Observers: Daniele Melasani, Adam Rubin
Support Team: Giorgos Leloudas, Kasper Elm Heintz
TAT: Joe Anderson, Kate Maguire
Weather: Clear, ~1'' seeing..
| UT |
Object |
setup |
slit |
exp |
airmass |
DIMM |
Acquisition Image quality |
Comments |
| 23:22 |
ASASSN-18fv + sky |
JHK burst |
|
1.6 |
1.34 |
|
1.26 |
|
| 23:29 |
2MASS_10360106-5937105 + sky |
JHK burst |
|
1.6 |
|
|
|
|
| 23:38 |
ASASSN-18fv + sky |
BG, RG |
|
6,7.5 |
|
|
1 |
|
| 23:48 |
HIP053982 |
BG, RG |
|
|
1.24 |
|
|
|
| 23:56 |
LTT3218 |
BG, RG |
|
|
1.01 |
|
1.4 |
|
| 00:04 |
SN2018oh |
JHK |
|
30x4, 72x4, 60x6 |
|
|
|
|
| 00:27 |
SN2017ijn |
JHK |
|
15x4, 36x4, 40x4 |
|
|
1.2 |
|
| 00:34 |
SN2018ec |
JHK |
|
90x12, 100x12, 90x16 |
1.09 |
|
|
PSF looks elongated |
| 02:11 |
SN2018agk |
JHK |
|
100x4, 90x4, 90x8 |
1.1 |
1 |
1 |
First two acq images should be discarded. Refocused the telescope. Improved image quality after refocus. |
| 02:40 |
SN2017jfs |
JHK |
|
|
1.36 |
0.9 |
|
|
| 04:00 |
|
|
|
|
|
|
|
Switch to EFOSC |
| 04:22 |
ASASSN-18fv |
g11,16,18,20 |
1 |
6, 4.5, 10.5, 10.5 |
1.26 |
0.8 |
|
saturated! |
| 04:30 |
ASASSN-18fv |
g11,16,18,20 |
1 |
3x1,3x1.5,3x1.5,3x0.7 |
|
|
1 |
grism 18, and 20 have a |
| 04:47 |
ASASSN-18fv |
g18,20 |
1 |
1x3, 1x3 |
|
|
|
redid 16 and 18 |
| 05:08 |
LTT3864 |
|
|
|
1.3 |
1.4 |
1 |
|
| 05:36 |
AT2018aqi |
g13 |
1 |
300 |
1.3 |
1.3 |
1.5 |
|
| 05:47 |
AT2018aqh |
g13 |
1 |
300 |
1.9 |
1.6 |
1.5 |
|
| 06:01 |
AT2018aqj |
g13 |
1 |
300 |
1.57 |
1.05 |
1.1 |
|
| 06:19 |
AT2018apm |
g13 |
1 |
600 |
1.3 |
1 |
1 |
|
| 06:36 |
AT2018apo |
g13 |
1 |
300 |
1.16 |
0.9 |
0.8 |
|
| 06:50 |
AT2018ail |
g13 |
1.5 |
900 |
1.4 |
0.9 |
1.2 |
Can’t identify sn. Positioning slit on the nucleus of the galaxy w/ 1.5’’ slit |
| 07:24 |
SN2018agk |
g16 |
1 |
1500 |
1.4 |
0.8 |
1.1 |
|
| 08:03 |
AT2018aqn |
g13 |
1 |
300 |
1.26 |
0.84 |
0.9 |
|
| 08:15 |
AT2017gge |
g18, g, r |
1 |
3600, 600, 600 |
1.7 |
1.4 |
1.1 |
spectroscopy + photometry |
| 09:52 |
EG274 |
g11, 13, 16 |
|
|
|
|
|
did not have time to do g18,20 |
| 10:13 |
Flats |
g, r, z |
|
|
|
|
|
|
|
|
