◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

S. Paltani

12 papers here

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

author position
  • middle author2

Across the 2 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
  • astro-ph.IM3
  • astro-ph2
  • astro-ph.CO2
  • astro-ph.GA1
ORCID 0000-0002-8108-9179
same name
  • S. Paltani — 468 papers, h 71
  • S. Paltani — 71 papers, h 0
  • S. Paltani — 4 papers, h 4
  • S. Paltani — 2 papers, h 6

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
20072025
most citedEuclid. I. Overview of the Euclid mission

550 citations · 1.2k across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2025★ 12 cited

Delving into the depths of NGC 3783 with XRISM II. Cross-calibration of X-ray instruments used in the large, multi-mission observational campaign

XRISM collaboration

Accurate X-ray spectroscopic measurements are fundamental for deriving basic physical parameters of the most abundant baryon components in the Universe. The plethora of X-ray obser…

astro-ph.HE2022

Euclid: Searching for pair-instability supernovae with the Deep Survey

T. J. Moriya, C. Inserra, M. Tanaka +106

Pair-instability supernovae are theorized supernovae that have not yet been observationally confirmed. They are predicted to exist in low-metallicity environments. Because overall…

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2017★ 116 cited

Solar abundance ratios of the iron-peak elements in the Perseus Cluster

Hitomi Collaboration

The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.