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D. Alves

77 papers hereh-index 446.8k citations159 works total

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

author position
  • sole author6
  • first author11
  • middle author38
  • last author3

Across the 58 of 77 papers where every author was matched, so the position is known.

fields
  • astro-ph77
same name
  • D. Alves — 31 papers, h 21
  • D. Alves — 30 papers, h 7
  • D. Alves — 7 papers, h 8
  • D. Alves — 2 papers, h 7
  • D. Alves — 1 paper, h 1
  • D. Alves — 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
19942006
most citedThe MACHO Project: Microlensing Results from 5.7 Years of LMC Observations

1k citations · 6.2k across the 77 of their papers we have counts for

collaborators
Showing 1995Show all

4 papers · 1 filter

astro-ph1995★ 202 cited

The MACHO Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge Data

C. Alcock, R. A. Allsman, T. S. Axelrod +15

We report the detection of 45 candidate microlensing events in fields toward the Galactic bulge. These come from the analysis of 24 fields containing 12.6 million stars observed fo…

astro-ph1995★ 1 cited

Real-time Detection of Gravitational Microlensing

M. R. Pratt, C. Alcock, R. A. Allsman +17

Real-time detection of microlensing has moved from proof of concept in 1994 to a steady stream of events this year. Global dissemination of these events by the MACHO and OGLE colla…

astro-ph1995★ 208 cited

First Observation of Parallax in a Gravitational Microlensing Event

C. Alcock, R. A. Allsman, D. Alves +14

We present the first detection of parallax effects in a gravitational microlensing event. Parallax in a gravitational microlensing event observed only from the Earth appears as a d…

astro-ph1995★ 9 cited

Ground-based Discovery of Cepheids and Miras in M101

David R. Alves, Kem H. Cook

We have identified 4 Cepheids and 5 Miras using KPNO 4m BVRI images of an outer field in M101. The Cepheid and Mira periods range from 30 to 60 days and 350 to 800 days, respective…

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