Index
-
AB magnitude F.4, 2.1
-
aberration
-
absorption 2.1, 2.2.1
-
accretion disk 5.6.2
-
action 7.1
-
active galactic nucleus 5.1
-
Airy pattern 3.3.2
-
aliasing A.3
-
ALMA 1.1.2, 2.8, Figure 8.5
-
ampere F.3
-
angular frequency 2.3, 3.1.1
-
antenna 3.1—3.1.6
-
alt-az mount 3.5
-
aperture 3.2.2, 3.2.3
-
aperture
efficiency 3.3.2
-
average collecting area 3.1.4
-
average gain 3.1.3
-
beam
efficiency 3.1.6
-
beam
solid angle 3.3.3
-
beam pattern 3.2.3
-
beam solid angle 3.1.3, 3.1.4
-
beamwidth 3.2.4
-
collecting area 3.1.4
-
current 3.1.1
-
diffraction limit 3.2.4
-
dipole 3.1.1
-
directivity 3.1.3
-
effective collecting area 3.1.4
-
efficiency 3.1.3
-
electric field pattern 3.2.3
-
equatorial mount 3.5
-
feed 3.1.1, 3.2.1
-
Fraunhofer approximation 3.2.3
-
gain 3.1.3
-
ground-plane
vertical 3.1.1
-
homologous 3.5
-
Huygens’s principle 3.2.3
-
illumination 3.2.3
-
isotropic 3.1.3
-
kelvins per
jansky 3.1.6
-
main
beam
-
main beam 3.1.6, 3.2.4
-
nulls 3.2.4
-
pointing accuracy 3.3.5
-
power
gain 3.1.3
-
power gain 3.1.5
-
power pattern 3.1.1
-
radiation
resistance 3.1.2
-
reciprocity theorem 3.1.5
-
reflector 3.2—3.2.5
-
resolving power 3.2.4
-
resonant 3.1.1, 3.1.2
-
sidelobes Figure 3.42, 3.1.6, 3.2.4
-
stray radiation 3.1.6
-
subreflector
-
temperature 2.5, 3.1.6
-
tracking error 3.3.5
-
waveguide
horn Figure 3.27
-
waveguide horn 2.6.3, 3.1.1, 3.2.1, 3.2.3, 3.3.2, 3.5, 3.5
-
Antennae Galaxies Figure 8.12
-
aperture 3.2.2, 3.2.3
-
aperture efficiency 3.3.2
-
aperture synthesis 3.7.4
-
Arecibo
Observatory Figure 8.2
-
ASKAP Figure 8.6
-
astronomical unit F.2, 1.3
-
atmosphere 2.2.3
-
atmospheric windows 1.1.2
-
autocorrelation A.7
-
autocorrelation
spectrometer 3.6.5
-
azimuth 1.2
-
bandwidth 3.6.2
-
bandwidth smearing 3.7.3
-
baryon/photon ratio 2.6.3
-
baryonic matter 2.6.1
-
beam
-
birefringent D.2
-
black
hole
-
black hole
-
blackbody 2.4
-
blackbody
radiation
-
integrated brightness 2.4.2
-
mode 2.4.1, 2.4.1
-
polarization 5.
-
Rayleigh–Jeans approximation 2.4.1
-
specific intensity 2.4.1
-
Stefan–Boltzmann constant B.2
-
Stefan–Boltzmann law B.2
-
ultraviolet catastrophe 3.
