CLIMB Observing Run 2011Jun-Jul-Aug: Difference between revisions

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Possible observing sequences (spend 2-3 nights on each configuration):'''<br>
Possible observing sequences (spend 2-3 nights on each configuration):'''<br>
<br>
<br>
=== Configuration E1-W1-W2, POP215, provides also long baselines and covers wider range of PA:
=== Configuration E1-W1-W2, POP215, provides also long baselines and covers wider range of PA:<br>
HD142666    21.0-21.8            (or AS205A  21.0-22.1, V=12.0, with very good conditions!)
HD142666    21.0-21.8            (or AS205A  21.0-22.1, V=12.0, with very good conditions!)<br>
      (or HD141569 21.0-22.2, V=7.0)
      (or HD141569 21.0-22.2, V=7.0)<br>
HD150193    21.2-22.5 (=MWC863)
HD150193    21.2-22.5 (=MWC863)<br>
HD163296    22.2-23.8
HD163296    22.2-23.8<br>
HD179218    23.5- 1.9 (=MWC614)
HD179218    23.5- 1.9 (=MWC614)<br>
HD190073      0.3- 2.7 (=V1295Aql)
HD190073      0.3- 2.7 (=V1295Aql)<br>
MWC340       0.6- 3.7           (or HD344361 23.8- 2.3, V=10.5, with good conditions =WW Vul)
MWC340       0.6- 3.7           (or HD344361 23.8- 2.3, V=10.5, with good conditions =WW Vul)<br>
HD200775    22.4- 5.2 (=MWC361)  (or MWC1080  2.4- 5.2, V=11.6, with good conditions)
HD200775    22.4- 5.2 (=MWC361)  (or MWC1080  2.4- 5.2, V=11.6, with good conditions)<br>
            (or LkHa234  23.8- 5.2, V=11.9, with good conditions)
            (or LkHa234  23.8- 5.2, V=11.9, with good conditions)<br>
<br>
<br>
=== Configuration E1-E2-W2, POP235, provides quite good radial sampling of visibility function towards similar PA with intermediate baseline lengths:
=== Configuration E1-E2-W2, POP235, provides quite good radial sampling of visibility function towards similar PA with intermediate baseline lengths:<br>
HD142666    21.0-21.8   (or AS205A  21.0-22.1, V=12.0, with very good conditions!)
HD142666    21.0-21.8   (or AS205A  21.0-22.1, V=12.0, with very good conditions!)<br>
      (or HD141569 21.0-22.2, V=7.0)
      (or HD141569 21.0-22.2, V=7.0)<br>
HD163296    22.2-23.8   (or HD150193 21.2-22.5, V=8.9, =MWC863)
HD163296    22.2-23.8   (or HD150193 21.2-22.5, V=8.9, =MWC863)<br>
HD179218    22.5- 2.1 (=MWC614)  (or HD190073 23.1- 2.7, V=7.2, =V1295Aql)
HD179218    22.5- 2.1 (=MWC614)  (or HD190073 23.1- 2.7, V=7.2, =V1295Aql)<br>
MWC340     23.8- 4.5
MWC340     23.8- 4.5<br>
HD200775    22.4- 5.2  (=MWC361)
HD200775    22.4- 5.2  (=MWC361)<br>
<br>
<br>
=== Configuration E2-W1-W2, POP 315,
=== Configuration E2-W1-W2, POP 315<br>
HD142666    21.0-22.7             
HD142666    21.0-22.7            <br>
HD141569    21.0-22.9            (or AS205A    21.0-23.0, V=12.0, with very good conditions)
HD141569    21.0-22.9            (or AS205A    21.0-23.0, V=12.0, with very good conditions)<br>
HD150193    21.2-23.5  (=MWC863)
HD150193    21.2-23.5  (=MWC863)<br>
HD163296    22.2- 0.7
HD163296    22.2- 0.7<br>
HD179218    23.5- 2.5  (=MWC614)
HD179218    23.5- 2.5  (=MWC614)<br>
MWC340        0.3- 4.2
MWC340        0.3- 4.2<br>
HD200775    22.2- 5.2  (=MWC361) (or MWC1080    1.0- 5.2, V=11.6, with good conditions)
HD200775    22.2- 5.2  (=MWC361) (or MWC1080    1.0- 5.2, V=11.6, with good conditions)<br>
<br>
<br>


Revision as of 18:49, 7 June 2011

Observing Strategy 2011 Jun 11-18:
We would like to observe some of our primary YSO targets with CLIMB using the telescope configuration E1-E2-W1-W2. For the POP setup, I propose E1(POP2)-E2(POP3)-W1(POP1)-W2(POP5).

