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 120 79.0439 -0.2064 78.404432 -0.260846 78.068932 -23.195412 201.74563913 -21.16237248 274.9546 54191.755162037 2007-04-01 18:07:26 54193.905150463 2007-04-03 21:43:25 702014010 100.8635 100 100.8635 100.8635 0 100.8635 2 2 0 2 1 0 0 95.3121 95.3121 185.7439 1 PROCESSED 57538.0955324074 2016-05-30 02:17:34 54744 2008-10-05 00:00:00 54200.5657060185 2007-04-10 13:34:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020035 We propose to obtain the broad-band spectra of the bright Seyfert 1 Ark 120 with Suzaku. Since Ark 120 shows no strong absorption features in its X-ray spectrum, we can cleanly measure the shape of the continuum and Fe K line without introducing any ambiguity caused by absorption along the line of sight. The spectrum will be used to test the diskline hypothesis in Seyferts and to study the fundamental processes producing broad band spectra of AGNs. EXTRAGALACTIC COMPACT SOURCES 7 A YUICHI TERASHIMA JAP 2 AO2 THE ORIGIN OF THE BROAD FE LINE IN THE SEYFERT 1 ARK 120 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702014010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702014010'

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