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GCN Circular 21772

Subject
LIGO/Virgo G299232: GRAWITA Asiago optical observations
Date
2017-08-31T10:39:34Z (8 years ago)
From
Lina Tomasella at INAF/OAPd <lina.tomasella@oapd.inaf.it>
L. Tomasella, S. Benetti, E. Cappellaro (INAF-OAPD), G. Greco (Urbino University/INFN Firenze), L. Amati (INAF-IASF Bo), L. A. Antonelli, S. Ascenzi (INAF-OAR),  M.T. Botticella (INAF-OAC), M. Branchesi (GSSI), S. Campana, S. Covino, P. D'Avanzo (INAF-OAB), V. D'Elia (INAF-ASDC), D. Fugazza, F. Getman, A. Grado (INAF-OAC), L. Limatola (INAF-OAC), M. Lisi (INAF-OAR), A. Melandri (INAF-OAB), L. Nicastro, E. Palazzi, E. Pian (INAF-IASF Bo), S. Piranomonte, L. Pulone (INAF-OAR), A. Rossi (INAF-IASF Bo), P. Schipani (INAF-OAC), G. Stratta (Urbino University/INFN Firenze), G. Tagliaferri (INAF-OAB), V. Testa (INAF-OAR), S. Yang (INAF-OAPD), E. Brocato (INAF-OAR) on behalf of GRavitational Wave Inaf TeAm report:



We carried out follow up observations of LIGO/Virgo G299232 (LVC, GCN 21693) with the Schmidt 67/92 telescope located at Cima Ekar (Asiago, Italy). 
Sloan gr-bands images were taken on 2017-08-26 starting from UT 00:10:21. 
The pointing sequence was generated using the GWskyscript (https://github.com/ggreco77/GWsky) starting from the high probability region of 
the bayestar skymap and taking into account the airmass and relative density of nearby galaxies.
Each pointing covers 1x1 square degrees of the sky with 3x180 sec exposure time per band.
The pointing blocks are centered on the following coordinates RA, Dec (J2000) and UT starting times of exposures:

a. 36.76037 +61.84232  2017-08-26T00:06:58  
b. 41.81579 +63.26814  2017-08-26T00:47:35
c. 28.76182 +34.24004  2017-08-26T01:15:13  
d. 29.34192 +32.22710  2017-08-26T01:41:33  
e. 25.77839 +32.19475  2017-08-26T02:06:24  
f. 28.89056 +30.76806  2017-08-26T02:30:09

The single exposure is characterised by an AB limiting magnitude of r > 22.

We also observed with the Copernico 1.82m telescope (Cima Ekar, Asiago, Italy) and equipped with AFOSC instrument. 
Sloan g and r-bands images (FOV = 8.8 X 8.8 arcmin) 
were taken on 2017-08-26 starting from UT 00:18:10 either of seven nearby galaxies whose location on the sky and distance falls in the 90% volume reported by the 
BAYESTAR probability sky map (Singer et al. 2016) and listed by Cook et al. 2017 in GCN n. 21707 (pointing 1-7), 
and generated using the GWskyscript (https://github.com/ggreco77/GWsky; pointing 8-11):

1.  IC 1695                   2017-08-26T01:44:39
2.  UGC01400                  2017-08-26T01:53:39
3.  UGC00774                  2017-08-26T01:59:13
4.  IC0260                    2017-08-26T02:07:20
5.  NGC0326                   2017-08-26T02:13:02
6.  SDSS J014929.88+123032.4  2017-08-26T02:18:27
7.  MRK 0567                  2017-08-26T02:30:00
8.  27.83787 +33.058979       2017-08-26T00:15:07
9.  30.54151 +52.365807       2017-08-26T00:29:12
10. 24.86730 +18.979811       2017-08-26T01:04:49
11. 28.69988 +31.314634       2017-08-26T01:29:22

Preliminary analysis do not show new transients in these fields.
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