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 4U 1822-37 276.4461 -37.1042 275.595774 -37.133404 275.279951 -13.781506 356.85149319 -11.29112534 258.4537 54010.4563888889 2006-10-02 10:57:12 54011.5189699074 2006-10-03 12:27:19 401051010 37.7434 40 37.7682 37.7682 37.7434 37.7434 2 2 2 2 1 0 0 33.1785 33.1785 91.8059 0 PROCESSED 57535.7615393518 2016-05-27 18:16:37 54695 2008-08-17 00:00:00 54024.6539814815 2006-10-16 15:41:44 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011121 We propose a 40 ks observation of the accretion disk corona source 4U 1822-37. Despite repeated observations over the years and even excellent high-resolution data from the Chandra Observatory, the nature and origin of the corona and even the source of the Fe K fluorescence emission remains controversial. The spectral resolution of the XIS and the broad-band coverage provided by the combined XIS and HXD instruments make Suzaku uniquely suited to a definitive measurement. Determining the physical conditions in this source is particularly interesting. Because of its geometry 4U 1822-37 is a link between x-ray binaries and AGN, and an therefore serve as a laboratory for studying accretion processes throughout the universe. GALACTIC POINT SOURCES 4 B JEAN COTTAM USA 1 AO1 ACCRETION PHYSICS IN THE ADC SOURCE 4U 1822-37 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401051010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401051010'

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