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researcher

K. Su

25 papers hereh-index 283.1k citations57 works total

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

author position
  • middle author16
  • last author2

Across the 18 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph15
  • astro-ph.SR6
  • astro-ph.EP2
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • K. Su — 121 papers, h 20
  • K. Su — 90 papers, h 36
  • K. Su — 3 papers, h 5
  • K. Su — 3 papers, h 2
  • K. Su — 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
20042023
most citedDebris disks in main sequence binary systems

369 citations · 2.2k across the 25 of their papers we have counts for

collaborators
Showing 2007 · astro-phShow all

4 papers · 2 filters

astro-ph2007★ 297 cited

Debris disks around Sun-like stars

D. E. Trilling, G. Bryden, C. A. Beichman +7

We have observed nearly 200 FGK stars at 24 and 70 microns with the Spitzer Space Telescope. We identify excess infrared emission, including a number of cases where the observed fl…

astro-ph2007★ 21 cited

Spitzer observations of V4332 Sagittarii: Detection of Alumina Dust

D. P. K. Banerjee, K. A. Misselt, K. Y. L. Su +2

We present broad-band 24, 70 and 160 micron photometry, 5-35 micron and 55-90 micron spectra of the eruptive variable V4332 Sgr from Spitzer observations. The distinguishing featur…

astro-ph2007★ 70 cited

The Dust and Gas Around beta Pictoris

C. H. Chen, A. Li, C. Bohac +12

We have obtained Spitzer IRS 5.5 - 35 micron spectroscopy of the debris disk around beta Pictoris. In addition to the 10 micron silicate emission feature originally observed from t…

astro-ph2007★ 123 cited

A Debris Disk around the Central Star of the Helix Nebula?

Kate Y. L. Su, Y. -H. Chu, G. H. Rieke +6

Excess emission from a point-like source coincident with the central star of the Helix Nebula is detected with Spitzer at 8, 24, and 70 um. At 24 um, the central source is superpos…

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