70-107
Determining the progenitor types of interacting supernovae
PI: Andrea Reguitti
Observing instructions:
Go to the directory
cd ~/scripts/70-107
execute the requested scripts.
| Program Tracking |
| Proposal |
70-107 |
| Semester |
P70: 20241001 - 20250401 |
| Principal Investigator |
Reguitti |
| Programme |
Determining the progenitor types of interacting supernovae |
| Instrument |
ALFOSC |
| Time Allocation |
2-3 transients followed over 6 epochs |
| Total Nights |
1.3 |
| Type |
ToO+SoftToO |
| Notes |
Override, but should aim for (soft) triggers during Nordic service or Technical nights |
| Total Time Spent |
03:32 (hh:mm)
|
| Proposal |
Date |
Time |
Type |
Targets |
Files |
Comments |
Status |
|
| 70-107 |
2024-10-10 |
00:35 |
SoftToO |
SN2024ueo |
ALHj100115 - ALHj100119 |
Clear skies and sub-arcsec seeing. |
Observed |
|
| 70-107 |
2024-10-18 |
00:42 |
SoftToO |
Feige110, SN2024vku |
ALHj180150 - ALHj180160 |
Targets observed with clear skies and sub-arcsecond seeing. |
Observed |
|
| 70-107 |
2024-10-31 |
01:05 |
SoftToO |
AT2024qtn |
ALHj310154 - ALHj310158 |
Seeing was ~1.2'' at the start of the observation. There is light from both the galaxy and the source in the slit. Strong spectral features in Quickspec. The standard was not observed, because another standard star with the same setup (Grism 4 and 1.0'' slit) was obtained. These calibration files are ALHj310148 & ALHj310149. |
Observed |
|
| 70-107 |
2024-11-10 |
00:19 |
SoftToO |
AT2024qtn |
ALHk100209 - ALHk100213 |
Observed with clear, dusty skies and seeing around 1 arcsec. |
Observed |
|
| 70-107 |
2024-11-13 |
00:51 |
SoftToO |
AT2024qtn |
ALHk130109 - ALHk130113 |
Target was observed in clear skies with seeing around 1.0" |
Observed |
|
| 70-107 |
2024-11-18 |
00:00 |
SoftToO |
|
|
No observations could be done due to bad weather |
Failed |
|
| 70-107 |
2024-11-19 |
00:00 |
SoftToO |
|
|
Targets could not be observed due to high humidity |
Failed |
|
The above information is collected from the ToO/Mon reports that have been created by the observer.
Should any of the observations have been carried out using the OB system, you will find additional information
HERE
|
