LSST Applications g07dc498a13+7851b72aa9,g1409bbee79+7851b72aa9,g1a7e361dbc+7851b72aa9,g1fd858c14a+a4e18a0dda,g33399d78f5+a0324bbf49,g35bb328faa+e55fef2c71,g3bd4b5ce2c+8524b1c0c8,g53246c7159+e55fef2c71,g579b87e3d2+a58ba40925,g60b5630c4e+7b4465799a,g78460c75b0+8427c4cc8f,g78619a8342+5517f7db9e,g786e29fd12+307f82e6af,g8534526c7b+8e1c6b434f,g89139ef638+7851b72aa9,g8b49a6ea8e+7b4465799a,g8ffcb69f3d+0065d7bbc8,g9125e01d80+e55fef2c71,g97b8272a79+a8c4cb337e,g989de1cb63+7851b72aa9,g9f33ca652e+747bd1f1f9,gaaedd4e678+7851b72aa9,gabe3b4be73+9c0c3c7524,gb1101e3267+c03a154bbb,gb58c049af0+28045f66fd,gc1fe0db326+7b4465799a,gca43fec769+e55fef2c71,gce7788e931+99adca4f64,gcf25f946ba+a0324bbf49,gd397e13551+18f805d5e0,gd6cbbdb0b4+f6e5445f66,gde0f65d7ad+78b6ec8427,ge278dab8ac+b4c2c8faf7,geab183fbe5+7b4465799a,gecb8035dfe+1f480bec5e,gf58bf46354+e55fef2c71,gf92a8ffd38+e7bc33f3ea,gfe7187db8c+38a2c5c626,w.2025.03
LSST Data Management Base Package
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Public Member Functions | |
__init__ (self, colFlux, colFluxErr=None, **kwargs) | |
columns (self) | |
name (self) | |
hypot (cls, a, b) | |
dn2flux (self, dn, fluxMag0) | |
dn2mag (self, dn, fluxMag0) | |
dn2fluxErr (self, dn, dnErr, fluxMag0, fluxMag0Err) | |
dn2MagErr (self, dn, dnErr, fluxMag0, fluxMag0Err) | |
Public Attributes | |
vhypot | |
col | |
colFluxErr | |
fluxMag0 | |
fluxMag0Err | |
Static Public Attributes | |
tuple | AB_FLUX_SCALE = (0 * u.ABmag).to_value(u.nJy) |
float | LOG_AB_FLUX_SCALE = 12.56 |
float | FIVE_OVER_2LOG10 = 1.085736204758129569 |
int | COADD_ZP = 27 |
Base class for Object table calibrated fluxes and magnitudes.
Definition at line 1562 of file functors.py.
lsst.pipe.tasks.functors.Photometry.__init__ | ( | self, | |
colFlux, | |||
colFluxErr = None, | |||
** | kwargs ) |
Reimplemented from lsst.pipe.tasks.functors.Functor.
Definition at line 1571 of file functors.py.
lsst.pipe.tasks.functors.Photometry.columns | ( | self | ) |
Columns required to perform calculation.
Reimplemented from lsst.pipe.tasks.functors.Functor.
Reimplemented in lsst.pipe.tasks.functors.NanoJanskyErr.
Definition at line 1582 of file functors.py.
lsst.pipe.tasks.functors.Photometry.dn2flux | ( | self, | |
dn, | |||
fluxMag0 ) |
Convert instrumental flux to nanojanskys.
Definition at line 1599 of file functors.py.
lsst.pipe.tasks.functors.Photometry.dn2fluxErr | ( | self, | |
dn, | |||
dnErr, | |||
fluxMag0, | |||
fluxMag0Err ) |
Convert instrumental flux error to nanojanskys.
Definition at line 1610 of file functors.py.
lsst.pipe.tasks.functors.Photometry.dn2mag | ( | self, | |
dn, | |||
fluxMag0 ) |
Convert instrumental flux to AB magnitude.
Definition at line 1603 of file functors.py.
lsst.pipe.tasks.functors.Photometry.dn2MagErr | ( | self, | |
dn, | |||
dnErr, | |||
fluxMag0, | |||
fluxMag0Err ) |
Convert instrumental flux error to AB magnitude error.
Definition at line 1616 of file functors.py.
lsst.pipe.tasks.functors.Photometry.hypot | ( | cls, | |
a, | |||
b ) |
Compute sqrt(a^2 + b^2) without under/overflow.
Definition at line 1590 of file functors.py.
lsst.pipe.tasks.functors.Photometry.name | ( | self | ) |
Reimplemented from lsst.pipe.tasks.functors.Functor.
Definition at line 1586 of file functors.py.
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static |
Definition at line 1565 of file functors.py.
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static |
Definition at line 1569 of file functors.py.
lsst.pipe.tasks.functors.Photometry.col |
Definition at line 1573 of file functors.py.
lsst.pipe.tasks.functors.Photometry.colFluxErr |
Definition at line 1574 of file functors.py.
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static |
Definition at line 1567 of file functors.py.
lsst.pipe.tasks.functors.Photometry.fluxMag0 |
Definition at line 1576 of file functors.py.
lsst.pipe.tasks.functors.Photometry.fluxMag0Err |
Definition at line 1577 of file functors.py.
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static |
Definition at line 1566 of file functors.py.
lsst.pipe.tasks.functors.Photometry.vhypot |
Definition at line 1572 of file functors.py.