20140919

重置插图计数器的时候

setcounter{figure}{1}

要放在chapter{}

后面，要不然会被重置为0。喵了个咪的！

20140809

ALFALFA的等效积分时间是40秒。

20140806

脉冲星星表

http://www.atnf.csiro.au/research/pulsar/psrcat/

20140725

cadcUrlList.txt

下载CGPS数据

wget --content-disposition -i cadcUrlList.txt

20140712

splatalogue的不同分子（能带）是用sid[]=xx来区分的，不同的xx代表不同的分子（能带）。

CI是125

CO（v=0）是204

C$^{17}$O是226

20140628
GBT谱线搜寻
http://www.cv.nrao.edu/~aremijan/PRIMOS/abstract.html

20140213

and $^{13}$CO center velocities is strong (Li & Goldsmith 2003). Hence, the vH parameter is held fixed for each velocity component. The TF estimates obtained from $^{12}$CO do not carry as much confidence (as discussed in the next section); however, the temperature is still kept as a fixed parameter during our fit. For optically thin spectral lines such as HINSA the temperature cannot sufficiently constrain the shape of the absorption feature to be allowed as a free parameter since a wide range of combinations of temperatures and optical depths would be able to fit the data. Thus the gas temperature must be specified in any fits.