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 | TON S180 | 14.333 | -22.3803 | 13.720307 | -22.650448 | 3.73482 | -26.131336 | 138.98529016 | -85.06726133 | 237.1425 | 54078.5680671296 | 2006-12-09 13:38:01 | 54081.3584953704 | 2006-12-12 08:36:14 | 701021010 | 120.6609 | 120 | 120.6849 | 120.6609 | 0 | 120.6769 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 109.3128 | 109.3128 | 241.052 | 3 | PROCESSED | 57536.3458680556 | 2016-05-28 08:18:03 | 54735 | 2008-09-26 00:00:00 | 54094.4773958333 | 2006-12-25 11:27:27 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010141 | TON S180 is a luminous Narrow Line Seyfert 1 galaxy, chracterizing enhanced Soft X-ray emission component without complex absorption/emission structures. The source is considered to be at super Eddington accretion rate. We aim to track change (or no change) in soft X-ray spectrum of this source according to factor of two ,rapid flux variation this source show. We partciularly focus on the slim disk model propsed for super Eddington accretion disk. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | KIYOSHI HAYASHIDA | JAP | 1 | AO1 | SOFT X-RAY EMISSION FROM SUPER-EDDINGTON ACCRETION DISK IN TON S180 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701021010'
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