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Size: 932
Comment:
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Size: 2541
Comment:
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| Deletions are marked like this. | Additions are marked like this. |
| Line 3: | Line 3: |
| In principle, efficiencies due to the filtering method have been taken into account || '''Source''' || '''Date''' || '''Flux''' || '''Stat. Error''' || '''Comments''' || '''Map''' || '''Scan info'''|| || 3C273 || 20091025 || 13.1Jy || 0.1 || || || || || B1418+546 || 20091024 || 1.18Jy || 0.040 || Flux decreasing (known reasons) || || || || Arp220=IC4553 || 20091025 || 114mJy || 18mJy || || || || || GRB091024 || 20091024 || 6.6mJy || 4.8mJy || Heavy weight on first 2 scans || || || || M51 || 20091024 || 1.5mJy || 12mJy || PS flux at the center, no detection || || || || G34.3 || 20091024 || 4.761Jy || 0.024 || Peak flux, source is extended, || || || || K3_50A || 20091024 || 1.442Jy || 0.008 || Peak flux, source is extended || || || || PCyg || 20091024 || 28mJy || 4mJy || || || || || B1800+440 || 20091024 || 103mJy || 7mJy || || || || || 3C345 || 20091024 || 5.051Jy || 0.009 || || || 69-72 || || MWC349 || 20091024 || 1.364Jy || 0.010 || || || || || WR147 || 20091025 || 263mJy || 24 || Detected. || || 129-148 || || M87 || 20091027 || || || || || || || Pluto || 20091025 || 12mJy || 23 || Not detected || || 93-102 || |
|
| Line 5: | Line 22: |
| || '''Source''' || '''Date''' || '''Flux''' || '''Error''' || '''Comments''' || '''Map''' || || 3C273 || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || || || 20091025 || || || || || |
Arp220: Expect 43mJy (from 1 to 3 mm PdB interpolate), result a bit high, One article quote 88+-8 G34.3: Sandell gives 12.5 Jy in 27" photometry WR147: Expected is 200mJy Altenhoff, 1994 |
NIKA Run 1 offline processing results (FXD)
In principle, efficiencies due to the filtering method have been taken into account
Source |
Date |
Flux |
Stat. Error |
Comments |
Map |
Scan info |
3C273 |
20091025 |
13.1Jy |
0.1 |
|
|
|
B1418+546 |
20091024 |
1.18Jy |
0.040 |
Flux decreasing (known reasons) |
|
|
Arp220=IC4553 |
20091025 |
114mJy |
18mJy |
|
|
|
GRB091024 |
20091024 |
6.6mJy |
4.8mJy |
Heavy weight on first 2 scans |
|
|
M51 |
20091024 |
1.5mJy |
12mJy |
PS flux at the center, no detection |
|
|
G34.3 |
20091024 |
4.761Jy |
0.024 |
Peak flux, source is extended, |
|
|
K3_50A |
20091024 |
1.442Jy |
0.008 |
Peak flux, source is extended |
|
|
PCyg |
20091024 |
28mJy |
4mJy |
|
|
|
B1800+440 |
20091024 |
103mJy |
7mJy |
|
|
|
3C345 |
20091024 |
5.051Jy |
0.009 |
|
|
69-72 |
MWC349 |
20091024 |
1.364Jy |
0.010 |
|
|
|
WR147 |
20091025 |
263mJy |
24 |
Detected. |
|
129-148 |
M87 |
20091027 |
|
|
|
|
|
Pluto |
20091025 |
12mJy |
23 |
Not detected |
|
93-102 |
Arp220: Expect 43mJy (from 1 to 3 mm PdB interpolate), result a bit high, One article quote 88+-8
G34.3: Sandell gives 12.5 Jy in 27" photometry
WR147: Expected is 200mJy Altenhoff, 1994