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researcher

D. Schneider

792 papers hereh-index 178148.1k citations1.3k works total

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

author position
  • first author3
  • middle author474
  • last author131

Across the 608 of 792 papers where every author was matched, so the position is known.

fields
  • astro-ph322
  • astro-ph.CO236
  • astro-ph.GA164
  • astro-ph.SR34
  • astro-ph.HE16
  • astro-ph.IM11
same name
  • D. Schneider — 38 papers, h 30
  • D. Schneider — 25 papers, h 23
  • D. Schneider — 18 papers, h 17
  • D. Schneider — 17 papers, h 12
  • D. Schneider — 12 papers, h 8
  • D. Schneider — 7 papers, h 11

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
19932023
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 158.2k across the 789 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2017★ 12 cited

Exploratory X-ray Monitoring of Luminous Radio-Quiet Quasars at High Redshift: No Evidence for Evolution in X-ray Variability

Ohad Shemmer, W. N. Brandt, Maurizio Paolillo +4

We report on the second installment of an X-ray monitoring project of seven luminous radio-quiet quasars (RQQs). New {\sl Chandra} observations of four of these, at $4.10\leq z\leq…

astro-ph.HE2017★ 88 cited

Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate

G. Yang, C. -T. J. Chen, F. Vito +14

We investigate the dependence of black-hole accretion rate (BHAR) on host-galaxy star formation rate (SFR) and stellar mass (M∗​) in the CANDELS/GOODS-South field in the redshift…

astro-ph.HE2017★ 90 cited

Observational constraints on the specific accretion-rate distribution of X-ray selected AGN

A. Georgakakis, J. Aird, A. Schulze +5

This paper estimates the specific accretion-rate distribution of AGN using a sample of 4821 X-ray sources from both deep and shallow surveys. The specific accretion-rate distributi…

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