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researcher

D. Monet

49 papers hereh-index 5241.7k citations236 works total

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

author position
  • first author3
  • middle author31
  • last author3

Across the 37 of 49 papers where every author was matched, so the position is known.

fields
  • astro-ph24
  • astro-ph.SR8
  • astro-ph.EP6
  • astro-ph.IM5
  • astro-ph.GA3
  • astro-ph.CO2
same name
  • D. Monet — 8 papers, h 9

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
19982018
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 26.1k across the 48 of their papers we have counts for

collaborators
Showing 2000Show all

4 papers · 1 filter

astro-ph2000★ 25 cited

CORMASS: A Compact and Efficient NIR Spectrograph for Studying Low-Mass Objects

J. C. Wilson, M. F. Skrutskie, M. R. Colonno +6

CorMASS (Cornell Massachusetts Slit Spectrograph) is a compact, low-resolution (R=300), double-pass prism cross-dispersed near-infrared (NIR) spectrograph in operation on the Palom…

astro-ph2000★ 10.4k cited

The Sloan Digital Sky Survey: Technical Summary

D. G. York

The Sloan Digital Sky Survey (SDSS) will provide the data to support detailed investigations of the distribution of luminous and non- luminous matter in the Universe: a photometric…

astro-ph2000★ 41 cited

A Survey for Faint Stars of Large Proper Motion Using Extra Poss II Plates

David G. Monet, Matthew D. Fisher, James Liebert +3

We have conducted a search for new stars of high proper motion (≥0.4 arcsec yr−1) using POSS II fields for which an extra IIIaF (red) plate of good quality exists, along…

astro-ph2000★ 503 cited

New Neighbors from 2MASS: Activity and Kinematics at the Bottom of the Main Sequence

John E. Gizis, David G. Monet, I. Neill Reid +3

We have combined 2MASS and POSS II data in a search for nearby ultracool (later than M6.5) dwarfs with K_s<12. Spectroscopic follow-up observations identify 53 M7 to M9.5 dwarfs an…

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