-
Wien’s law 2.4.2
-
blackbody radiation 2.4—2.4.2
-
Bohr atom 7.2.1
-
Bohr magneton 7.8
-
Bohr radius F.1, 4.2, 7.2.1
-
Boltzmann distribution 2.4.1
-
Boltzmann equation 7.3.1, 7.3.2
-
Boltzmann’s constant F.1
-
bremsstrahlung 4.1
-
brightness 2.1—2.1
-
brightness
temperature 2.2.3
-
brightness sensitivity 3.7.6
-
brightness temperature
-
calorimeter model 5.6.3
-
canonical neutron star 6.1.2
-
carbon monoxide (CO) 2., 7.7.1, 7.7.1
-
Cas A Figure 1.14, 3.5, Figure 5.13
-
Cassegrain
subreflector Figure 3.21, 3.5
-
Cassegrain subreflector 3.5
-
cavity
radiation 2.4
-
CGS units F.3
-
Chandrasekhar mass 6.1.2
-
CO conversion factor 7.7.3
-
coherent
-
collisional broadening 7.2.2
-
collisional excitation 7.4
-
column density 7.3.2, 7.8, 7.8.2
-
complex exponentials B.3
-
Compton thick 1.1.1, 1.1.4
-
conductivity D.1, D.2
-
confusion 3.6.3
-
confusion limit 3.6.3
-
constants Appendix F—F.6
-
convolution A.7
-
correlator 3.7.1
-
correspondence principle 7.2.2
-
cosmic microwave
background
-
blackbody spectrum 2.6.3
-
expansion scale factor 2.6.2
-
flatness problem 2.6.5
-
recombination era 2.6.2
-
surface of last scattering 2.6.2
-
cosmic microwave background 2.6—2.6.5
-
cosmic rays 5.2
-
Coulomb’s law 2.7
-
counterjet 5.6.1
-
Crab
Nebula 6.1.2
-
Crab Nebula Figure 8.10
-
critical frequency 5.3.1
-
cross-correlation A.7, A.7
-
current 3.1.1, 3.1.2
-
current density D.1
-
curvature
radiation 6.1.10
-
cyclotron
radiation 5.1
-
Cyg
A 1.3
-
Cyg A Figure 5.13, 5.4.3
-
dark ages 7.8.3
-
De
Broglie wavelength 7.1
-
debye 7.7.3
-
Debye length 4.2, 4.3.2
-
decibel (dB) F.4, 3.1.3
-
declination 5.6.4
-
declination axis 3.5
-
delta function 5.3.1
-
density-bounded Hii region 4.2
-
detailed balance 7.3.1
-
diffraction 3.2.4, 3.7
-
diffraction
limited 3.2.4
-
dimension F.6
-
dimensional analysis F.6
-
dipole
moment 7.7.3
-
dipole anisotropy 2.6.4
-
dipole antenna 3.1.1
-
directivity 3.1.3
-
dispersion 3.4
-
dispersion
delay 6.2
-
dispersion measure (DM) 6.2
-
Doppler
shift
-
Doppler shift
-
dust 2.8—2.8, 5.4.2, 5.6.2, 5.6.3
-
ecliptic
latitude 6.3
-
ecliptic plane 6.3
-
Eddington luminosity 5.4.2
-
Einstein
coefficients
-
Einstein coefficients
-
spontaneous emission 7.3.1
-
stimulated emission 7.3.1
-
electric field 2.7
-
elevation angle 3.5
-
emission 2.1
-
emission coefficient 2.2.2, 2.2.4
-
emission measure
(EM) 4.3.2
-
energy
density
-
energy density
-
epoch of
reionization 7.8.3
-
equilibrium radiation 2.4
-
equipartition 5.4.1, 5.4.1
-
Euler’s formula B.3
-
event C.1
-
excitation temperature 7.4—7.4
-
extinction 2.8
-
far-field
distance 3.2.2
-
Faraday depolarization D.2
-
Faraday rotation D.2—D.2
-
filter
bank 3.6.5
-
fine-structure
constant 7.8
-
flatness problem 2.6.5
-
flux
-
flux density 2.1
-
Fourier
transforms
-
autocorrelation A.7
-
convolution theorem A.7
-
cross-correlation A.7
-
derivative theorem A.6
-
Euler’s formula A.1
-
inverse A.1
-
modulation theorem A.6
-
Nyquist frequency A.3
-
similarity theorem A.6
-
Fourier transform spectrometer 3.6.5
-
