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 | ETA CARINAE | 161.2639 | -59.6881 | 160.777388 | -59.424763 | 202.155739 | -58.924842 | 287.59810122 | -0.63296206 | 310.0122 | 55766.0329398148 | 2011-07-24 00:47:26 | 55766.9286226852 | 2011-07-24 22:17:13 | 406039010 | 42.0302 | 50 | 42.0302 | 42.0302 | 0 | 42.0302 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 49.0937 | 49.0937 | 77.3839 | 0 | PROCESSED | 57602.6625462963 | 2016-08-02 15:54:04 | 56163 | 2012-08-24 00:00:00 | 55785.0281712963 | 2011-08-12 00:40:34 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061205 | Eta Car is the nearest highly unstable extremely massive star and a key object for understanding how mass and angular momentum change as an extremely massive star heads towards hypernova. Periodic minima in X-rays and other wavebands show it as an extremely eccentric binary with a massive companion. A surprising change in the X-ray emission during the January 2009 X-ray minimum probably indicates a large-scale variation in the LBV primary's mass loss rate. We propose a Suzaku observation in AO6 to monitor the change of the absorption column in the line of sight and the non-thermal emission above 10 keV. The observation will help to study geometry of the binary orbit of Eta Car and the mechanism of the non-thermal emission. | GALACTIC POINT SOURCES | 4 | B | KENJI HAMAGUCHI | USA | 6 | AO6 | MONITORING DYNAMICAL MASS LOSS FROM ETA CAR WITH SUZAKU: APASTRON | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406039010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406039010'
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