With this configuration, many of our primary targets accessible on all sub-triplets.


Sky Map
Media:Target_skymap_YSO_2011Apr.pdf


Calibrator List
Media:Cals_2011Jun.txt


Observing Logs:
please put in here:
Media:CHARA_CLIMB_2011Jun11.txt
Media:CHARA_CLIMB_2011Jun12.txt
Media:CHARA_CLIMB_2011Jun13.txt
Media:CHARA_CLIMB_2011Jun14.txt
Media:CHARA_CLIMB_2011Jun15.txt
Media:CHARA_CLIMB_2011Jun16.txt
Media:CHARA_CLIMB_2011Jun17.txt
Media:CHARA_CLIMB_2011Jun18.txt

Possible observing sequences (spend 2-3 nights on each configuration):
=== Configuration E1-W1-W2, POP215, provides also long baselines and covers wider range of PA:
HD142666 21.0-21.8 (or AS205A 21.0-22.1, V=12.0, with very good conditions!)
(or HD141569 21.0-22.2, V=7.0)
HD150193 21.2-22.5 (=MWC863)
HD163296 22.2-23.8
HD179218 23.5- 1.9 (=MWC614)
HD190073 0.3- 2.7 (=V1295Aql)
MWC340 0.6- 3.7 (or HD344361 23.8- 2.3, V=10.5, with good conditions =WW Vul)
HD200775 22.4- 5.2 (=MWC361) (or MWC1080 2.4- 5.2, V=11.6, with good conditions)
(or LkHa234 23.8- 5.2, V=11.9, with good conditions)

=== Configuration E1-E2-W2, POP235, provides quite good radial sampling of visibility function towards similar PA with intermediate baseline lengths:
HD142666 21.0-21.8 (or AS205A 21.0-22.1, V=12.0, with very good conditions!)
(or HD141569 21.0-22.2, V=7.0)
HD163296 22.2-23.8 (or HD150193 21.2-22.5, V=8.9, =MWC863)
HD179218 22.5- 2.1 (=MWC614) (or HD190073 23.1- 2.7, V=7.2, =V1295Aql)
MWC340 23.8- 4.5
HD200775 22.4- 5.2 (=MWC361)

=== Configuration E2-W1-W2, POP 315
HD142666 21.0-22.7
HD141569 21.0-22.9 (or AS205A 21.0-23.0, V=12.0, with very good conditions)
HD150193 21.2-23.5 (=MWC863)
HD163296 22.2- 0.7
HD179218 23.5- 2.5 (=MWC614)
MWC340 0.3- 4.2
HD200775 22.2- 5.2 (=MWC361) (or MWC1080 1.0- 5.2, V=11.6, with good conditions)

CHARA-ID numbers for YSOs:

MWC 297 = CHARA 320030
MWC 340 = CHARA 320079
MWC 342 = CHARA 320106
MWC 300 = CHARA 320108
V1057 Cyg = CHARA 320109
V1977 Cyg = CHARA 320107
VV Ser = CHARA 320105
Lkha234 = CHARA 320080
MWC1080 = CHARA 320081
AS205A = CHARA 320093

Target list:

Source        Ra            Dec        Weight   V       H       K   SType    Type   Vsini(km/s)  Diam(mas)          Comments
 142666   15 56 40.0    -22 01 40.0     0.00    8.8    6.7    6.1    A8       -      -            -                  =V1026 Sco
 144432   16 06 58.0    -27 43 09.8     0.00    8.2    6.5    5.9    A9       -      -            -                  (2)
 AS205A   16 11 31.3    -18 38 25.9     0.00   12.0    6.7    5.8    -        -      -            -		     =CHARA 320093 (1,2)
 150193   16 40 17.9    -23 53 45.2     0.00    8.9    6.2    5.5    -        -      -            -                  =MWC863 (2)
 163296   17 56 21.3    -21 57 21.9     0.00    6.9    5.5    4.8    A1       HAe    -            -                  =MWC275
 MWC297   18 27 39.5    -03 49 52.0     0.00   12.3    4.4    3.0    -        -      -            -		     =CHARA 320030 (1,2)
 179218   19 11 11.2    +15 47 15.6     0.00    7.2    6.6    6.0    -        -      -            -                  =MWC614 (1)
 MWC340   20 20 28.2    +41 21 51.5     0.00   10.7    6.8    5.7    -        -      -            -                  =V1685 Cyg = CHARA 320079 [need different POP setup]


Notes: (1) The targets AS205A and MWC297 are very promising, but are likely difficult due to the low V-band magnitude. Please try only under exceptional atmospheric conditions. (2) Complements with our VLTI MR/HR-data

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