Size: 2696
Comment:
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Size: 4053
Comment:
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Deletions are marked like this. | Additions are marked like this. |
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Last updated: 23 Nov 2012 last scan 153 | Last updated: 25 Nov 2012 last scan 248 |
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* Source Legend: | '''Source Legend:''' |
Line 6: | Line 6: |
CRS = Compact Radio Source | WGS = Weak Galactic Source |
Line 9: | Line 9: |
WGS = Weak Galactic Source |
|
Line 16: | Line 14: |
CRS = Compact Radio Source |
|
Line 18: | Line 18: |
DS = Deep survey | |
Line 19: | Line 20: |
* Typical observation times for standard procedures: | GRB = Gamma Ray Burst '''Typical observation times for standard procedures:''' |
Line 33: | Line 36: |
||TYPE || SOURCENAME || OBSERVATION TYPE || OBSERVATION TIME (hours) || COMMENTS || ||CRS || 3C84 || OTF2x2 || 0.1 || || ||WGS || IRC10420 || OTF_FAINT || 0.46 || || ||SGS|| MWC349 || OTF_FAINT || 0.66 || || ||WGS || WR147 || OTF_FAINT || 0.27 || || |
||'''TYPE''' || '''SOURCENAME''' || '''OBSERVATION TYPE''' || '''OBSERVATION TIME (hours)''' || '''COMMENTS''' || ||WGS || IRC10420 || OTF_FAINT || 0.46 || 1mm Array observing with 8pixels || ||WGS || WR147 || OTF_FAINT || 0.27 || 1mm Array observing with 8pixels || ||WGS || FTtau || OTF_FAINT || 0.27 || || ||WGS || DRtau || OTF_FAINT || 0.27 || || ||WGS || ZZTAU IRS || OTF_FAINT || 0.66 || || ||WGS || CXTAU || OTF_FAINT || 0.66 || || ||SGS|| HORSEHEAD || OTF_5X5 || 1.33 || || |
Line 40: | Line 46: |
||WGS || FTtau || OTF_FAINT || 0.27 || || ||WGS || DRtau || OTF_FAINT || 0.27 || || |
||SGS|| MWC349 || OTF_FAINT || 0.66 || 1mm Array observing with 8pixels || |
Line 47: | Line 52: |
||SGS|| M87 || OTF FAINT || 0.53 || || ||SGS|| LKH234 || OTF FAINT || 0.33 || || ||SGS|| CRL2688 || OTF FAINT || 0.67 || || |
|
Line 48: | Line 56: |
||EG || NGC1068 || OTF_FAINT || 0.13 || || ||CG || MACS0717 || OTF_SZ || 7.93 || || ||CG || RXJ1347-1145 || OTF_SZ || 9.06 || || ||CG || IDCSJ1426 || OTF_SZ || 11.53 || || ||CG || M2228 || OTF_SZ || 4.78 || || ||CRS || 3C84 || OTF2x2 || 0.1 || || ||CRS || CygA || OTF_DS || 0.8 || || ||CRS || 0923+392 || OTF_SZ || 0.06 || || |
|
Line 49: | Line 65: |
||CRS || 0923+392 || OTF_SZ || 0.06 || || | |
Line 55: | Line 70: |
||GC || MACS0717 || OTF_SZ || 7.93 || || ||GC || RXJ1347-1145 || OTF_SZ || 9.06 || || ||CRS || CygA || OTF_DS || 0.8 || || |
|
Line 59: | Line 71: |
||HZS || PSS2322 || OTF_FAINT || 1 || || ||HZS || MM18423 || OTF_FAINT || 1.4 || || ||HZS || ARP220 || OTF_FAINT || 0.87 || || ||GC || SXDF || OTF_DS || 1.03 || || ||WGS || ZZTAU IRS || OTF_FAINT || 0.66 || || ||WGS || CXTAU || OTF_FAINT || 0.66 || || ||SGS|| HORSEHEAD || OTF_5X5 || 1.33 || || ||GC || IDCSJ1426 || OTF_SZ || 2.33 || || |