Fourier transforms A.1—A.8, 3.2.3
-
addition
theorem A.6
-
aliasing A.3
-
bandwidth A.3
-
complex
exponential A.1
-
convolution A.7
-
cross-correlation A.7
-
cross-correlation theorem A.7
-
discrete Fourier transform (DFT) A.2
-
fast Fourier transform (FFT) A.2
-
forward A.1
-
power spectrum A.4
-
Rayleigh’s
theorem A.4
-
sampling theorem A.3
-
shift
theorem A.6
-
similarity theorem 3.2.4
-
Wiener–Khinchin
theorem A.7
-
free–free
emission
-
free–free emission 4.3—4.3.2
-
gain
-
Galactic
latitude 1.3
-
Galactic longitude 1.3, Figure 7.18
-
galaxies
-
Galilean relativity C.1
-
Galilean transform C.1
-
Gaunt
factor 4.3.2
-
Gaussian
-
Gaussian CGS F.3
-
GBT (Green Bank
Telescope) Figure 8.1
-
gravitational waves 6.3
-
Gregorian
subreflector Figure 3.27, 3.5
-
Gregorian subreflector Figure 3.24, 3.5, 3.5
-
group velocity D.1, 6.2
-
gyro
frequency D.2
-
gyro
radiation 5.1
-
gyro frequency 5.1.1
-
Her
A Figure 8.14
-
Hi 21-cm line
-
Hi 21-cm line 7.8—7.8.3
-
Bohr magneton 7.8
-
column density 7.8
-
epoch of
reionization 7.8.3
-
fine-structure
constant 7.8
-
hyperfine line 7.8
-
kinematic
distance 7.8.1
-
line flux 7.8.2
-
nuclear factor 7.8
-
rotation curve 7.8.2
-
spin temperature 7.8
-
Hii regions
-
density bounded 4.2
-
free–free radiation 4.2
-
Strömgren sphere 4.2
-
thermal emission 4.1
-
ultra-compact (UC) 4.2
-
ultra-dense (UD) 4.2
-
Hii regions 4.2—4.2
-
emission measure (EM) 4.3.2
-
ionization bounded 4.2
-
matter
bounded 4.2
-
recombination rate 4.2
-
temperature 4.2
-
HL Tau Figure 8.9
-
horizon problem 2.6.5
-
hotspot 5.6.1
-
hour angle 3.5
-
hour-angle axis 3.5
-
Hubble
constant 2.6.1
-
Hubble constant F.2, 7.8.2
-
Hubble distance 2.6.1
-
Hubble time 2.6.1
-
hydrosols 3.
-
hyperfine
line 7.8
-
ideal gas law 7.1
-
impact parameter Figure 4.2
-
index of refraction D.1
-
inflation 2.6.5
-
initial mass function (IMF) 4.2
-
intensity
-
interferometer 3.7—3.7.6
-
interstellar
medium (ISM)
-
interstellar medium
(ISM)
-
dispersion measure (DM) 6.2
-
magnetic field 5.6.3
-
phases 7.1
-
scintillation 6.2
-
interstellar medium (ISM)
-
inverse Compton
(IC)
-
maximum frequency 5.5.2
-
net radiated power 5.5.1
-
synchrotron self-Compton 5.5.3
-
inverse Compton (IC) 5.5—5.5.3
-
average frequency 5.5.2
-
brightness
limit 5.5.3
-
IC/synchrotron power
ratio 5.5.1
-
inverse square law 2.1
-
ionization
bounded 4.2
-
ionosphere D.1, 1.1.1
-
isotopologue 7.7.3
-
jansky (Jy) 2.1
-
Jansky, Karl Guthe Figure 1.7, 1.2
-
Kirchhoff’s
law 2.2.4
-
Kirchhoff’s law 2.2.2
-
Larmor
radiation 2.7
-
Larmor’s equation 2.7
-
recombination lines 7.2.2
-
synchrotron spectrum 5.3.1
-
Larmor radiation 2.7—2.7
-
antenna 3.1.1
-
free–free 4.3.1
-
recombination lines 4.2
-
rotating
electric dipole 6.1.4
-
rotating magnetic dipole 6.1.4
-
rotating polar molecule 7.7.3
-
synchrotron power 5.2.3
-
Thomson
scattering 5.5.1
-
length contraction C.2
-
line
profile
-
line
trapping 7.7.3
-
line
width
-
line flux 7.8.2
-
line profile 7.2.2
-
line width 7.2.2
-
collisional
broadening 7.2.2
-
Doppler
broadened 1.
