activity
20132023
most citedStructure of neutron stars in R-squared gravity

107 citations · 512 across the 17 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2023★ 38 cited

A variable corona during the transition from type-C to type-B quasi-periodic oscillations in the black hole X-ray binary MAXI J1820+070

Ruican Ma, Mariano Mendez, Federico Garcia +3

We analyze a Neutron Star Interior Composition Explorer (NICER) observation of the black hole X-ray binary MAXI J1820+070 during a transition from type-C to type-B quasi-periodic o…

astro-ph.HE2023★ 12 cited

The X-ray corona in the black-hole binary GRO J1655--40 from the properties of non-harmonically related quasi-periodic oscillations

Sandeep K. Rout, Mariano Mendez, Federico Garcia

The study of quasi periodic oscillations (QPOs) plays a vital role in understanding the nature and geometry of the Comptonizing medium around black-hole X-ray binaries. The spectra…

astro-ph.IM2023

Pulsar Observations at low latitudes and low frequencies

Carlos O. Lousto, R. Missel, E. Zubieta +6

The Pulsar Monitoring in Argentina (PuMA) is a collaboration between the Argentine Institute for Radioastronomy (IAR) and the Rochester Institute of Technology (RIT) that since 201…

astro-ph.HE2023★ 25 cited

A NICER look at the jet-like corona of MAXI J1535-571 through type-B quasi-periodic oscillations

Yuexin Zhang, Mariano Méndez, Federico García +7

MAXI J1535-571 is a black-hole X-ray binary that in 2017 exhibited a very bright outburst which reached a peak flux of up to 5 Crab in the 2-20 keV band. Given the high flux, sever…

astro-ph.HE2023★ 85 cited

A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era

Francis Fortin, Federico Garcia, Adolfo Simaz-Bunzel +1

High-mass X-ray binaries (HMXBs) are a particular class of high-energy sources that require multi-wavelength observational efforts to be properly characterised. New identifications…

astro-ph.GA2022★ 11 cited

Finding the birthplace of HMXBs in the Galaxy using Gaia EDR3: kinematical age determination through orbit integration

Francis Fortin, Federico Garcia, Sylvain Chaty

High-Mass X-ray Binaries (HMXBs) are produced after the first supernova event in a massive binary. These objects are intrinsically young, and can suffer from a significant natal ki…