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 | 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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