Peer Reviewed Journal]

2016. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Nov 10, 2016 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/831/2/147

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14
Constraints to Dark Energy Using PADE Parameterizations
Constraints to Dark Energy Using PADE Parameterizations
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Constraints to Dark Energy Using PADE Parameterizations

The Astrophysical journal, 2017-07, Vol.843 (1), p.65 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jul 01, 2017 ;info:eu-repo/semantics/openAccess ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa7898

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15
Thresholds for Particle Clumping by the Streaming Instability
Thresholds for Particle Clumping by the Streaming Instability
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Thresholds for Particle Clumping by the Streaming Instability

The Astrophysical journal, 2021-10, Vol.919 (2), p.107 [Peer Reviewed Journal]

2021. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Oct 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac0e9f

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16
Observational Constraints on the Tilted Spatially Flat and the Untilted Nonflat φCDM Dynamical Dark Energy Inflation Models
Observational Constraints on the Tilted Spatially Flat and the Untilted Nonflat φCDM Dynamical Dark Energy Inflation Models
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Observational Constraints on the Tilted Spatially Flat and the Untilted Nonflat φCDM Dynamical Dark Energy Inflation Models

The Astrophysical journal, 2018-12, Vol.868 (2), p.83 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Dec 01, 2018 ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aae82d

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17
Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data
Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data
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Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data

The Astrophysical journal, 2019-09, Vol.882 (2), p.158 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Sep 10, 2019 ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab3641

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18
Streaming Instability in Turbulent Protoplanetary Disks
Streaming Instability in Turbulent Protoplanetary Disks
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Streaming Instability in Turbulent Protoplanetary Disks

The Astrophysical journal, 2020-05, Vol.895 (1), p.4 [Peer Reviewed Journal]

2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing May 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab899d

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19
On the Detection of Coronal Dimmings and the Extraction of Their Characteristic Properties
On the Detection of Coronal Dimmings and the Extraction of Their Characteristic Properties
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On the Detection of Coronal Dimmings and the Extraction of Their Characteristic Properties

The Astrophysical journal, 2018-03, Vol.855 (2), p.137 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aaadb5

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20
How Efficient Is the Streaming Instability in Viscous Protoplanetary Disks?
How Efficient Is the Streaming Instability in Viscous Protoplanetary Disks?
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How Efficient Is the Streaming Instability in Viscous Protoplanetary Disks?

The Astrophysical journal, 2020-03, Vol.891 (2), p.132 [Peer Reviewed Journal]

2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 10, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab76ca

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