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K. Tassis

36 papers hereh-index 13453 citations42 works total

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

author position
  • middle author27
  • last author6

Across the 33 of 36 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO11
  • astro-ph.GA9
  • astro-ph.HE6
  • astro-ph.IM6
  • astro-ph.SR2
  • cs.LG1
same name
  • K. Tassis — 68 papers, h 26
  • K. Tassis — 26 papers, h 15
  • K. Tassis — 2 papers, 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
20142026
most citedThe magnetic field and dust filaments in the Polaris Flare

63 citations · 376 across the 34 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.GA2021★ 14 cited

HI-H2​ transition: exploring the role of the magnetic field

R. Skalidis, K. Tassis, G. V. Panopoulou +6

Atomic gas in the diffuse interstellar medium (ISM) is organized in filamentary structures. These structures usually host cold and dense molecular clumps. The Galactic magnetic fie…

astro-ph.GA2021★ 2 cited

Why take the square root? An assessment of interstellar magnetic field strength estimation methods

R. Skalidis, J. Sternberg, J. R. Beattie +2

The magnetic field strength in interstellar clouds can be estimated indirectly by using the spread of dust polarization angles (δθ). The method developed by Davis 1951 and by Cha…

astro-ph.CO2021★ 23 cited

SMILE: Search for MIlli-LEnses

C. Casadio, D. Blinov, A. C. S. Readhead +17

Dark Matter (DM) halos with masses below ∼108 M⊙​, which would help to discriminate between DM models, may be detected through their gravitational effect on distant…

astro-ph.CO2021★ 10 cited

Local alignments of parsec-scale AGN radiojets

N. Mandarakas, D. Blinov, C. Casadio +4

Context.Coherence in the characteristics of neighboring sources in 2D and 3D space may suggest the existence of large-scale cosmic structures, which are useful for cosmological stu…

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