1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
|
.help skysub Mar94 noao.imred.specred
.ih
NAME
skysub -- Sky subtract extracted multispec spectra
.ih
USAGE
skysub input
.ih
PARAMETERS
.ls input
List of input multispec spectra to sky subtract.
.le
.ls output = ""
List of output sky subtracted spectra. If no output is specified then
the output replaces the input spectra.
.le
.ls objaps = "", objbeams = ""
Object aperture and beam numbers. An empty list selects all aperture
or beam numbers. Only the selected apertures are sky subtracted.
Other apertures are left unmodified. Note that it is valid to include
the sky apertures in the object selection which results in residual
sky spectra after subtraction by a mean sky.
.le
.ls skyaps = "", skybeams = ""
Sky aperture and beam numbers. An empty list selects all aperture or
beam numbers.
.le
.ls skyedit = yes
Edit the sky spectra? If yes the sky spectra are graphed using the
task \fBspecplot\fR and the user may delete contaminated sky spectra with
the 'd' key and exit with 'q'.
.le
.ls combine = "average" (average|median|sum)
Option for combining pixels at the same dispersion coordinate after any
rejection operation. The options are to compute the "average", "median",
or "sum" of the pixels. The median uses the average of the two central
values when the number of pixels is even.
.le
.ls reject = "none" (none|minmax|avsigclip)
Type of rejection operation performed on the pixels which overlap at each
dispersion coordinate. The algorithms are discussed in the
DESCRIPTION section. The rejection choices are:
.nf
none - No rejection
minmax - Reject the nlow and nhigh pixels
avsigclip - Reject pixels using an averaged sigma clipping algorithm
.fi
.le
.ls scale = no
Scale the sky spectra by the mode?
.le
.ls saveskys = yes
Save the sky spectra? If no then the mean sky spectra will be deleted after
sky subtraction is completed. Otherwise a one dimensional image with
the prefix "sky" and then the output name is created.
.le
.ls logfile = ""
Logfile for making a record of the sky subtraction operation.
.le
.ih
DESCRIPTION
This task selects a subset of aperture spectra from a multispec
format image, called sky spectra though they could be anything,
and combines them into a master spectrum which is subtracted
from another subset of spectra called the objects. Options include
saving the master sky spectrum and reviewing the selected sky spectra
graphically and deleting some of them.
The sky apertures are selected using the aperture and beam numbers
defined during extraction (see the \fBapextract\fR package). In
some applications the beam numbers are used to code object and sky
apertures and selection by beam number is quite easy. Otherwise one
must list the aperture numbers explicitly.
The object apertures are also selected using an aperture and beam
number list. Spectra not selected to be objects are not modified
by the sky subtraction. Note that it is perfectly valid to include
the sky spectra in the object list to produce residual sky spectra.
When interactively editing the sky spectra the task \fBspecplot\fR
is used. To delete a spectrum type 'd'. To undelete the last deleted
spectrum type 'e'. When finished type 'e'.
The sky spectra are combined using one of combining and rejection options from
the task \fBscombine\fR except for the option "none".
.ih
EXAMPLES
1. To median and subtract apertures 1,10,15,20 from all apertures:
.nf
ms> skysub obj010.ms out=skysub010.ms skyaps="1,10,15,20"
.fi
.ih
SEE ALSO
specplot, scombine
.endhelp
|
