| /dports/astro/astrometry/astrometry.net-0.85/doc/ |
| H A D | build-index.rst | 105 example, doing an initial photometric calibration by tagging-along one
106 or more bands of photometric data for each astrometric star.
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| /dports/astro/celestia-gtk/celestia-1.6.1/ |
| H A D | ChangeLog | 1048 * Added Lunar-Lambert photometric model (linear combination of Lambert and
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| H A D | README | 331 at Lowell Observatory. Buie's maps were generated from photometric data
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| /dports/astro/celestia-gtk/celestia-1.6.1/data/ |
| H A D | galaxies.dsc | 43 # cep=Cepheids, P=photometric, N(G)=planetary nebula (globular cluster) luminosity function
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| /dports/astro/celestia/celestia-1.6.1/ |
| H A D | ChangeLog | 1048 * Added Lunar-Lambert photometric model (linear combination of Lambert and
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| H A D | README | 331 at Lowell Observatory. Buie's maps were generated from photometric data
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| /dports/astro/celestia/celestia-1.6.1/data/ |
| H A D | galaxies.dsc | 43 # cep=Cepheids, P=photometric, N(G)=planetary nebula (globular cluster) luminosity function
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| /dports/astro/gnuastro/gnuastro-0.16/doc/ |
| H A D | gnuastro.info-2 | 4435 example finding the stellar mass or photometric redshift from magnitudes
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| H A D | gnuastro.info-3 | 1721 ## also sort the rows by the input's photometric redshift (`Z_PHOT')
1726 ## Similar to the above, but only print rows that have a photometric
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| H A D | gnuastro.texi | 8520 …tep for higher-level analysis, for example finding the stellar mass or photometric redshift from m…
11157 ## also sort the rows by the input's photometric redshift (`Z_PHOT')
11162 ## Similar to the above, but only print rows that have a photometric
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| /dports/astro/kstars/kstars-3.5.6/doc/ |
| H A D | colorandtemp.docbook | 89 photometric system is called the <firstterm>Johnson UBV
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| H A D | ellipticalgalaxies.docbook | 92 blue. Thehave photometric colors of B-V = 0.0 to 0.30 mag, which is
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| /dports/astro/kstars/kstars-3.5.6/po/en_GB/docs/kstars/ |
| H A D | colorandtemp.docbook | 64 …rum of light to pass through while rejecting all others. A widely used photometric system is calle…
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| H A D | ellipticalgalaxies.docbook | 79 >Small galaxies that are unusually blue. Thehave photometric colors of B-V = 0.0 to 0.30 mag, which…
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| /dports/astro/p5-Astro-ADS/Astro-ADS-1.26/t/ |
| H A D | query.t | 206 %B We present a comprehensive photometric data set taken over the entire
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| /dports/astro/py-astlib/astLib-0.11.7/ |
| H A D | README.rst | 9 …, magnitudes from stellar population models or spectral templates, fit photometric observations us…
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| /dports/astro/py-astlib/astLib-0.11.7/docs/_build/json/ |
| H A D | usage.fjson | 2 …, magnitudes from stellar population models or spectral templates, fit photometric observations us…
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| /dports/astro/py-astropy/astropy-5.0/ |
| H A D | CHANGES.rst | 3388 favour of ``astropy.units.photometric`` since 3.1. [#9353]
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| /dports/astro/py-astropy/astropy-5.0/astropy/io/ascii/tests/data/cds/glob/ |
| H A D | ReadMe | 119 different from the photometric one
242 DQ or IP: photometric period if it is different from the
248 SH: photometric period, presumably superhump period of either
250 NS: photometric period, period of either permanent or transient
318 photometric period, presumably superhump
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| /dports/astro/py-astropy/astropy-5.0/astropy/units/ |
| H A D | __init__.py | 22 from . import photometric
28 from .photometric import *
47 set_enabled_units([si, cgs, astrophys, function_units, misc, photometric])
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| /dports/astro/py-astropy/astropy-5.0/astropy/units/function/ |
| H A D | logarithmic.py | 5 from astropy.units import (dimensionless_unscaled, photometric, Unit,
363 STmag = MagUnit(photometric.STflux)
366 ABmag = MagUnit(photometric.ABflux)
369 M_bol = MagUnit(photometric.Bol)
371 "L_bol0={}".format(photometric.Bol.si))
373 m_bol = MagUnit(photometric.bol)
375 "f_bol0={}".format(photometric.bol.si))
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| /dports/astro/py-astropy/astropy-5.0/astropy/wcs/tests/data/ |
| H A D | invalid_header.hdr | 1 … 1 / SCAMP photometric instrument label PHOTLINK= ' F' /…
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| H A D | siponly.hdr | 1 …ted? PHTCALFL= 0 / Flag for image is photometric (0=N, 1=Y) …
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| H A D | too_many_pv.hdr | 1 …ted? PHTCALFL= 0 / Flag for image is photometric (0=N, 1=Y) …
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| H A D | tpvonly.hdr | 1 …ted? PHTCALFL= 0 / Flag for image is photometric (0=N, 1=Y) …
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