-
natural 7.2.2
-
load 2.5, 2., 3.6.6
-
local oscillator (LO) 3.6.4
-
local thermodynamic
equilibrium (LTE) 2.2.2
-
LOFAR Figure 8.8
-
Lorentz factor C.1, 5.2.1
-
Lorentz force 6.1.10
-
Lorentz transform Appendix C—C.4
-
luminosity
-
M81 group Figure 8.11
-
M82 Figure 2.24, 5.3.3, 5.6.3, Figure 8.13
-
magnetic
dipole
-
magnetic dipole
-
magnetic energy density (5.35)
-
magnetic force 5.1.1
-
magnetobremsstrahlung 5.1—5.1.1
-
curvature
radiation 6.1.10
-
cyclotron radiation 5.1
-
gyro radiation 5.1
-
synchrotron radiation 5.1
-
magnitude (AB) F.4, 2.1
-
maser 5., 7.5—7.5
-
mass–energy equation 5.2.2
-
matter-bounded
Hii region 4.2
-
Maxwell’s equations Appendix D
-
Maxwellian distribution B.8, 4.1, 4.3.2
-
meridian 3.5
-
metals 4.2
-
mixer 3.6.4
-
MKS units F.3
-
molecular lines 7.7—7.7.3
-
molecule
-
moment of inertia 6.1.5
-
MWA 7.8.3, Figure 8.7
-
negative absorption 7.3.1
-
neutron star 6.1, 6.1.2
-
NGC 4258 7.5
-
noise
temperature
-
noise factor 3.6.6
-
noise figure 3.6.6
-
noise temperature
-
nonthermal
emission 4.1
-
Nyquist approximation 2.5
-
Nyquist formula 2.5
-
observable universe 2.6.5
-
ohm F.3
-
Ohm’s law D.1, 3.1.2
-
opacity 2.2.1
-
opaque body 2.2.4
-
optical depth 2.2.1
-
optical velocity convention 7.8.2
-
optically thick 2.2.1
-
optically thin 2.2.1
-
PAPER 7.8.3
-
paraboloid Figure 3.7
-
parsec F.2, 1.2
-
Parseval’s theorem A.4
-
permeability of free space F.3
-
permittivity of free space F.3
-
phase
(interferometer fringe) 3.7.1
-
phase (interferometer
fringe) Figure 3.41
-
phase velocity 3.4
-
phases of interstellar medium 7.1
-
photon 2.4.2
-
pitch
angle 5.2.3
-
pitch angle 5.2.3, 5.3.1
-
Planck’s constant F.1, 2.4.2
-
Planck’s law 2.4.2
-
planetary nebula 2., 4.2
-
plasma
-
polarization 2.3—2.3
-
post-Keplerian (PK) parameters 6.3
-
power
spectrum
-
power spectrum A.4
-
autocorrelation A.7
-
radiometer
postdetection 3.6.3
-
synchrotron 5.3.1
-
Poynting flux 2.7
-
pressure
-
equipartition 5.6.1
-
ideal gas 7.1
-
interstellar medium 7.1
-
line broadening 2.
-
radiation 5.4.2
-
principal quantum number 4.2, 7.2.1
-
protoplanetary disk 2.8, Figure 8.9
-
pulsar 6.1—6.3
-
pulsar
timing
-
pulse phase 6.3
-
timing residuals 6.3
-
pulsar timing 2., 6.3—6.3
-
average pulse profile 6.3
-
Einstein delay 6.3
-
Keplerian parameters 6.3
-
post-Keplerian (PK)
parameters 6.3
-
pulsar timing array
(PTA) 6.3
-
Roemer
delay 6.3
-
Shapiro delay 6.3
-
time of arrival
(TOA) 6.3
-
topocentric
frame 6.3
-
pwv 4.
-
quantum
noise 1.1.5
-
quantum
number
-
quantum noise 1.1.1
-
quantum number
-
quasi-stellar object (QSO) 5.6.2
-
radial velocity 7.2.2
-
radiation
-
radiation constant 2.4.2
-
radiation resistance
-
radiative transfer equation 2.2.2
-
radio
telescopes
-
radio astronomy 1.1.1
-
radio frequencies 1.1.1
-
radio telescopes
-
radio velocity convention 7.8.2
-
radiometer 2.5, 3.6—3.6.6
-
ray optics approximation 2.1
-
Rayleigh
scattering 2.8
-
Rayleigh distribution 3.3.5
-
Rayleigh resolution
criterion 3.2.4
-
Rayleigh–Jeans approximation 2.4.1
-
reciprocity theorem 3.1.5
-
recombination
coefficient 4.2
-
recombination
lines 7.2.2
-
collisional broadening 7.2.2
-
spontaneous emission rate 7.2.2
-
recombination
rate 4.2
-
recombination era 2.6.2
-
recombination lines 7.2—7.2
-
recombination time 4.2
-
redshift 2.6.2
-
reflection coefficient 2.2.4
-
refraction D.1
-
refractive index D.1, D.2
-
relativistic aberration 5.3.1
-
relativistic beaming 5.2.2, 5.3.1, 5.6.2
-
relativity Appendix C—C.4
-
relativity principle C.1
-
resistance 3.1.2
-
resistor 2.4, 2.5
-
resolution
-
resolving
power 3.2.4
-
RFI 4.
