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researcher

M. Bulla

124 papers hereh-index 356.3k citations148 works total

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

author position
  • sole author1
  • first author6
  • middle author98
  • last author1

Across the 106 of 124 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE98
  • astro-ph.SR8
  • astro-ph.IM7
  • gr-qc5
  • astro-ph.GA3
  • astro-ph.CO1
same name
  • M. Bulla — 13 papers, h 4
  • M. Bulla — 4 papers, h 3
  • M. Bulla — 2 papers, h 0
  • M. Bulla — 1 paper, h 1
  • M. Bulla — 1 paper, h 1
  • M. Bulla — 1 paper, h 0

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 Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 8.4k across the 119 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2022★ 4 cited

Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae

Takashi Nagao, Ferdinando Patat, Keiichi Maeda +8

Investigating interstellar (IS) dust properties in external galaxies is important not only to infer the intrinsic properties of astronomical objects but also to understand the star…

astro-ph.GA2021

An imaging polarimetry survey of Type Ia supernovae: are peculiar extinction and polarization properties produced by circumstellar or interstellar matter?

Matthew R. Chu, Aleksandar Cikota, Dietrich Baade +8

Some highly reddened Type Ia supernovae (SNe Ia) display low total-to-selective extinction ratios (RV​≲2) in comparison to that of typical Milky Way dust ($R_V \approx 3…

astro-ph.GA2017★ 12 cited

Probing gas and dust in the tidal tail of NGC 5221 with the type Ia supernova iPTF16abc

R. Ferretti, R. Amanullah, A. Goobar +8

Context. Type Ia supernovae (SNe Ia) can be used to address numerous questions in astrophysics and cosmology. Due to their well known spectral and photometric properties, SNe Ia ar…

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