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J. Melbourne

25 papers hereh-index 203.1k citations40 works total

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

author position
  • first author6
  • middle author13
  • last author2

Across the 21 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO17
  • astro-ph3
  • astro-ph.GA3
  • astro-ph.SR2
same name
  • J. Melbourne — 27 papers, h 22
  • J. Melbourne — 27 papers, h 14
  • J. Melbourne — 2 papers
  • J. Melbourne — 1 paper, h 5

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
20002020
most citedThe Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample

1.7k citations · 3.9k across the 25 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 23 cited

Morphologies of High Redshift, Dust Obscured Galaxies from Keck Laser Guide Star Adaptive Optics

J. Melbourne, V. Desai, Lee Armus +7

Spitzer MIPS images in the Bootes field of the NOAO Deep Wide-Field Survey have revealed a class of extremely dust obscured galaxy (DOG) at z~2. The DOGs are defined by very red op…

astro-ph2004★ 6 cited

Measuring the Slope of the Dust Extinction Law and the Power Spectrum of Dust Clouds Using Differentially-Reddened Globular Clusters

J. Melbourne, P. Guhathakurta

We present 3 methods for measuring the Galactic dust extinction law slope R_V and a method for quantifying fine structure in dust clouds in the direction of differentially-reddened…

astro-ph2000★ 18 cited

CCD Photometry of the Globular Cluster NGC 4833 and Extinction Near the Galactic Plane

Jason Melbourne, Ata Sarajedini, Andrew Layden +1

We present CCD photometry for the Galactic globular cluster NGC 4833. Our BVI color magnitude diagrams (CMD) extend from above the red giant branch (RGB) tip to several magnitudes…

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