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 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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