Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS2.6k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Massachusetts Institute of TechnologyUS1.9k papers
- University of FloridaUS1.8k papers
- Carnegie Mellon UniversityUS1.7k papers
- Princeton UniversityUS1.7k papers
- University of RochesterUS1.7k papers
- Purdue University West LafayetteUS1.6k papers
- Johns Hopkins UniversityUS1.6k papers
- University of Maryland, College ParkUS1.6k papers
- The Ohio State UniversityUS1.6k papers
- University of California, Santa BarbaraUS1.6k papers
10 papers · 2 filters
PSR J1841-0500: a radio pulsar that mostly is not there
F. Camilo, S. M. Ransom, S. Chatterjee +2
In a search for radio pulsations from the magnetar 1E 1841-045, we have discovered the unrelated pulsar J1841-0500, with rotation period P=0.9 s and characteristic age 0.4 Myr. One…
Fullerenes in circumstellar and interstellar environments
Jan Cami, Jeronimo Bernard-Salas, Els Peeters +1
We recently identified several emission bands in the Spitzer-IRS spectrum of the unusual planetary nebula Tc 1 with the infrared active vibrational modes of the neutral fullerene s…
The Magnetic Field in Taurus Probed by Infrared Polarization
Nicholas L. Chapman, Paul F. Goldsmith, Jorge L. Pineda +3
We present maps of the plane-of-sky magnetic field within two regions of the Taurus molecular cloud: one in the dense core L1495/B213 filament, the other in a diffuse region to the…
The Herschel M33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302
B. Mookerjea, C. Kramer, C. Buchbender +19
Context: The emission line of [CII] at 158 micron is one of the strongest cooling lines of the interstellar medium (ISM) in galaxies. Aims: Disentangling the relative contributions…
Minimum Requirements for Detecting a Stochastic Gravitational Wave Background Using Pulsars
J. M. Cordes, R. M. Shannon
We assess the detectability of a nanohertz gravitational wave (GW) background with respect to additive red and white noise in the timing of millisecond pulsars. We develop detectio…
On the Formation of CO2 and Other Interstellar Ices
Robin T. Garrod, Tyler Pauly
We investigate the formation and evolution of interstellar dust-grain ices under dark-cloud conditions, with a particular emphasis on CO2. We use a three-phase model (gas/surface/m…
Formation of Massive Black Holes in Dense Star Clusters. II. IMF and Primordial Mass Segregation
Sanghamitra Goswami, Stefan Umbreit, Matt Bierbaum +1
A promising mechanism to form intermediate-mass black holes (IMBHs) is the runaway merger in dense star clusters, where main-sequence stars collide and form a very massive star (VM…
An Arecibo Search for Pulsars and Transient Sources in M33
N. D. R. Bhat, J. M. Cordes, P. J. Cox +4
We report on a systematic and sensitive search for pulsars and transient sources in the nearby spiral galaxy M33, conducted at 1.4 GHz with the Arecibo telescope's seven-beam recei…
Arecibo PALFA Survey and Einstein@Home: Binary Pulsar Discovery by Volunteer Computing
B. Knispel, P. Lazarus, B. Allen +35
We report the discovery of the 20.7 ms binary pulsar J1952+2630, made using the distributed computing project Einstein@Home in Pulsar ALFA survey observations with the Arecibo tele…
The GALFA-HI Survey: Data Release 1
J. E. G. Peek, Carl Heiles, Kevin A. Douglas +10
We present the Galactic Arecibo L-Band Feed Array HI (GALFA-HI) survey, and its first full data release (DR1). GALFA-HI is a high resolution (~ 4'), large area (13000 deg^2), high…