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Python AbsLine.attrib['sig_N']方法代码示例

本文整理汇总了Python中linetools.spectralline.AbsLine.attrib['sig_N']方法的典型用法代码示例。如果您正苦于以下问题:Python AbsLine.attrib['sig_N']方法的具体用法?Python AbsLine.attrib['sig_N']怎么用?Python AbsLine.attrib['sig_N']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linetools.spectralline.AbsLine的用法示例。


在下文中一共展示了AbsLine.attrib['sig_N']方法的4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: lyman_comp

# 需要导入模块: from linetools.spectralline import AbsLine [as 别名]
# 或者: from linetools.spectralline.AbsLine import attrib['sig_N'] [as 别名]
def lyman_comp(radec, z=2.92939):
    # HI Lya, Lyb
    lya = AbsLine(1215.670*u.AA, z=z, linelist=ism)
    lya.limits.set([-300.,300.]*u.km/u.s)
    lya.attrib['flag_N'] = 1
    lya.attrib['N'] = 1e17 /  u.cm**2
    lya.attrib['sig_N'] = 1e16 /  u.cm**2
    lya.attrib['coord'] = radec
    # Lyb
    lyb = AbsLine(1025.7222*u.AA, z=z, linelist=ism)
    lyb.limits.set([-300.,300.]*u.km/u.s)
    lyb.attrib['coord'] = radec
    lyb.attrib['flag_N'] = 1
    lyb.attrib['N'] = 1e17 /  u.cm**2
    lyb.attrib['sig_N'] = 1e16 /  u.cm**2
    # Build
    abscomp = AbsComponent.from_abslines([lya,lyb])
    #abscomp.synthesize_colm()

    return abscomp
开发者ID:linetools,项目名称:linetools,代码行数:22,代码来源:utils.py

示例2: add_abslines_from_linelist

# 需要导入模块: from linetools.spectralline import AbsLine [as 别名]
# 或者: from linetools.spectralline.AbsLine import attrib['sig_N'] [as 别名]
    def add_abslines_from_linelist(self, llist='ISM', wvlim=None, min_Wr=None, **kwargs):
        """
        It adds associated AbsLines satisfying some conditions (see parameters below).

        Parameters
        ----------
        llist : str
            Name of the linetools.lists.linelist.LineList
            object where to look for the transition names.
            Default is 'ISM', which means the function looks
            within `list = LineList('ISM')`.
        wvlims : Quantity array, optional
            Observed wavelength limits for AbsLines to be added.
            e.g. [1200, 2000]*u.AA.
        min_Wr : Quantity, optional
            Minimum rest-frame equivalent with for AbsLines to be added.
            This is calculated in the very low optical depth regime tau0<<1,
            where Wr is independent of Doppler parameter or gamma (see eq. 9.15 of
            Draine 2011). Still, a column density attribute for the AbsComponent
            is needed.

        Returns
        -------
        Adds AbsLine objects to the AbsComponent._abslines list.

        Notes
        -----
        **kwargs are passed to AbsLine.add_absline() method.

        """
        # get the transitions from LineList
        llist = LineList(llist)
        name = ions.ion_name(self.Zion, nspace=0)
        transitions = llist.all_transitions(name)
        # unify output to be always QTable
        if isinstance(transitions, dict):
            transitions = llist.from_dict_to_qtable(transitions)

        # check wvlims
        if wvlim is not None:
            cond = (transitions['wrest']*(1+self.zcomp) >= wvlim[0]) & \
                   (transitions['wrest']*(1+self.zcomp) <= wvlim[1])
            transitions = transitions[cond]

        # check outputs
        if len(transitions) == 0:
            warnings.warn("No transitions satisfying the criteria found. Doing nothing.")
            return

