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19942026
most citedThe Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

837 citations · 19.2k across the 257 of their papers we have counts for

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10 papers · 1 filter

astro-ph.GA2023

The Central Kinematics and Black Hole Mass of 4C+37.11

Tirth Surti, Roger W. Romani, Julia Scharwächter +2

We report on IFU measurements of the host of the radio source 4C+37.11. This massive elliptical contains the only resolved double compact nucleus at pc-scale separation, likely a b…

astro-ph.GA2023★ 2 cited

Ultra-Low Frequency Gravitational Waves from Massive Clusters at z~1

David K. Wendt, Roger W. Romani

Recent progress with pulsar timing array experiments, especially from the NANOGrav collaboration indicate that we are on the cusp of detecting significant signals from the inspiral…

astro-ph.GA2017★ 95 cited

Constraining the Orbit of Supermassive Black Hole Binary 0402+379

Karishma Bansal, Greg B. Taylor, Alison. B. Peck +2

The radio galaxy 0402+379 is believed to host a supermassive black hole binary (SMBHB). The two compact core sources are separated by a projected distance of 7.3 pc, making it the…

astro-ph.GA2016★ 65 cited

Compact Symmetric Objects and Supermassive Binary Black Holes in the VLBA Imaging and Polarimetry Survey

S. E. Tremblay, G. B. Taylor, A. A. Ortiz +3

We present multi-frequency Very Long Baseline Array (VLBA) follow-up observations of VLBA Imaging and Polarimetry Survey sources identified as likely compact symmetric objects (CSO…

astro-ph.GA2014★ 10 cited

Imaging Redshift Estimates for Fermi BL Lacs

Matt Stadnik, Roger W. Romani

We have obtained WIYN and SOAR i' images of BL Lacertae objects (BL Lacs) and used these to detect or constrain the flux of the host galaxy. Under common standard candle assumption…

astro-ph.GA2013★ 8 cited

A Multi-wavelength Study of the Host Environment of SMBHB 4C+37.11

Roger W. Romani, W. R. Forman, Christine Jones +4

4C+37.11, at z=0.055 shows two compact radio nuclei, imaged by VLBI at 7mas separation, making it the closest known resolved super-massive black hole binary (SMBHB). An important q…

astro-ph.GA2010★ 11 cited

Radio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740

A. Noutsos, A. A. Abdo, M. Ackermann +146

We report on the first year of Fermi gamma-ray observations of pulsed high-energy emission from the old PSR J2043+2740. The study of the gamma-ray efficiency of such old pulsars gi…

astro-ph.GA2010★ 338 cited

Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT

LAT Collaboration

Pulsars are rapidly-rotating, highly-magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until r…

astro-ph.GA2009★ 144 cited

Radio detection of LAT PSRs J1741-2054 and J2032+4127: no longer just gamma-ray pulsars

F. Camilo, P. S. Ray, S. M. Ransom +24

Sixteen pulsars have been discovered so far in blind searches of photons collected with the Large Area Telescope on the Fermi Gamma-ray Space Telescope. We here report the discover…

astro-ph.GA2009★ 3 cited

Identifying Compact Symmetric Objects from the VLBA Imaging and Polarization Survey

S. E. Tremblay, G. B. Taylor, J. F. Helmboldt +2

Compact Symmetric Objects (CSOs) are small (less than 1 kpc) radio sources which have symmetric double lobes or jets. The dominant theory for the small size of these objects is tha…