SIMBADEntry

class SIMBADEntry

Bases: dict

Attributes

Note: attributes inherited from parent classes are not shown here, if any

Name	Starname
Simbad_name	Starname in simbad query
Sp_type	Stellar spectral type
Ra	Right ascension coordinate
Dec	Declination coordinate
Pma	Proper motion ascension
Pmd	Proper motion declination
RV_sys	Systemic RV in km/s
Mstar	Stellar mass in solar mass
Rstar	Stellar radius in solar radius
Umag	U band magnitude
Bmag	B band magnitude
Vmag	V band magnitude
Rmag	R band magnitude
UB	UB color index
BV	BV color index
VR	VR color index
Dist_pc	Stellar distance in parsec
Teff	Stellar effective temperature in Kelvin
Log_g	Stellar surface gravity in cgs
FeH	Stellar metallicity
Vsini	Stellar vsini in km/s
Vmicro	Stellar microturbulence+macro in km/s
Prot	Stellar rotationnal period
Pmag	Stellar vsini in km/s
FWHM	FWHM of the CCF in km/s
Contrast	Contrast of the CCF in km/s
CCF_delta	Width of the CCF comb in wavelength index
stellar_template	Name of the stellar template in the ATLAS database

Methods

clear
copy
fromkeys	Create a new dictionary with keys from iterable and values set to value.
get	Return the value for key if key is in the dictionary, else default.
items
keys
pop	If key is not found, d is returned if given, otherwise KeyError is raised
popitem	Remove and return a (key, value) pair as a 2-tuple.
setdefault	Insert key with a value of default if key is not in the dictionary.
update	If E is present and has a .keys() method, then does: for k in E: D[k] = E[k] If E is present and lacks a .keys() method, then does: for k, v in E: D[k] = v In either case, this is followed by: for k in F: D[k] = F[k]
values

List of members of SIMBADEntry

Name: str

Starname

Simbad_name: FixedString

Starname in simbad query

Sp_type: FixedString

Stellar spectral type

Ra: FixedString

Right ascension coordinate

Dec: FixedString

Declination coordinate

Pma: FixedFloat

Proper motion ascension

Pmd: FixedFloat

Proper motion declination

RV_sys: FixedFloat

Systemic RV in km/s

Mstar: FixedFloat

Stellar mass in solar mass

Rstar: FixedFloat

Stellar radius in solar radius

Umag: FixedFloat

U band magnitude

Bmag: FixedFloat

B band magnitude

Vmag: FixedFloat

V band magnitude

Rmag: FixedFloat

R band magnitude

UB: FixedFloat

UB color index

BV: FixedFloat

BV color index

VR: FixedFloat

VR color index

Dist_pc: FixedFloat

Stellar distance in parsec

Teff: FixedInt

Stellar effective temperature in Kelvin

Log_g: FixedFloat

Stellar surface gravity in cgs

FeH: FixedFloat

Stellar metallicity

Vsini: FixedFloat

Stellar vsini in km/s

Vmicro: FixedFloat

Stellar microturbulence+macro in km/s

Prot: FixedInt

Stellar rotationnal period

Pmag: FixedInt

Stellar vsini in km/s

FWHM: FixedFloat

FWHM of the CCF in km/s

Contrast: FixedFloat

Contrast of the CCF in km/s

CCF_delta: FixedInt

Width of the CCF comb in wavelength index

stellar_template: FixedString

Name of the stellar template in the ATLAS database

__init__(*args, **kwargs)

static __new__(cls, _typename, _fields=None, /, **kwargs)

clear() → None.  Remove all items from D.

copy() → a shallow copy of D

fromkeys(value=None, /)

Create a new dictionary with keys from iterable and values set to value.

get(key, default=None, /)

Return the value for key if key is in the dictionary, else default.

items() → a set-like object providing a view on D's items

keys() → a set-like object providing a view on D's keys

pop(k[, d]) → v, remove specified key and return the corresponding value.

If key is not found, d is returned if given, otherwise KeyError is raised

popitem()

Remove and return a (key, value) pair as a 2-tuple.

Pairs are returned in LIFO (last-in, first-out) order. Raises KeyError if the dict is empty.

setdefault(key, default=None, /)

Insert key with a value of default if key is not in the dictionary.

Return the value for key if key is in the dictionary, else default.

update([E, ]**F) → None.  Update D from dict/iterable E and F.

If E is present and has a .keys() method, then does: for k in E: D[k] = E[k] If E is present and lacks a .keys() method, then does: for k, v in E: D[k] = v In either case, this is followed by: for k in F: D[k] = F[k]

values() → an object providing a view on D's values