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researcher

S. Schmidt

47 papers hereh-index 279k citations93 works total

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

author position
  • sole author1
  • first author11
  • middle author29
  • last author3

Across the 44 of 47 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR37
  • astro-ph.IM5
  • astro-ph.CO3
  • astro-ph.GA2
same name
  • S. Schmidt — 69 papers, h 39
  • S. Schmidt — 56 papers, h 32
  • S. Schmidt — 40 papers, h 23
  • S. Schmidt — 28 papers, h 15
  • S. Schmidt — 23 papers
  • S. Schmidt — 16 papers, h 7

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
20092021
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 7.9k across the 46 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2012★ 2.1k cited

The Baryon Oscillation Spectroscopic Survey of SDSS-III

Kyle S. Dawson, David J. Schlegel, Christopher P. Ahn +162

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the…

astro-ph.CO2012

PHL 1811 Analogs: A Population of X-ray Weak Quasars

Jianfeng Wu, W. N. Brandt, Patrick B. Hall +6

We report on a population of X-ray weak quasars with similar UV emission-line properties to those of the remarkable quasar PHL 1811. All radio-quiet PHL 1811 analogs are notably X-…

astro-ph.CO2011★ 99 cited

A Population of X-ray Weak Quasars: PHL 1811 Analogs at High Redshift

Jianfeng Wu, W. N. Brandt, Patrick B. Hall +6

We report the results from Chandra and XMM-Newton observations of a sample of 10 type 1 quasars selected to have unusual UV emission-line properties (weak and blueshifted high-ioni…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.