||HZS || PSS2322 || OTF_FAINT || 1 || || ||HZS || MM18423 || OTF_FAINT || 1.4 || for 1mm 13scans with 8pixels and 9scans with 91 pixels || ||HZS || HAT08933 || OTF_FAINT || 1 || || ||HZS || HAT133008 || OTF_FAINT || 0.93 || || ||HZS || HAT13349 || OTF_FAINT || 0.87 || || ||DS || SXDF || OTF_DS || 4.13 || || ||GRB || GRB12113A || OTF_FAIT || 1.13 || || Overall the run 5 was highly successful. 33.5 hours were spent on SZ studies, 17 hours on faint high-z point sources, 2.5 hours on extended external galaxies and 11 hours on galactic sources. The first week was used to characterize the instrument with 42 (6x7) hours of telescope. The second week allowed 122 hours of telescope time out of which 64 hours on scientific targets. Not many hours were lost due to technical reasons (estimated at 3h). The rest is split between numerous calibration procedures (pointing, focusing, geometry measuring, skydips) and bad weather. |
Time of observation in hours. Last updated: 25 Nov 2012 last scan 248
Source Legend:
WGS = Weak Galactic Source
SGS = Strong Galactic Source
EG = Extended Galaxy
CG = Cluster of Galaxies
CRS = Compact Radio Source
HZS = High Redshift Source
DS = Deep survey
GRB = Gamma Ray Burst
Typical observation times for standard procedures:
OTF_faint : 4 min
OTF_10x10 : 19 min
OTF_5x5 : 10 min
OTF_SZ : 7 min
OTF_DF : 6 min
TYPE |
SOURCENAME |
OBSERVATION TYPE |
OBSERVATION TIME (hours) |
COMMENTS |
WGS |
IRC10420 |
OTF_FAINT |
0.46 |
1mm Array observing with 8pixels |
WGS |
WR147 |
OTF_FAINT |
0.27 |
1mm Array observing with 8pixels |
WGS |
FTtau |
OTF_FAINT |
0.27 |
|
WGS |
DRtau |
OTF_FAINT |
0.27 |
|
WGS |
ZZTAU IRS |
OTF_FAINT |
0.66 |
|
WGS |
CXTAU |
OTF_FAINT |
0.66 |
|
SGS |
HORSEHEAD |
OTF_5X5 |
1.33 |
|
SGS |
K3-50A |
OTF_FAINT |
0.13 |
|
SGS |
LKH234 |
OTF_FAINT |
0.13 |
|
SGS |
MWC349 |
OTF_FAINT |
0.66 |
1mm Array observing with 8pixels |
SGS |
Crab |
OTF10x10 |
0.63 |
|
SGS |
DR21_OH |
OTF10x10 |
0.63 |
|
SGS |
OrionLBS23SM |
OTF10x10 |
1.26 |
|
SGS |
CAS A |
OTF 10x10 |
0.63 |
|
SGS |
NGC2023 |
OTF 10x10 |
1.23 |
|
SGS |
M87 |
OTF FAINT |
0.53 |
|
SGS |
LKH234 |
OTF FAINT |
0.33 |
|
SGS |
CRL2688 |
OTF FAINT |
0.67 |
|
EG |
M82 |
OTF10x10 |
1.26 |
|
EG |
NGC1068 |
OTF_FAINT |
0.13 |
|
CG |
MACS0717 |
OTF_SZ |
7.93 |
|
CG |
RXJ1347-1145 |
OTF_SZ |
9.06 |
|
CG |
IDCSJ1426 |
OTF_SZ |
11.53 |
|
CG |
M2228 |
OTF_SZ |
4.78 |
|
CRS |
3C84 |
OTF2x2 |
0.1 |
|
CRS |
CygA |
OTF_DS |
0.8 |
|
CRS |
0923+392 |
OTF_SZ |
0.06 |
|
HZS |
OJ287 |
OTF_FAINT |
0.06 |
|
HZS |
APM08279 |
OTF_FAINT |
0.80 |
|
HZS |
HLS091828 |
OTF_FAINT |
1.96 |
|
HZS |
4C05.19 |
OTF_FAINT |
0.53 |
|
HZS |
MM18423 |
OTF_FAINT |
0.93 |
|
HZS |
SMMJ2135 |
OTF_FAINT |
1.86 |
|
HZS |
ARP220 |
OTF_FAINT |
0.87 |
|
HZS |
PSS2322 |
OTF_FAINT |
1 |
|
HZS |
MM18423 |
OTF_FAINT |
1.4 |
for 1mm 13scans with 8pixels and 9scans with 91 pixels |
HZS |
HAT08933 |
OTF_FAINT |
1 |
|
HZS |
HAT133008 |
OTF_FAINT |
0.93 |
|
HZS |
HAT13349 |
OTF_FAINT |
0.87 |
|
DS |
SXDF |
OTF_DS |
4.13 |
|
GRB |
GRB12113A |
OTF_FAIT |
1.13 |
|
Overall the run 5 was highly successful. 33.5 hours were spent on SZ studies, 17 hours on faint high-z point sources, 2.5 hours on extended external galaxies and 11 hours on galactic sources. The first week was used to characterize the instrument with 42 (6x7) hours of telescope. The second week allowed 122 hours of telescope time out of which 64 hours on scientific targets. Not many hours were lost due to technical reasons (estimated at 3h). The rest is split between numerous calibration procedures (pointing, focusing, geometry measuring, skydips) and bad weather.