DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | ARK 564 | 340.6583 | 29.7351 | 340.07073 | 29.472916 | 355.35057 | 34.71587 | 92.13955378 | -25.32593551 | 75.7895 | 57167.0898842593 | 2015-05-25 02:09:26 | 57168.4029282407 | 2015-05-26 09:40:13 | 710018010 | 52.5104 | 50 | 52.5104 | 53.9344 | 0 | 53.9344 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 27.9802 | 27.9802 | 100.9477 | 2 | PROCESSED | 57618.7636921296 | 2016-08-18 18:19:43 | 57548 | 2016-06-09 00:00:00 | 57178.248587963 | 2015-06-05 05:57:58 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 102721 | A NuSTAR legacy is emerging through long observations of bare Seyfert galaxies that reveal an unprecedented look at relativistic reflection off an ionized accretion disc. We propose now to look at the Seyfert galaxy Ark 564 for 200 ks with NuSTAR and 50 ks with Suzaku in order to understand the reflection in this bright source. Ark 564 has been well-studied in the soft band, revealing a steep spectrum, strong soft excess, broad iron K emission line and dramatic variability on the order of hours. It is very akin to two other well-known bare Seyferts, 1H0707-405 and IRAS 13224-3809, except it is an order of magnitude brighter. With this 200 ks observation, we will probe the geometry of the corona, through a complete spectral and timing analysis. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | ERIN KARA | EUR | 10 | AO10 | UNDERSTANDING REFLECTION IN THE BARE SEYFERT I ARK 564 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/710018010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '710018010'
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