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
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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