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 GX17+2 274.0087 -14.1006 273.298097 -14.118345 273.929719 9.285377 16.37694194 1.24456043 269.7113 54362.2773032407 2007-09-19 06:39:19 54362.8543402778 2007-09-19 20:30:15 402050010 19.0959 20 19.0959 19.1044 0 19.0959 2 1 0 2 1 0 0 16.0445 16.0445 49.8499 0 PROCESSED 57540.0136458333 2016-06-01 00:19:39 54751 2008-10-12 00:00:00 54384.4487037037 2007-10-11 10:46:08 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021111 Z sources are bright low-mass X-ray binaries with variable spectra that describe a characteristic "Z" shape in an X-ray color-color plot. The forces driving the spectral shape and variability of the Z sources are not well understood, as there are few detectors with the necessary capabilities. GX17+2 is a Sco-type Z sources with an unusual time-varying hard X-ray tail whose origin is uncertain. Bright X-ray sources also illuminate the interstellar medium. Highly absorbed X-ray sources show halos due to dust scattering as well as absorption features. These will allow us to place constraints on interstellar dust and gas models. Suzaku can address all of these issues with simultaneous observations of the hard X-ray continuum and the dust-scattered X-ray halo. GALACTIC POINT SOURCES 4 A RANDALL SMITH USA 2 AO2 OBSERVING THE SPECTRUM AND HALO OF GX17+2 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402050010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402050010'

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