本文整理汇总了Python中astroquery.vizier.Vizier.find_catalogs方法的典型用法代码示例。如果您正苦于以下问题：Python Vizier.find_catalogs方法的具体用法？Python Vizier.find_catalogs怎么用？Python Vizier.find_catalogs使用的例子？那么恭喜您, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类astroquery.vizier.Vizier的用法示例。
在下文中一共展示了Vizier.find_catalogs方法的5个代码示例，这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞，您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: search_catalog
# 需要导入模块: from astroquery.vizier import Vizier [as 别名]
# 或者: from astroquery.vizier.Vizier import find_catalogs [as 别名]
def search_catalog(self, term, obsolete):
json_result = '{"catalogs":[]}'
try:
catalog_list = Vizier.find_catalogs(term, include_obsolete=obsolete)
if catalog_list:
catalogs = CatalogCollection(catalog_list)
json_result = dumper(catalogs)
self.logger.info("Result from Vizier catalog search for '{0}' \n {1}".format(term, json_result))
else:
self.logger.info("Nothing found for '{0}'".format(term))
except:
self.logger.error("Error in SimbadProvider", exc_info=True)
raise ProviderException("error", "something")
return json_result示例2: get_usnob1_cat
# 需要导入模块: from astroquery.vizier import Vizier [as 别名]
# 或者: from astroquery.vizier.Vizier import find_catalogs [as 别名]
import numpy as np
from astroquery.vizier import Vizier
from astropy.coordinates import SkyCoord
import astropy.units as u
from astropy import table
import numpy as np
usnob_cat = Vizier.find_catalogs('USNO-B1.0')
def get_usnob1_cat(ra, dec, blim):
ra_u = ra*u.degree
dec_u = dec*u.degree
coords = SkyCoord(ra_u, dec_u, frame='icrs') #Should this be ICRS or FK5
#Only Class 0 (stars) - unable to implement this at the current time. Need to understand
#USNO-B1 s/g classification
v = Vizier(columns=['USNO-B1.0', '_RAJ2000', '_DEJ2000',
'B1mag', 'R1mag', 'B2mag', 'R2mag',
'pmRA', 'pmDE', 'Imag', 'B1s/g', '_r'],
row_limit=500000,
column_filters={"B2mag":">6", 'B2mag':'<{}'.format(blim)}) #B2mag fainter than 6, brighter than blim
new_table_list = v.query_region(coords,
radius=900*u.arcsecond, #Search 900 arcseconds
catalog = 'I/284')
if len(new_table_list) ==0:
return None
else:
new_table = new_table_list[0]
#Get the 5000 closest
new_table.sort('_r')
if len(new_table) > 5000:
new_table.remove_rows(np.arange(5001, len(new_table)))示例3: len
# 需要导入模块: from astroquery.vizier import Vizier [as 别名]
# 或者: from astroquery.vizier.Vizier import find_catalogs [as 别名]
from astroquery.vizier import Vizier
catalog_list = Vizier.find_catalogs('J/ApJS/204/5')
Vizier.ROW_LIMIT = -1
cata = Vizier.get_catalogs(catalog_list.keys())[0]
print len(cata)示例4: Vizier
# 需要导入模块: from astroquery.vizier import Vizier [as 别名]
# 或者: from astroquery.vizier.Vizier import find_catalogs [as 别名]
# the luminosity is just not right...
# (this is not included in the paper because I'm worried about a factor of
# at least 4 pi being left out...)
sfr2cm = ((cont2cm*u.K).to(u.Jy, u.brightness_temperature(gbbeamarea,
h2co22freq)) *
#gb_ppbeam / gb_pixelsize_deg**2 * u.sr *
#(4*np.pi*distance**2) *
distance**2 * # there is a 4 pi missing here... but it may come from elsewhere
sfrperergshz).to(u.M_sun/u.yr)
sfr2cmd = (sfr2cm / pixel_area).to(u.M_sun/u.yr/u.kpc**2)
ok2cm = cont2cm > 0.1
from astroquery.vizier import Vizier
catalog_list = Vizier.find_catalogs('Kang W51')
ysos = Vizier(row_limit=1e6).query_region(coordinates.SkyCoord.from_name('W51'),
radius=1*u.deg,
catalog=catalog_list.keys())
cl1lt10 = ((ysos[0]['Cl1'] == 'I') |
(ysos[0]['Cl1'] == 'F') |
(ysos[0]['Cl2'] == 'I') |
(ysos[0]['Cl2'] == 'F')) & (ysos[0]['Mstar'] < 10)
cl1gt10 = ((ysos[0]['Cl1'] == 'I') |
(ysos[0]['Cl1'] == 'F') |
(ysos[0]['Cl2'] == 'I') |
(ysos[0]['Cl2'] == 'F')) & (ysos[0]['Mstar'] >= 10)
cl1lt10coords = coordinates.SkyCoord(ysos[0][cl1lt10]['_RAJ2000'],
ysos[0][cl1lt10]['_DEJ2000'],
frame='fk5').galactic
cl1gt10coords = coordinates.SkyCoord(ysos[0][cl1gt10]['_RAJ2000'],示例5:
# 需要导入模块: from astroquery.vizier import Vizier [as 别名]
# 或者: from astroquery.vizier.Vizier import find_catalogs [as 别名]
import matplotlib.pyplot as plt
import matplotlib.lines as mlines
from matplotlib.patches import Circle
import mpl_toolkits.mplot3d.art3d as art3d
from astroquery.vizier import Vizier
from spaceutils import show_maximized_plot, kiloparsec_to_lightyear
# =====================================================================================================
catalog_list = Vizier.find_catalogs('VII/202')
Vizier.ROW_LIMIT = 1000000
catalogs = Vizier.get_catalogs(catalog_list.keys())
data = catalogs[0]
# =====================================================================================================
data.sort('Name')
data["X"] = kiloparsec_to_lightyear(data["X"])
data["Y"] = kiloparsec_to_lightyear(data["Y"])
data["Z"] = kiloparsec_to_lightyear(data["Z"])
data["Rsun"] = kiloparsec_to_lightyear(data["Rsun"])
SUN_TO_CENTER_DISTANCE = 27200
MILKY_WAY_RADIUS = 110000 / 2