CLIMB Observing Run 2011Apr: Difference between revisions

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(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.
(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
(2) Complements with our VLTI MR/HR-data
For the first half nights, we would like to observe Regulus and some its calibrators with PAVO 2T. The best configurations are (S1, S2, E2) - W2, pops: 1 - 5.
UV coverage:
[[Media:UV_REGULUS_PAVO_2T_S1-W2_2011-04-21.pdf]]
[[Media:UV_REGULUS_PAVO_2T_S2-W2_2011-04-21.pdf]]
[[Media:UV_REGULUS_PAVO_2T_E2-W2_2011-04-21.pdf]]
Observability:
[[Media:OBS_PAVO_2T_S1-W2_2011-04-21.pdf]]
[[Media:OBS_PAVO_2T_S2-W2_2011-04-21.pdf]]
[[Media:OBS_PAVO_2T_E2-W2_2011-04-21.pdf]]

Latest revision as of 07:54, 20 April 2011

Observing Strategy:
We would like to observe some of our primary YSO targets with CLIMB on the telescope configuration S1-E1-W1 (first priority) and S2-E2-W2 (second priority). If telescope S1 is not available, please replace with telescope S2 (and vice versa). For the POP setup, I propose S1(POP5)-S2(POP4)-E1(POP1)-E2(POP1)-W1(POP1)-W2(POP5).

First night: I suggest starting on S1-E1-W1 (POPs: 5-1-1) and to observe HD142666 (LT 23.9-1.8), HD144432 (LT 0.7-1.5), AS205A (LT 0.1-2.3, only with excellent seeing conditions), HD150193 (LT 0.9-2.4), HD163296 (LT 1.9-3.8), MWC297 (LT 2.7-5.0, only with excellent seeing conditions), HD179218 (LT 4.6-5.5).

Second night: If the first night was relatively successful, I suggest switching to S2-E2-W2 (POPs: 4-1-5) and to observe HD142666 (LT 23.9-5.1), AS205A (LT 24.0-5.4, only with excellent seeing conditions), HD144432 (LT 0.7-3.4), HD150193 (LT 0.9-5.8), MWC297 (LT 2.7-5.8, only with excellent seeing conditions), HD179218 (LT 5.2-5.8).


Sky Map
Media:Target_skymap_YSO_2011Apr.pdf


Calibrator List
Media:Cals_2011Apr.txt


Observing Logs:
please put in here:
Media:CHARA_CLIMB_2011Apr21.txt
Media:CHARA_CLIMB_2011Apr22.txt

CHARA-ID numbers for YSOs:

MWC 297 = CHARA 320030
MWC 340 = CHARA 320079
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


For the first half nights, we would like to observe Regulus and some its calibrators with PAVO 2T. The best configurations are (S1, S2, E2) - W2, pops: 1 - 5.

UV coverage:

Media:UV_REGULUS_PAVO_2T_S1-W2_2011-04-21.pdf

Media:UV_REGULUS_PAVO_2T_S2-W2_2011-04-21.pdf

Media:UV_REGULUS_PAVO_2T_E2-W2_2011-04-21.pdf

Observability:

Media:OBS_PAVO_2T_S1-W2_2011-04-21.pdf

Media:OBS_PAVO_2T_S2-W2_2011-04-21.pdf

Media:OBS_PAVO_2T_E2-W2_2011-04-21.pdf

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