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B. Shahzamanian

Identifiers

  • name variant B. Shahzamanian 0.60 · backfill

Papers (16)

  1. A new bow-shock source with bipolar morphology in the vicinity of Sgr A* astro-ph.GA · 2019 · author #5
  2. Light and shadow in the Galactic Center - On the detection of the relativistic periastron shift of star S2 in the Galactic Center astro-ph.HE · 2018 · author #4
  3. The Multifrequency Behavior of Sagittarius A* astro-ph.HE · 2018 · author #6
  4. Nuclear Activity and the Conditions of Star-formation at the Galactic Center astro-ph.GA · 2017 · author #3
  5. Investigating the Relativistic Motion of the Stars Near the Supermassive Black Hole in the Galactic Center astro-ph.GA · 2017 · author #3
  6. Polarized near-infrared light of the Dusty S-cluster Object (DSO/G2) at the Galactic Center astro-ph.GA · 2016 · author #1
  7. Monitoring the Galactic Centre with Australia Telescope Compact Array astro-ph.GA · 2016 · author #7
  8. Wisps in the Galactic center: NIR triggered observations of the radio source Sgr A* at 43 GHz astro-ph.GA · 2015 · author #6
  9. The Center of the Milky Way from Radio to X-rays astro-ph.GA · 2015 · author #3
  10. Polarized light from Sgr A* in the near-infrared $K_{s}$-band astro-ph.GA · 2014 · author #1
  11. Monitoring the Dusty S-Cluster Object (DSO/G2) on its Orbit towards the Galactic Center Black Hole astro-ph.GA · 2014 · author #12
  12. The infrared K-band identification of the DSO/G2 source from VLT and Keck data astro-ph.GA · 2013 · author #7
  13. The Galactic Center as a Paradigm for Low Luminosity Nuclei? The K-band identification of the DSO/G2 source from VLT and Keck data astro-ph.GA · 2013 · author #7
  14. Source-intrinsic near-infrared properties of Sgr A*: Total intensity measurements astro-ph.HE · 2012 · author #5
  15. Near-infrared proper motions and spectroscopy of infrared excess sources at the Galactic Center astro-ph.IM · 2012 · author #4
  16. Beating the confusion limit: The necessity of high angular resolution for probing the physics of Sagittarius A* and its environment: Opportunities for LINC-NIRVANA (LBT), GRAVITY (VLTI) and and METIS (E-ELT) astro-ph.IM · 2012 · author #5

Mentions

  • 1501.02164 #3 · backfill · confidence 0.70 B. Shahzamanian
  • 1411.0006 #1 · backfill · confidence 0.70 B. Shahzamanian
  • 1410.8731 #12 · backfill · confidence 0.70 B. Shahzamanian
  • 1311.2753 #7 · backfill · confidence 0.70 B. Shahzamanian
  • 1311.2743 #7 · backfill · confidence 0.70 B. Shahzamanian
  • 1208.5836 #5 · backfill · confidence 0.70 B. Shahzamanian
  • 1208.1907 #4 · backfill · confidence 0.70 B. Shahzamanian
  • 1208.1129 #5 · backfill · confidence 0.70 B. Shahzamanian

Frequent Coauthors