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 | SS CYG | 325.6789 | 43.5736 | 325.187819 | 43.344381 | 350.451149 | 52.649921 | 90.55119171 | -7.12024619 | 276.5788 | 53676.0503703704 | 2005-11-02 01:12:32 | 53676.9856944444 | 2005-11-02 23:39:24 | 400006010 | 39.4512 | 40 | 39.4512 | 39.4512 | 39.4512 | 39.4512 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 32.0472 | 32.0472 | 80.81 | 1 | PROCESSED | 57527.7175925926 | 2016-05-19 17:13:20 | 54247 | 2007-05-27 00:00:00 | 54036.9898148148 | 2006-10-28 23:45:20 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001043 | Although the boundary layer that is formed between the rapidly rotating inner accretion disk and the white dwarf surface has been known as a hard-X-ray emitter, its geometry and structure has not been well understood yet. We aim to investigate the boundary layer structure with SS Cyg, the brightest dwarf nova, by means of a soft X-ray component with the BI CCD, a fluorescent Fe K-alpha line with the FI CCDs, and a continuum reflection by the white dwarf surface with the HXD PIN. It is of great use to observe states of a different mass accretion rate, and hence we propose to observe both in quiescence and in outburst. | GALACTIC POINT SOURCES | 4 | A | MANABU ISHIDA | JAP | 0 | SWG | SS CYG OBSERVATION IN QUIESCENCE | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400006010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '400006010'
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