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 | EG AND | 11.168 | 40.673 | 10.482613 | 40.399604 | 27.902454 | 32.653699 | 121.54657283 | -22.18054863 | 225.2111 | 55597.6281018518 | 2011-02-05 15:04:28 | 55600.0030092593 | 2011-02-08 00:04:20 | 405034010 | 100.5333 | 100 | 100.5333 | 100.5413 | 0 | 100.5493 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 84.6589 | 84.6589 | 205.1719 | 3 | PROCESSED | 57600.9241666667 | 2016-07-31 22:10:48 | 55983 | 2012-02-26 00:00:00 | 55614.2972106482 | 2011-02-22 07:07:59 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051211 | The goals of this proposal are to use Suzaku XIS observations to : 1) determine whether EG And, BX Mon, and BF Cyg are members of the recently recognized class of hard X-ray emitting symbiotic stars; and 2) if they are, compare the nature of any absorption, the optical depth of the boundary layer, and the accretion rate to those of the well established hard X-ray symbiotics. Understanding the accretion processes in symbiotic stars is a crucial step in determining the role they play as progenitors of type Ia supernovae. | GALACTIC POINT SOURCES | 4 | C | THOMAS NELSON | USA | 5 | AO5 | EXPLORING THE ACCRETION DISK BOUNDARY LAYERS OF SYMBIOTIC STARS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405034010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '405034010'
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