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 | SGR 1806-20 | 272.1607 | -20.4008 | 271.416415 | -20.409492 | 272.01832 | 3.024829 | 10.00344249 | -0.23433657 | 89.0334 | 56010.449837963 | 2012-03-24 10:47:46 | 56012.5314814815 | 2012-03-26 12:45:20 | 406069010 | 70.5964 | 70 | 70.5964 | 70.5964 | 0 | 70.5964 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 63.9571 | 63.9571 | 179.8279 | 2 | PROCESSED | 57605.0500462963 | 2016-08-05 01:12:04 | 56399 | 2013-04-17 00:00:00 | 56023.2387384259 | 2012-04-06 05:43:47 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061301 | Recent Suzaku investigations revealed that a broad-band (0.8-70 keV) spectra of known magnetars systematically change depending on their characteristic ages. The hard X-rays of magnetars become weaker but harder for older objects. In order to accomplish this picture, we have to verify that this correlation is rather free from selection effects, and holds even when the sources vary on long time scales. Here we propose a 70 ks observation of SGR 1806-20. If we detect the hard X-rays from this source at a rather intensity, the above correlation will be much reinforced. | GALACTIC POINT SOURCES | 4 | C | TERUAKI ENOTO | USA | 6 | AO6 | VARIABILITY OF HARD X-RAYS FROM MAGNETARS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406069010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406069010'
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