pith. sign in

E)

Identifiers

  • name variant E) 0.60 · backfill

Papers (16)

  1. Kinetic Inductance Detectors for the OLIMPO experiment: in--flight operation and performance astro-ph.IM · 2019 · author #18
  2. Observation of $D^+_s\rightarrow p\bar{n}$ and confirmation of its large branching fraction hep-ex · 2018 · author #389
  3. Panoramic optical and near-infrared SETI instrument: overall specifications and science program astro-ph.IM · 2018 · author #6
  4. Observation of the decay $B^0_s \to \phi\pi^+\pi^-$ and evidence for $B^0 \to \phi\pi^+\pi^-$ hep-ex · 2016 · author #119
  5. Amplitude analysis of the $\chi_{c1} \to \eta\pi^+\pi^-$ decays hep-ex · 2016 · author #3
  6. Baseline design of the filters for the LAD detector on board LOFT astro-ph.IM · 2014 · author #6
  7. Study of $e^+e^- \rightarrow p\bar{p}$ in the vicinity of $\psi(3770)$ hep-ex · 2014 · author #17
  8. The X-ray variability history of Markarian 3 astro-ph.CO · 2012 · author #13
  9. Two-photon widths of the $\chi_{c0, 2}$ states and helicity analysis for $\chi_{c2}\ar\gamma\gamma$} hep-ex · 2012 · author #217
  10. Study of $J/\psi\to p\bar{p}$ and $J/\psi\to n\bar{n}$ hep-ex · 2012 · author #217
  11. The final verdict by XMM-Newton: the X-ray obscured Seyfert galaxy NGC5506 has a broad Fe K-alpha line astro-ph.CO · 2010 · author #3
  12. X-ray obscuration in local Universe AGN astro-ph · 2006 · author #3
  13. On the origin of soft X-rays in obscured AGN: answers from high-resolution spectroscopy with XMM-Newton astro-ph · 2006 · author #4
  14. The history of the iron K-alpha line profile in the Piccinotti AGN ESO198-G24 astro-ph · 2003 · author #3
  15. The XMM-Newton Science Archive astro-ph · 2002 · author #9
  16. The formerly X-ray reflection-dominated Seyfert~2 galaxy NGC6300 astro-ph · 2001 · author #5

Mentions

  • 1408.6546 #6 · backfill · confidence 0.70 E)
  • 1403.6011 #17 · backfill · confidence 0.70 E)
  • 1209.0706 #13 · backfill · confidence 0.70 E)
  • 1205.4284 #217 · backfill · confidence 0.70 E)
  • 1205.1036 #217 · backfill · confidence 0.70 E)
  • 1004.1442 #3 · backfill · confidence 0.70 E)

Frequent Coauthors