◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

M. Murphy

4 papers hereh-index 331 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph.SR2
same name
  • M. Murphy — 60 papers, h 47
  • M. Murphy — 26 papers, h 28
  • M. Murphy — 14 papers, h 14
  • M. Murphy — 6 papers, h 11
  • M. Murphy — 5 papers, h 4
  • M. Murphy — 3 papers, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
most citedOn the 12C/13C isotopic ratio at the dawn of chemical evolution

20 citations · 20 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2026

The ESPRESSO Redshift Drift Experiment III -- The Third Epoch of QSO J052915.80-435152.0

Andrea Trost, Catarina M. J. Marques, S. Cristiani +25

The Sandage-Loeb test probes cosmic expansion directly by measuring the redshift drift in quasar absorption features in a model-independent way. In this series of papers, we have l…

astro-ph.SR2025

Unveiling the nature of HE 0107-5240

E. Caffau, M. Steffen, P. Molaro +27

The vast majority of the most iron-poor stars in the Galaxy exhibit a strong carbon enhancement, with C/H ratios only about two orders of magnitude below solar. This unusual chemic…

astro-ph.CO2023

Cosmology and fundamental physics with the ELT-ANDES spectrograph

C. J. A. P. Martins, R. Cooke, J. Liske +20

State-of-the-art 19th century spectroscopy led to the discovery of quantum mechanics, and 20th century spectroscopy led to the confirmation of quantum electrodynamics. State-of-the…

astro-ph.SR2023★ 20 cited

On the 12C/13C isotopic ratio at the dawn of chemical evolution

P. Molaro, D. S. Aguado, E. Caffau +21

The known Mega and Hyper Metal-Poor (MMP-HMP) stars with [Fe/H]<-6.0 and <-5.0, respectively, likely belong to the CEMP-no class, i.e. carbon-enhanced stars with low or absent seco…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.