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
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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