Michael Line

Michael Line

University of California, Santa Cruz

H-index: 60

North America-United States

About Michael Line

Michael Line, With an exceptional h-index of 60 and a recent h-index of 54 (since 2020), a distinguished researcher at University of California, Santa Cruz, specializes in the field of Planetary Atmospheres, Exoplanets, Brown Dwarfs.

His recent articles reflect a diverse array of research interests and contributions to the field:

WASP-77Ab through the eyes of JWST/NIRSpec: pearls, pitfalls and lessons learned

Strongly varying water absorption in the ultra-hot Jupiter WASP-121b at high spectral resolution

A High-Performance Analysis Framework for JWST Exoplanet Observations

A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree that the Atmosphere of WASP-77A b Is Metal-poor

High-Precision Atmospheric Constraints for a Cool T Dwarf from JWST Spectroscopy

High-precision atmospheric characterization of a Y dwarf with JWST NIRSpec G395H spectroscopy: isotopologue, C/O ratio, metallicity, and the abundances of six molecular species

Fundamental Properties and Formation Pathways of an Extremely Cold Companion

From Dawn to Dusk: Diagnosing Asymmetric Limbs in Exoplanet Transmission Spectra

Michael Line Information

University

Position

Postdoctoral Researcher

Citations(all)

11403

Citations(since 2020)

8356

Cited By

6345

hIndex(all)

60

hIndex(since 2020)

54

i10Index(all)

118

i10Index(since 2020)

116

Email

University Profile Page

Google Scholar

Michael Line Skills & Research Interests

Planetary Atmospheres

Exoplanets

Brown Dwarfs

Top articles of Michael Line

WASP-77Ab through the eyes of JWST/NIRSpec: pearls, pitfalls and lessons learned

AAS/Division for Extreme Solar Systems Abstracts

2024/4

Strongly varying water absorption in the ultra-hot Jupiter WASP-121b at high spectral resolution

AAS/Division for Extreme Solar Systems Abstracts

2024/4

A High-Performance Analysis Framework for JWST Exoplanet Observations

JWST Proposal. Cycle 3

2024/3

A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree that the Atmosphere of WASP-77A b Is Metal-poor

The Astronomical Journal

2024/2/14

High-Precision Atmospheric Constraints for a Cool T Dwarf from JWST Spectroscopy

arXiv preprint arXiv:2402.05345

2024/2/8

High-precision atmospheric characterization of a Y dwarf with JWST NIRSpec G395H spectroscopy: isotopologue, C/O ratio, metallicity, and the abundances of six molecular species

arXiv preprint arXiv:2402.05900

2024/2/8

Fundamental Properties and Formation Pathways of an Extremely Cold Companion

JWST Proposal. Cycle 3

2024/2

From Dawn to Dusk: Diagnosing Asymmetric Limbs in Exoplanet Transmission Spectra

JWST Proposal. Cycle 3

2024/2

Around the world in less than two days: observing the spectral phase curve of an ultra-hot Jupiter with JWST/NIRSpec

JWST Proposal. Cycle 3

2024/2

The Roasting Marshmallows Campaign with IGRINS on Gemini South: Characterizing the Composition and Climate of Transiting Exoplanets

American Astronomical Society Meeting Abstracts

2024/2

Improving Atmospheric Retrieval Techniques with Fitted Covariance Structures

American Astronomical Society Meeting Abstracts

2024/2

Michael Line
Michael Line

H-Index: 43

Luis Welbanks
Luis Welbanks

H-Index: 8

The JWST Emission Spectrum of the Inflated Hot Saturn WASP-69 b

American Astronomical Society Meeting Abstracts

2024/2

Protosolar D/H abundance in the coldest brown dwarf

AAS/Division for Extreme Solar Systems Abstracts

2024/4

The Detection of Multiple Molecular Species in the Atmospheres of a Sub-Neptune and Super-Neptune

AAS/Division for Extreme Solar Systems Abstracts

2024/4

JWST/NIRSpec Transmission Spectrum of the Hazy Sub-Neptune GJ1214 b

AAS/Division for Extreme Solar Systems Abstracts

2024/4

The first full broadband transmission spectrum of an exoplanet. The chemistry of WASP-39b revealed from 0.5 to 12 μm with JWST

AAS/Division for Extreme Solar Systems Abstracts

2024/4

Search for C, N, O in a long-period transiting warm Saturn

HST Proposal

2024/1

Michael Line
Michael Line

H-Index: 43

The SPHINX M-dwarf Spectral Grid. II. Fundamental Properties of Mid-to-Late M-dwarfs

AAS/Division for Extreme Solar Systems Abstracts

2024/4

Aishwarya Iyer
Aishwarya Iyer

H-Index: 5

Michael Line
Michael Line

H-Index: 43

See List of Professors in Michael Line University(University of California, Santa Cruz)