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← Revision 50 as of 2012-11-27 14:05:33 ⇥
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Last updated: 23 Nov 2012 last scan 153 | Last updated: 27 Nov 2012. |
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*Source Legend:* | = Summary = 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 (details given below). 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. One must say that some (between 1/3 and 1/2) of the 64 hours were taken in sub-optimal conditions. |
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CRS = Compact Radio Source | '''Source Legend:''' WGS = Weak Galactic Source |
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WGS = Weak Galactic Source |
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CRS = Compact Radio Source |
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DS = Deep survey | |
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*Typical observation times for standard procedures:* | GRB = Gamma Ray Burst '''Typical observation times for standard procedures:''' |
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||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 || || |
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||WGS || FTtau || OTF_FAINT || 0.27 || || ||WGS || DRtau || OTF_FAINT || 0.27 || || |
||SGS|| MWC349 || OTF_FAINT || 0.66 || 1mm Array observing with 8pixels || |
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||SGS|| M87 || OTF FAINT || 0.53 || || ||SGS|| LKH234 || OTF FAINT || 0.33 || || ||SGS|| CRL2688 || OTF FAINT || 0.67 || || |
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||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 || || |
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||CRS || 0923+392 || OTF_SZ || 0.06 || || | |
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||GC || MACS0717 || OTF_SZ || 7.93 || || ||GC || RXJ1347-1145 || OTF_SZ || 9.06 || || ||CRS || CygA || OTF_DS || 0.8 || || |
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||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 || || |
Time of observation in hours. Last updated: 27 Nov 2012.
Summary
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 (details given below). 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. One must say that some (between 1/3 and 1/2) of the 64 hours were taken in sub-optimal conditions.
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 |
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