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 | CH CYG | 291.1621 | 50.2424 | 290.833167 | 50.142645 | 313.7082 | 70.490137 | 81.86550652 | 15.56609243 | 185.7481 | 53739.5736458333 | 2006-01-04 13:46:03 | 53740.2919560185 | 2006-01-05 07:00:25 | 400016020 | 33.3058 | 25 | 33.3075 | 33.3378 | 33.3155 | 33.3058 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 28.4615 | 28.4615 | 62.056 | 1 | PROCESSED | 57532.6355902778 | 2016-05-24 15:15:15 | 54247 | 2007-05-27 00:00:00 | 54039.6712268518 | 2006-10-31 16:06:34 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001082 | CH Cygni is a symbiotic star in which a white dwarf is believed to be accreting the wind of the red giant. ASCA observation revealed a complex X-ray spectrum consisting of a heavily absorbed hard component and a relatively unabsorbed soft component. We propose to obtain the spectrum of CH Cyg above 10 keV for the first time using Suzaku HXD (PIN), while simultaneously obtaining high quality spectrum below 10 keV with the XIS. | GALACTIC POINT SOURCES | 4 | A | KOJI MUKAI | JAP | 0 | SWG | SUZAKU OBSERVATION OF THE SYMBIOTIC SYSTEM CH CYGNI | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400016020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '400016020'
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