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M. Pettini

13 papers hereh-index 2728 citations9 works total

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

author position
  • first author1
  • middle author11

Across the 12 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph4
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • M. Pettini — 204 papers, h 85
  • M. Pettini — 58 papers, h 32
  • M. Pettini — 11 papers, h 8
  • M. Pettini — 1 paper, h 1

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
19952026
most citedLyman Limit Imaging of High Redshift Galaxies. III. New Observations of 4 QSO Fields

231 citations · 513 across the 12 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2001★ 1 cited

Deep Observations of Lyman Break Galaxies

Max Pettini, Charles C. Steidel, Alice E. Shapley +5

We summarise the main results of recent work on the Lyman break galaxy population which takes advantage of newly commissioned instrumentation on the VLT and Keck telescopes to push…

astro-ph1998★ 6 cited

Galaxy Clustering at z~3

C. Steidel, K. Adelberger, M. Giavalisco +3

Galaxies at very high redshift (z~3 or greater) are now accessible to wholesale observation, making possible for the first time a robust statistical assessment of their spatial dis…

astro-ph1998★ 5 cited

Galaxies and Large Scale Structure at z~3

C. Steidel, K. Adelberger, M. Giavalisco +3

We summarize the status of a ``targeted'' redshift survey aimed at establishing the properties of galaxies and their large scale distribution in the redshift range 2.5 < z < 3.5. A…

astro-ph1995★ 231 cited

Lyman Limit Imaging of High Redshift Galaxies. III. New Observations of 4 QSO Fields

C. Steidel, M. Pettini, D. Hamilton

We present the results of deep Lyman limit imaging in four new fields as part of a continuing search for galaxies at 3.0≤z≤3.5. The technique uses a custom broad--band fi…

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