GCN Circular 20717
Subject
LIGO/Virgo G274296: iPTF Optical Transient Candidates
Date
2017-02-22T01:11:33Z (8 years ago)
From
Mansi M. Kasliwal at Caltech <mansi@astro.caltech.edu>
R. Ferretti (OKC), R. Lunnan (Caltech), M. M. Kasliwal (Caltech), L. P.
Singer (NASA/GSFC), S. B. Cenko (NASA/GSFC), D. Cook (Caltech), C. Cannella
(Caltech), A. van Sistine (UWM), T. Barlow (Caltech), V. Bhalerao (IUCAA),
J. Rana (IUCAA), A. A. Miller (Northwestern/Adler), Y. Cao (UW)
report on behalf of the iPTF (intermediate Palomar Transient Factory) and
GROWTH (Global Relay of Observatories Watching Transients Happen)
collaborations:-
We performed tiled observations of LIGO/Virgo G274296 (LVC, GCN 20689)
using the Palomar 48-inch Oschin telescope (P48) on the night of 2017-02-21
UTC. We imaged 111 fields spanning 807 square degrees, with a 54% chance of
containing the true location of the source. Of these, 69 fields (502 square
degrees; 42% probability) were imaged twice and searched for transient
candidates.
During preliminary sifting through candidate variable sources using image
subtraction by our IPAC pipeline (Masci et al. 2016), and applying standard
iPTF vetting procedures, we flagged the following optical transient
candidates (60 total) for further follow-up:
name RA Dec time mag
z notes
-------- ---------- ---------- ----- -----
------ ---------
iPTF17bed 234.991732 +34.088243 2457806.0160 20.17
0.138 photz; at edge of galaxy
iPTF17bec 232.665446 +33.928645 2457806.0160 19.90
0.0482 specz; irregular galaxy; fading (0.34 mag intra-night)
iPTF17beb 235.828735 +32.682827 2457806.01757 19.03
0.07 photz
iPTF17bdz 174.715936 +33.828372 2457805.90013 20.05
0.0327 specz; nuclear edge-on
iPTF17bdy 178.129375 +35.456339 2457805.90162 20.30
0.0943 specz; slightly off-center
iPTF17bdw 178.329915 +36.442293 2457805.90313 20.29
0.18 photz
iPTF17bds 183.323594 +39.266026 2457805.9061 20.11
0.13 photz; fading (0.40 mag intra-night)
iPTF17bdq 181.290430 +37.270222 2457805.90762 19.94
0.0226 specz
iPTF17bdp 182.529730 +36.393440 2457805.90762 20.08
0.2432 specz; nuclear (SDSS QSO)
iPTF17bdn 184.075520 +40.796273 2457805.93462 20.57
0.136 photz
iPTF17bdl 183.608407 +42.063649 2457805.9346 19.65
0.0231 specz; nuclear?
iPTF17bdk 186.611638 +40.726698 2457805.9346 20.55
0.0699 specz; nuclear?
iPTF17bdj 185.368397 +42.208415 2457805.93462 19.51
0.1206 specz
iPTF17bdf 188.315478 +36.824458 2457805.93763 19.68
0.095 photz
iPTF17bde 187.281321 +36.457123 2457805.93763 19.58
0.0714 specz; slightly off-center
iPTF17bdd 191.013043 +41.168996 2457805.93912 19.04
0.0237 specz; nuclear?; rising (0.48 mag intra-night)
iPTF17bdc 192.553197 +36.464676 2457805.9421 20.49
0.1448 specz; at edge of galaxy
iPTF17bda 193.915287 +39.855467 2457805.9436 19.21
0.38 photz
iPTF17bcz 196.354965 +39.004452 2457805.9436 19.59
0.0808 specz; off-center
iPTF17bcy 197.058084 +41.600850 2457805.9466 20.23
0.0272 specz
iPTF17bcw 201.468624 +39.173964 2457805.94814 20.65
0.0636 specz
iPTF17bcs 198.456906 +38.894402 2457805.94814 19.60
0.0794 spez; nuclear
iPTF17bcr 200.757880 +40.201309 2457805.9481 20.35
0.0640 specz
iPTF17bcn 201.030920 +42.445651 2457805.95116 19.99
0.079 photz; nuclear
iPTF17bcl 207.110772 +41.975701 2457805.95416 20.44
0.183 photz
iPTF17bck 208.258285 +40.302280 2457805.95715 19.85
? no photz available
iPTF17bci 209.602490 +43.662936 2457805.95867 19.74
0.065 specz; nuclear
iPTF17bch 209.362268 +44.387701 2457805.95867 19.65
0.072 specz; nuclear?
