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 NGC 4593 189.9132 -5.341 189.26831 -5.066485 191.201043 -0.986248 297.48043001 57.40595243 111.8998 57021.7640856482 2014-12-30 18:20:17 57025.333287037 2015-01-03 07:59:56 709014050 145.2819 30 145.2819 145.3032 0 145.2899 1 1 0 1 0 0 0 0 0 0 0 PROCESSED 57617.5760069445 2016-08-17 13:49:27 57415 2016-01-28 00:00:00 57049.4542939815 2015-01-27 10:54:11 3.0.22.44 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090097 In the AO-8 cycle, we proposed six X-ray and optical simultaneous observations of type I Seyfert galaxy NGC 3516, and now obtaining a good correlation between those wavelengths. In the observations, we confirmed that a hard X-ray primary component (HXPC) found in Noda et al. (2013) was dominant, and its variation is well correlated with an optical one. To verify the probability that a variation of HXPC in other Seyfert also correlates with that in its optical, we propose six X-ray and optical simultaneous observations of NGC 4593, which has an X-ray spectrum dominated by HXPC as well as NGC 3516 in 2013. EXTRAGALACTIC COMPACT SOURCES 7 A HIROFUMI NODA JAP 9 AO9 X-RAY AND OPTICAL SIMULTANEOUS OBSERVATIONS OF TYPICAL TYPE I SEYFERT NGC 4593 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709014050/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '709014050'

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