C. F. Astrophysics

发表

BATSE Observations of Gamma-Ray Burst Spectra. IV. Time-resolved High-Energy Spectroscopy

Huntsville, Al., NASAMarshall Space Flight Center, 1997, astro-ph/9711153.

DEMOGRAPHICS AND PHYSICAL PROPERTIES OF GAS OUTFLOWS/INFLOWS AT 0.4 < z < 1.4

Astronomy, D. O. Astronomy, B. Weiner, 2012, 1206.5552.

Direct Detection of Cold Dark Matter Substructure

Ucsd, C. Physics, C. F. Astrophysics, 2001, astro-ph/0111456.

Superhumps in Cataclysmic Binaries. XXIII. V442 Ophiuchi and RX J1643.7+3402

J. Thorstensen, E. Beshore, D. O'donoghue, 2002, astro-ph/0211615.

NOVA-LIKE CATACLYSMIC VARIABLES IN THE INFRARED

Heidelberg, Seattle, Boulder, 2014, 1403.6601.

Formation of millisecond pulsars. I. Evolution of low-mass X-ray binaries with P_orb> 2 days

University of Amsterdam, G. J. Savonije, T. Tauris, 1999 .

Extreme HBL behavior of Markarian 501 during 2012

India., Ireland, Newark, 2018, Astronomy & Astrophysics.

1–2.4 μm Near-IR Spectrum of the Giant Planet β Pictoris b Obtained with the Gemini Planet Imager

Lunar, Arizona State University, Cosmology, 2017, 1703.00011.

Acoustic wave propagation in the solar atmosphere. V. Observations versus simulations

Heidelberg, H Germany, Usa, 1997, astro-ph/9704067.

A SEARCH FOR PULSATIONS FROM GEMINGA ABOVE 100 GeV WITH VERITAS

Cambridge, Ireland, Newark, 2014, 1412.4734.

Noise from undetected sources in Dark Energy Survey images

Astronomy, University College London, Lsst, 2020, Monthly Notices of the Royal Astronomical Society.

An HST Survey of the mid-UV Morphology of Nearby Galaxies

Nasa, Caltech, C. Conselice, 2002, astro-ph/0204398.

A COMPREHENSIVE SPECTRAL ANALYSIS OF THE X-RAY PULSAR 4U 1907+09 FROM TWO OBSERVATIONS WITH THE SUZAKU X-RAY OBSERVATORY

Technology, A. Markowitz, K. Pottschmidt, 2009, 0912.3023.

The 2009 multiwavelength campaign on Mrk 421: variability and correlation studies

Engineering, Landessternwarte, Cambridge, 2015, 1502.02650.

Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven Hα Filaments

Astrophysics, Astronomy, L. Ho, 2022, The Astrophysical Journal Letters.

Estimation of Carbon Abundances in Metal-Poor Stars. I. Application to the Strong G-Band Stars of Beers, Preston, and Shectman

Caltech, T. Beers, Brazil., 2005, astro-ph/0508202.

Peaks in the Cosmic Microwave Background: Flat versus Open Models

Berkeley, Instituto de Fisica de Cantabria, R. B. Barreiro, 1996, astro-ph/9612114.

Effects of model incompleteness on the drift-scan calibration of radio telescopes

Cambridge, Arizona State University, National Radio Astronomy Observatory, 2021, Monthly Notices of the Royal Astronomical Society.

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Tucson, India., Cambridge, 2016, 1612.09472.

Unprecedented study of the broadband emission of Mrk 421 during flaring activity in March 2010

Tucson, Engineering, Landessternwarte, 2014, 1412.3576.

The X-ray emission of the most luminous 3CR radio sources

P. Véron, M. Salvati, G. Risaliti, 2007, 0710.5220.

SPECTRAL ENERGY DISTRIBUTIONS OF 3C 279 REVISITED: BeppoSAX OBSERVATIONS AND VARIABILITY MODELS

Astrophysics, Milano, Merate, 2001, astro-ph/0111499.

Detection of chloronium and measurement of the Cl-35/Cl-37 isotopic ratio at z=0.89 toward PKS 1830-211

Technology, Hanoi, King Abdulaziz University, 2014, 1404.7668.

An ALMA Early Science survey of molecular absorption lines toward PKS 1830−211 - Analysis of the absorption profiles

Santiago, National Radio Astronomy Observatory, Technology, 2014, 1404.7667.

Detection of magnetic helicity

Case Western Reserve University, C. F. Astrophysics, T. Kahniashvili, 2005, astro-ph/0511373.

Dissipation in Compressible Magnetohydrodynamic Turbulence

E. Ostriker, C. Gammie, J. Stone, 1998, astro-ph/9809357.

NUCLEAR X-RAY PROPERTIES OF THE PECULIAR RADIO-LOUD HIDDEN AGN 4C+29.30

Usa, D. Evans, Dc, 2012, 1208.4581.

Precession during merger: Strong polarization changes are observationally accessible features of strong-field gravity during binary black hole merger

J. Healy, L. London, R. O’Shaughnessy, 2012, 1209.3712.

Q2237+0305 source structure and dimensions from light‐curve simulation

Cambridge, Kharkov, Ukraine, 2007, 0708.1082.

Apsidal Alignment and Anti-Alignment of Planets in Mean-Motion Resonance: Disk-Driven Migration and Eccentricity Driving

Ny, Ithaca, C. University, 2022, 2206.04810.

Hydrodynamics and survivability during post-main-sequence planetary engulfment

Astrophysics, Berkeley, Statistics, 2022, 2203.11227.

SEPARATING THE X-RAY EMISSIONS OF UV CETI A AND B WITH CHANDRA

Paul Scherrer Institut, M. Audard, U. Colorado, 2003, astro-ph/0303492.

Spectral Energy Distributions of 3C 279 Revisited: BeppoSAX Observations and Variability Models

Astrophysics, Milano, Merate, 2001, astro-ph/0111499.