        # loop over the transitions when more than one found
        for transition in transitions:
            iline = AbsLine(transition['name'], z=self.zcomp)
            iline.limits.set(self.vlim)
            iline.attrib['coord'] = self.coord
            iline.attrib['logN'] = self.logN
            iline.attrib['sig_logN'] = self.sig_logN
            iline.attrib['flag_N'] = self.flag_N
            iline.attrib['N'] = 10**iline.attrib['logN'] / (u.cm * u.cm)
            iline.attrib['sig_N'] = 10**iline.attrib['sig_logN'] / (u.cm * u.cm)

            for key in self.attrib.keys():
                iline.attrib[key] = self.attrib[key]

            if min_Wr is not None:
                # check logN is defined
                logN = self.logN
                if logN == 0:
                    warnings.warn("AbsComponent does not have logN defined. Appending AbsLines "
                                 "regardless of min_Wr.")
                else:
                    N = 10**logN / (u.cm*u.cm)
                    Wr_iline = iline.get_Wr_from_N(N=N)  # valid for the tau0<<1 regime.
                    if Wr_iline < min_Wr:  # do not append
                        continue
            # add the absline
            self.add_absline(iline)
开发者ID:jnburchett,项目名称:linetools,代码行数:78,代码来源:abscomponent.py

示例3: read_clmfile

# 需要导入模块: from linetools.spectralline import AbsLine [as 别名]
# 或者: from linetools.spectralline.AbsLine import attrib['sig_N'] [as 别名]
def read_clmfile(clm_file,linelist=None):
    """ Read in a .CLM file in an appropriate manner

    NOTE: If program breaks in this function, check the clm to see if it is properly formatted.


    RETURNS two dictionaries CLM and LINEDIC. CLM contains the contents of CLM
    for the given DLA. THe LINEDIC that is passed (when not None) is updated appropriately.

    Keys in the CLM dictionary are:
      INST - Instrument used
      FITS - a list of fits files
      ZABS - absorption redshift
      ION - .ION file location
      HI - THe HI column and error; [HI, HIerr]
      FIX - Any abundances that need fixing from the ION file
      VELS - Dictioanry of velocity limits, which is keyed by
        FLAGS - Any measurment flags assosicated with VLIM
        VLIM - velocity limits in km/s [vmin,vmax]
        ELEM - ELement (from get_elem)

    See get_elem for properties of LINEDIC

    Parameters
    ----------
    clm_file : str
      Full path to the .clm file
    linelist : LineList
      can speed up performance
    """
    clm_dict = {}
    # Read file
    f=open(clm_file, 'r')
    arr=f.readlines()
    f.close()
    nline = len(arr)
    # Data files
    clm_dict['flg_data'] = int(arr[1][:-1])
    clm_dict['fits_files']={}
    ii=2
    for jj in range(0,6):
        if (clm_dict['flg_data'] % (2**(jj+1))) > (2**jj - 1):
            clm_dict['fits_files'][2**jj] = arr[ii].strip()
            ii += 1

    # Redshift
    clm_dict['zsys']=float(arr[ii][:-1]) ; ii+=1
    clm_dict['ion_fil']=arr[ii].strip() ; ii+=1
    # NHI
    tmp = arr[ii].split(',') ; ii+=1
    if len(tmp) != 2:
        raise ValueError('ionic_clm: Bad formatting {:s} in {:s}'
                                       .format(arr[ii-1],clm_file))
    clm_dict['NHI']=float(tmp[0])
    clm_dict['sigNHI']=float(tmp[1])
    # Abundances by hand
    numhand=int(arr[ii][:-1]) ; ii+=1
    clm_dict['fixabund']={}
    if numhand>0:
        for jj in range(numhand):
            # Atomic number
            atom=int(arr[ii][:-1]) ; ii+=1
            # Values
            tmp = arr[ii].strip().split(',') ; ii+=1
            clm_dict['fixabund'][atom]= float(tmp[0]), float(tmp[1]), int(tmp[2])
    # Loop on lines
    clm_dict['lines'] = {}
    while ii < (nline-1):
        # No empty lines allowed
        if len(arr[ii].strip()) == 0:
           break
        # Read flag
        ionflg = int(arr[ii].strip()); ii+=1
        # Read the rest
        tmp = arr[ii].split(',') ; ii+=1
        if len(tmp) != 4: raise ValueError('ionic_clm: Bad formatting {:s} in {:s}'
                                        .format(arr[ii-1],clm_file))
        vmin = float(tmp[1].strip())
        vmax = float(tmp[2].strip())
        key = float(tmp[0].strip()) # Using a float not string!
        # Generate
        clm_dict['lines'][key] = AbsLine(key*u.AA,closest=True,linelist=linelist)
        clm_dict['lines'][key].attrib['z'] = clm_dict['zsys']
        clm_dict['lines'][key].analy['FLAGS'] = ionflg, int(tmp[3].strip())
        pdb.set_trace()
        # By-hand
        if ionflg >= 8:
            clm_dict['lines'][key].attrib['N'] = 10.**vmin / u.cm**2
            clm_dict['lines'][key].attrib['sig_N'] = (10.**(vmin+vmax) - 10.**(vmin-vmax))/2/u.cm**2
        else:
            clm_dict['lines'][key].analy['vlim']= [vmin,vmax]*u.km/u.s
    # Return
    return clm_dict
开发者ID:banados,项目名称:xastropy,代码行数:95,代码来源:ionclms.py

