Difference between revisions of "EGAL10 C2"
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When checking the RTA for Perseus-MA, note that the pivot of the wobbles has no sources, The targets of these observations are actually NGC1275 and IC310, which are located at | When checking the RTA for Perseus-MA, note that the pivot of the wobbles has no sources, The targets of these observations are actually NGC1275 and IC310, which are located at | ||
| − | + | NGC1275 (RA): 3h:19m:48.4s, (Dec): +41:30:41 | |
| − | + | IC310 (RA): 3h:16m:43.0s, (Dec): +41:19:29 | |
Revision as of 11:31, 17 April 2024
Contents
Proposal
Proposal: EGAL10:Monitoring of classical radio galaxies with LST-1
PI: Mireia Nievas Rosillo (mnievas@iac.es)
Source information
Source: Perseus-MA
RA (J2000): 49.563 deg
Dec (J2000): 41.4181 deg
Source: M87
RA (J2000): 187.708 deg
Dec (J2000): 12.39 deg
Observational settings/limits
Perseus-MA Min Zenith [deg] = 0
Max Zenith [deg] = 50
Night Sky Background = Both
Wobbles = W0.26+108 W0.26+288
M87 Min Zenith [deg] = 0
Max Zenith [deg] = 50
Night Sky Background = Both
Wobbles = Standard
Instructions for shifters
When checking the RTA for Perseus-MA, note that the pivot of the wobbles has no sources, The targets of these observations are actually NGC1275 and IC310, which are located at
NGC1275 (RA): 3h:19m:48.4s, (Dec): +41:30:41 IC310 (RA): 3h:16m:43.0s, (Dec): +41:19:29