-
right
ascension Figure 6.1
-
Roemer delay 6.3
-
rotation curve 7.8.1, 7.8.2
-
rotation measure (RM) D.2
-
RRAT Figure 6.3, 6.1.9
-
Ruze
equation 3.3.4
-
Rydberg
constant 7.2.1
-
Rydberg frequency 4.2, 7.2.1
-
Saha equation 7.6.1
-
sampling theorem A.3, 3.6
-
scattering 2.1
-
scintillation
-
sensitivity
-
shah function A.5, 5.3.1
-
Shapiro delay 6.3
-
SI units F.3, F.3
-
sidelobes 3.1.6
-
sidereal day 1.2
-
sinc function 3.2.4
-
SMBH 10., 2., 1.1.4, 1.3, 5.4.2, 5.4.3, 7.5
-
solar luminosity F.2
-
solar mass F.2
-
special
relativity
-
special relativity Appendix C—C.4
-
aberration 5.3.1
-
Doppler boosting 5.6.1
-
energy C.4
-
event C.1
-
Galilean relativity C.1
-
Galilean transform C.1
-
invariant speed C.1
-
length contraction C.2
-
Lorentz
transform C.1
-
Lorentz factor C.1
-
mass C.4
-
power C.4
-
relativistic
beaming 5.2.2, 5.3.1
-
superluminal velocities 5.6.1
-
time dilation C.2
-
velocity addition C.3
-
specific
intensity 2.1
-
spectral brightness 2.1
-
spectral index 4.3.2
-
spectral lines 7.1—7.8.3
-
spectrometer 3.6.5—3.6.5
-
autocorrelation spectrometer 3.6.5
-
channel 3.6.5
-
filter bank 3.6.5
-
Fourier
transform spectrometer 3.6.5
-
spillover 5., 3.2.5
-
spontaneous emission coefficient 7.3.1
-
spontaneous emission rate 7.2.2
-
square-law
detector 3.6
-
square-law detector B.6
-
stationary source 3.7.1
-
statistical weights 7.3.1, 7.8
-
Stefan–Boltzmann
constant 2.4.2
-
Stefan–Boltzmann constant B.2
-
Stefan–Boltzmann law B.2, 2.4.2
-
steradian (sr) F.4
-
stimulated emission 7.3.1
-
stimulated emission coefficient 7.3.1
-
Stokes parameters 2.3
-
Strehl ratio 3.3.4
-
Strömgren
radius 4.2
-
Strömgren radius Figure 4.1
-
Strömgren sphere Figure 4.1, 4.2
-
superluminal velocities 5.6.1
-
supermassive
black hole 5.4.2
-
supermassive black
hole 1.3
-
supermassive black hole 10., 2., 1.1.4, 5.4.3, 7.5
-
synchrotron
radiation
-
synchrotron radiation 5.1—5.4.3
-
temperature
-
thermal emission 4.1
-
thermodynamic equilibrium 2.2.2
-
local thermodynamic
equilibrium 2.2.2
-
Thomson cross
section 5.2.3, 5.5.1
-
Thomson scattering 5.2.3, 5.5, 5.5.1
-
time dilation C.2
-
Tully–Fisher relation 7.8.2
-
ultraviolet catastrophe 3.
-
unit rectangle function 3.2.4
-
units F.3—F.3
-
() plane 3.7.4
-
() plane Figure 3.44
-
variance 3.6.3
-
velocity
convention
-
vertex Figure 3.21, Figure 3.24, Figure 3.7, 1., 3.5
-
Vir A Figure 5.13, 5.4.3
-
VLA Figure 8.4
-
voltage 3.1.2
-
wave vector 2.3
-
waveguide 3.4
-
white dwarf star 6.1.2
-
Wien’s displacement law 2.4.2
-
Wiener–Khinchin theorem A.7
-
WSRT Figure 8.3
-
factor 3.6.6
-
zenith 1.1.2
-
zenith angle 2.2.3, 2.2.3
-
zenith opacity 1.1.2