NGC7314
We propose to observe the bright Sy1.9 NGC 7314 as the ideal candidate to unveil the structure and physical conditions through emission lines from cold and ionized material. We will investigate the iron K alpha and K beta narrow and broad emission components and disentangle the contribution to the line of the distant reflector, disk and broad line region. This source is also ideal to study the prominent emission from ionized gas and determine its origin and geometry.
obsid = 201124010 / Unique Observation/Sequence Number
object = NGC7314 / Object name
pi_name = COSTANTINI ELISA / Proposal Principal Investigator Name
ra = 338.942099196663 / Right Ascension (Pointing Position) (deg)
dec = -26.0502297693447 / Declination (Pointing Position) (deg)
roll_angle = 74.0222785508898 / Roll Angle (deg)
start_time = 2025-06-13T20:07:04 / Start Time of the Observation
stop_time = 2025-06-15T17:39:04 / Stop Time of the Observation
exposure = 89615.575444 / Effective Total Observation Exposure (s)
public_date= 2026-06-25 / Public Date