示例4: add_abslines_from_linelist

# 需要导入模块: from linetools.spectralline import AbsLine [as 别名]
# 或者: from linetools.spectralline.AbsLine import attrib['sig_N'] [as 别名]
    def add_abslines_from_linelist(self, llist='ISM', init_name=None, wvlim=None, min_Wr=None, **kwargs):
        """
        It adds associated AbsLines satisfying some conditions (see parameters below).

        Parameters
        ----------
        llist : str, optional
            Name of the linetools.lists.linelist.LineList
            object where to look for the transition names.
            Default is 'ISM', which means the function looks
            within `list = LineList('ISM')`.
        init_name : str, optional
            Name of the initial transition used to define the AbsComponent
        wvlim : Quantity array, optional
            Observed wavelength limits for AbsLines to be added.
            e.g. [1200, 2000]*u.AA.
        min_Wr : Quantity, optional
            Minimum rest-frame equivalent with for AbsLines to be added.
            This is calculated in the very low optical depth regime tau0<<1,
            where Wr is independent of Doppler parameter or gamma (see eq. 9.15 of
            Draine 2011). Still, a column density attribute for the AbsComponent
            is needed.

        Returns
        -------
        Adds AbsLine objects to the AbsComponent._abslines list.

        Notes
        -----
        **kwargs are passed to AbsLine.add_absline() method.

        """
        from linetools.lists import utils as ltlu

        # get the transitions from LineList
        llist = LineList(llist)
        if init_name is None:  # we have to guess it
            if (self.Zion) == (-1, -1):  # molecules
                # init_name must be in self.attrib (this is a patch)
                init_name = self.attrib['init_name']
            else:  # atoms
                init_name = ions.ion_to_name(self.Zion, nspace=0)
        transitions = llist.all_transitions(init_name)

        # unify output to be a Table
        if isinstance(transitions, dict):
            transitions = ltlu.from_dict_to_table(transitions)

        # check wvlims
        if wvlim is not None:
            # Deal with units
            wrest = transitions['wrest'].data * transitions['wrest'].unit
            # Logic
            cond = (wrest*(1+self.zcomp) >= wvlim[0]) & \
                   (wrest*(1+self.zcomp) <= wvlim[1])
            transitions = transitions[cond]

        # check outputs
        if len(transitions) == 0:
            warnings.warn("No transitions satisfying the criteria found. Doing nothing.")
            return

        # loop over the transitions when more than one found
        for transition in transitions:
            iline = AbsLine(transition['name'], z=self.zcomp, linelist=llist)
            iline.limits.set(self.vlim)
            iline.attrib['coord'] = self.coord
            iline.attrib['logN'] = self.logN
            iline.attrib['sig_logN'] = self.sig_logN
            iline.attrib['flag_N'] = self.flag_N
            iline.attrib['N'] = 10**iline.attrib['logN'] / (u.cm * u.cm)
            iline.attrib['sig_N'] = 10**iline.attrib['sig_logN'] / (u.cm * u.cm)

            for key in self.attrib.keys():
                iline.attrib[key] = self.attrib[key]

            if min_Wr is not None:
                # check logN is defined
                if self.logN == 0:
                    pass
                else:
                    N = 10.**self.logN / u.cm**2
                    Wr_iline = iline.get_Wr_from_N(N=N)  # valid for the tau0<<1 regime.
                    if Wr_iline < min_Wr:  # do not append
                        continue
            # add the absline
            self.add_absline(iline)
开发者ID:linetools,项目名称:linetools,代码行数:89,代码来源:abscomponent.py


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