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: http://xmm.vilspa.esa.es/sas/5.4.1/doc/esky2det/node4.html
Дата изменения: Fri Jan 10 22:40:40 2003 Дата индексирования: Sat Dec 22 09:04:46 2007 Кодировка: Поисковые слова: m 35 |
The sky position of a single source may be entered via the parameters ra, dec and (optionally) errorradius. These are parameters of type angle and can therefore be provided in a variety of formats. See the task param documentation for further details.
In this mode, the output positions are printed to a single line of standard output. The format of this output line is given in the following examples.
esky2det datastyle=user ra=03h47m40.2s dec=24d21m54.62s outunit=raw
gives the output
# Instrument: EPN # Coord sytem of output is RAWXY (PIXCOORD1). # Source RA = 56.917500 deg. # Source dec = 24.365171 deg. # # rawX rawY ccd 32 188 8
32 188 8
This style is suitable for batch running of esky2det from scripts.
esky2det datastyle=user ra=03h46m25.3s dec=24d18m30.3s outunit=det witherrors=yes errorradius=00d00m05.0s
which gives the output
# Instrument: EPN # Coord sytem of output is DETXY (CAMCOORD2 but in units of 0.05 arcsec). # Source RA = 56.605415 deg. # Source dec = 24.308416 deg. # # detX detY det err -15043.9 -2111.8 100.0
# Instrument: EPN # Coord sytem of output is RAWXY (PIXCOORD1). # Source RA = 56.605415 deg. # Source dec = 24.308416 deg. # # rawX rawY ccd X err Y err 40 189 12 1 1
No output is performed for sources which are outside the field of view or, in the case of RAWX/Y, not located on a ccd: an error message is generated instead.
You may be asking yourself "how is the pointing and instrument information obtained in these examples?" The answer this question is found in subsection 3.4.
XMM-Newton SOC/SSC -- 2003-01-10