Astronomy & Celestial Mechanics
the sky, computed
Concept

Damped random walk — where it appears

A random process that takes small random steps while being pulled back towards its mean, so it wanders without drifting away. Its one characteristic time, over which it forgets its past, describes the optical flicker of quasars well.

Named by 2 essays across 2 fields — each of them below, with the objects they name alongside it.

A 20-day delay, recovered at 20 days from two curves that share no wavelength. Above: a quasar's continuum, drawn as a damped random walk with a 90-day damping time, and the broad emission line responding to it. The line curve is the continuum convolved with a top-hat response of half-width 20 days, so it is later and smoother — it varies only 51 per cent as much, because at any instant it is an average of the continuum over a range of light-travel times. Below: the cross-correlation of the two, which peaks at 20 days. That number is a length: 20 light-days is 5.2·10¹⁴ metres, or 3463 astronomical units, and it has been measured for an object that subtends 3.5·10⁻⁵ arcseconds at a hundred megaparsecs — some thirty times finer than the best optical interferometry has ever resolved anything, and reached here with a photometer and a clock. The irregularity of the continuum is what makes this work. A periodic source would give a cross-correlation with many equal peaks and no way to choose; a random one gives a single peak, and the whole method rests on active nuclei being erratic.

A size measured from a delay

An active nucleus at redshift two is a point source in every telescope ever built, and its central mass is measured anyway. The continuum varies, the broad lines follow days later, and the lag is a light-travel time — which is a length, recovered from two light curves that share no wavelength.

galaxies · Quasars Three reasons the flicker slows with redshift, only one of them cosmology. The observed flicker timescale of the faintest quasars a flux-limited survey can see, relative to its value at redshift 0.2, logarithmic, separated into its causes: time dilation alone (a factor 5.0 by redshift 4); the bluer rest-frame wavelength a fixed band samples at higher redshift, which shortens the timescale (×0.78); and the heavier black holes the flux limit selects (×15.3). Together, ×49.9. Read as a power of (1+z) the total has exponent 2.74 where dilation alone has 1.00: a test that does not hold mass and wavelength fixed measures the selection, not the expansion.

A clock that flickers without a tick

If the universe expands, every process seen at redshift z runs (1+z) times slow. A supernova carries a calibrated clock and shows it. A quasar's light wanders with no period at all, and its characteristic timescale grows with the mass of its black hole and shrinks with the colour it is seen in, both of which change with redshift in any real survey. Reading the dilation from quasars means holding those fixed first, and on a short enough baseline the measurement hides the effect it is looking for.

cosmology · Expansion

Named alongside it

The objects these essays reach for when they reach for this one.

Accretion discBroad-line regionContinuum variabilityCross-correlationEddington ratioLight-travel timeLuminosity distanceMalmquist biasQuasarQuasarsRadius luminosity relationReverberation mapping

All concepts