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Michael T. Murphy

4 papers hereh-index 4171 citations7 works total

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

author position
  • middle author2
  • last author2

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

fields
  • astro-ph.CO2
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • Michael T. Murphy — 3 papers, h 2
  • Michael T. Murphy — 2 papers, h 2
  • Michael T. Murphy — 1 paper, h 2
  • Michael T. Murphy — 1 paper, h 2

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

collaborators

4 papers

astro-ph.IM2013

A Community Science Case for E-ELT HIRES

R. Maiolino, M. Haehnelt, M. T. Murphy +57

Building on the experience of the high-resolution community with the suite of VLT high-resolution spectrographs, which has been tremendously successful, we outline here the (scienc…

astro-ph.CO2010

The neutral gas extent of galaxies as derived from weak intervening CaII absorbers

P. Richter, F. Krause, C. Fechner +2

(Abridged) We present a systematic study of weak intervening CaII absorbers at low redshift (z<0.5), based on the analysis of archival high resolution (R>45,000) optical spectra of…

astro-ph.GA2010

Absorption and emission line studies of gas in the Milky Way halo

N. Ben Bekhti, P. Richter, B. Winkel +4

We perform a systematic study of physical properties and distribution of neutral and ionised gas in the halo of the Milky Way (MW). Beside the large neutral intermediate- and high-…

astro-ph.CO2010

Galaxy Group at z=0.3 Associated with the Damped Lyman Alpha System Towards Quasar Q1127-145

G. G. Kacprzak, M. T. Murphy, C. W. Churchill

(Abridged) We performed a spectroscopic galaxy survey, complete to m<20.3 (L_B>0.15L_B* at z=0.3), within 100x100" of the quasar Q1127-145 (z=1.18). The VLT/UVES quasar spectrum co…

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