iPTF17bcg 211.528986 +42.673631 2457805.96015 19.37
0.088 specz
iPTF17bce 212.679949 +37.081015 2457805.96316 20.37
0.224 photz
iPTF17bbv 174.674325 +36.232952 2457805.8986 18.27
0.05996 specz
iPTF17bbu 167.125966 +31.440313 2457805.8911 19.70
0.06 photz
iPTF17bbt 166.948991 +31.255977 2457805.8911 20.02
0.087 photz
iPTF17bbs 166.950771 +31.311975 2457805.8911 19.95
0.072 specz
iPTF17bbq 168.377846 +29.667545 2457805.8911 20.25
0.0455 specz; =PS17bew (GCN 20699)
iPTF17bbp 166.537702 +30.246383 2457805.8911 19.95
0.030 specz
iPTF17bbn 167.184990 +31.218324 2457805.8911 19.29
0.073 specz; also detected 2017-02-17 (g=20.11); nuclear
iPTF17bbg 169.748759 +35.743451 2457805.89411 19.89
0.104 specz
iPTF17bbf 170.901072 +34.765936 2457805.89411 19.60
0.186 photz
iPTF17bbe 170.036330 +34.312810 2457805.89411 20.49
0.037 specz; nuclear (SDSS AGN)
iPTF17bbb 170.475973 +33.961040 2457805.89411 20.11
0.078 photz
iPTF17bba 170.464827 +33.845571 2457805.89411 19.88
0.044 specz
iPTF17baz 170.427019 +34.363034 2457805.89411 19.05
0.035 specz
iPTF17bav 168.441386 +37.278479 2457805.8956 19.61
0.100 specz
iPTF17bat 171.393094 +40.511821 2457805.89712 20.01
0.122 specz
iPTF17baq 134.698013 +01.842508 2457805.78102 19.70
0.058 specz; nuclear?
iPTF17bap 134.438423 +00.933616 2457805.78102 19.80
0.120 specz; nuclear
iPTF17bao 133.976313 +00.853143 2457805.78102 19.41
0.053 specz; nuclear (SDSS AGN)
iPTF17bam 134.670596 +02.078209 2457805.78102 19.88
0.125 specz; rising (0.35 mag intra-night)
iPTF17bal 138.036706 +06.780975 2457805.78255 19.72
0.143 specz; nuclear
iPTF17bak 138.746540 +05.045414 2457805.78404 20.55
0.143 specz; nuclear (SDSS AGN); rising (0.39 mag intra-night)
iPTF17bai 141.156805 +08.409091 2457805.78853 19.97
0.129 specz; nuclear?
iPTF17bah 141.492784 +08.840897 2457805.78853 20.51
0.107 specz; nuclear?; rising (0.59 mag intra-night)
iPTF17bag 137.893562 +06.774493 2457805.78255 20.20
0.225 photz; nuclear
iPTF17bad 141.730214 +08.380390 2457805.78853 19.72
0.122 specz; nuclear?
iPTF17baa 133.693265 +01.183738 2457805.78102 19.46
0.066 photz
iPTF17aas 170.123758 +34.754070 2457805.89411 18.96
0.042 specz; =SN2017aas=PTSS-17dib=PS17bey, known SNIa.
iPTF17mf 214.129450 +39.586295 2457805.96167 17.21
0.0257 specz; =SN2017mf, known SNIa.
iPTF17jg 204.057109 +38.348005 2457805.94963 18.57
0.014 specz; =ATLAS17aic, first discovered 2017-01-09
iPTF17hy 202.138887 +39.486881 2457805.94963 20.18
0.064 specz; =Gaia17abk=PS17hc, first discovered 2017-01-12.
Positions are stated in the ICRS. Times are in UTC. Magnitudes are based on
image subtraction; they are in the Mould R filter and in the AB system,
calibrated with respect to point sources in SDSS as described in Ofek et
al. 2012.
None of the above transients show prior history of detection in iPTF
archival images. All of the above transients coincide with a galaxy that is
visible in iPTF and/or SDSS images. Archival spectroscopic or photometric
redshifts of the transients' likely host galaxies are given above.
We cross-matched this list to our ongoing effort to build a more complete
Census of the Local Universe (CLU; Cook et al. 2017) by identifying
redshifted Halpha emitters out to 200 Mpc. The hosts of iPTF17bdq,
iPTF17bdl, iPTF17bcy, iPTF17bcn, iPTF17bbe, and iPTF17bbb, are viable
emission line candidates.
We encourage spectroscopic classification of these candidates. In
particular, we highlight iPTF17bec, iPTF17bds, iPTF17bdd, iPTF17bam, and
iPTF17bah as fast-evolving by more than 0.3 mag in the same night. In
addition, our local transients (d < 100 Mpc) are iPTF17jg, iPTF17bdq,
iPTF17bbp, iPTF17bdl, and iPTF17bdd, and our bright transients (R < 19 mag)
are iPTF17bbv, iPTF17jg, iPTF17bdd, iPTF17baz, and iPTF17beb.