No matter the form, half-celestials are always comely and delightful to the senses, having golden skin, sparkling eyes, angelic wings, or some other sign of their higher nature.
Creating A Half-Celestial
"Half-celestial" is an inherited template that can be added to any living, corporeal creature with an Intelligence score of 4 or higher and nonevil alignment (referred to hereafter as the base creature).
A half-celestial uses all the base creature’s statistics and special abilities except as noted here.
Size and Type
The creature’s type changes to outsider. Do not recalculate the creature’s Hit Dice, base attack bonus, or saves. Size is unchanged. Half-celestials are normally native outsiders.
A half-celestial has feathered wings and can fly at twice the base creature’s base land speed (good maneuverability). If the base creature has a fly speed, use that instead.
Natural armor improves by +1 (this stacks with any natural armor bonus the base creature has).
A half-celestial retains all the special attacks of the base creature and also gains the following special abilities.
Half-celestials can use a daylight effect (as the spell) at will.
Smite Evil (Su)
Once per day a half-celestial can make a normal melee attack to deal extra damage equal to its HD (maximum of +20) against an evil foe.
A half-celestial with an Intelligence or Wisdom score of 8 or higher has two or more spell-like abilities, depending on its Hit Dice, as indicated on the table below. The abilities are cumulative
Unless otherwise noted, an ability is usable once per day. Caster level equals the creature’s HD, and the save DC is Charisma-based.
A half-celestial has all the special qualities of the base creature, plus the following special qualities.
Increase from the base creature as follows: Str +4, Dex +2, Con +4, Int +2, Wis +4, Cha +4.
A half-celestial gains skill points as an outsider and has skill points equal to (8 + Int modifier) × (HD +3). Do not include Hit Dice from class levels in this calculation—the half-celestial gains outsider skill points only for its racial Hit Dice, and gains the normal amount of skill points for its class levels. Treat skills from the base creature’s list as class skills, and other skills as cross-class.
HD 5 or less, as base creature +1; HD 6 to 10, as base creature +2; HD 11 or more, as base creature +3.
Always good (any).
Same as base creature +4.
We present WMAP seven-year observations of bright sources which are often used as calibrators at microwave frequencies. Ten objects are studied in five frequency bands (23-94 GHz): the outer planets (Mars, Jupiter, Saturn, Uranus, and Neptune) and five fixed celestial sources (Cas A, Tau A, Cyg A, 3C274, and 3C58). The seven-year analysis of Jupiter provides temperatures which are within 1 sigma of the previously published WMAP five-year values, with slightly tighter constraints on variability with orbital phase (0.2% +/- 0.4%), and limits (but no detections) on linear polarization. Observed temperatures for both Mars and Saturn vary significantly with viewing geometry. Scaling factors are provided which, when multiplied by the Wright Mars thermal model predictions at 350 mu m, reproduce WMAP seasonally averaged observations of Mars within similar to 2%. An empirical model is described which fits brightness variations of Saturn due to geometrical effects and can be used to predict the WMAP observations to within 3%. Seven-year mean temperatures for Uranus and Neptune are also tabulated. Uncertainties in Uranus temperatures are 3%-4% in the 41, 61, and 94 GHz bands; the smallest uncertainty for Neptune is 8% for the 94 GHz band. Intriguingly, the spectrum of Uranus appears to show a dip at similar to 30 GHz of unidentified origin, although the feature is not of high statistical significance. Flux densities for the five selected fixed celestial sources are derived from the seven-year WMAP sky maps and are tabulated for Stokes I, Q, and U, along with polarization fraction and position angle. Fractional uncertainties for the Stokes I fluxes are typically 1% to 3%. Source variability over the seven-year baseline is also estimated. Significant secular decrease is seen for Cas A and Tau A: our results are consistent with a frequency-independent decrease of about 0.53% per year for Cas A and 0.22% per year for Tau A. We present WMAP polarization data with uncertainties of a few percent for Tau A. Where appropriate, WMAP results are compared against previous findings in the literature. With an absolute calibration uncertainty of 0.2%, WMAP data are a valuable asset for calibration work.
CitationWeiland, J. L., N. Odegard, R. S. Hill, E. Wollack, G. Hinshaw, M. R. Greason, N. Jarosik et al. "Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Planets and Celestial Calibration Sources. APJS 192, 19. doi: 10.1088." arXiv preprint arXiv:1001.4731 (Feb., 2011).Sours: https://repositories.lib.utexas.edu/handle/2152/42999
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Free-to-Play award winning action RPG. Immerse in an epic story with classic MMO and role-playing elements. Enter the fantastic world of Althea.
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