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 3C279 194.0685 -5.7338 193.421343 -5.463366 195.163667 0.26086 305.14803375 57.11713803 113.6423 54850.9795833333 2009-01-19 23:30:36 54853.9391203704 2009-01-22 22:32:20 703049010 134.1106 200 134.1106 134.1106 0 134.1106 2 2 0 2 1 0 0 82.8563 82.8563 255.689 7 PROCESSED 57545.3939351852 2016-06-06 09:27:16 55328 2010-05-12 00:00:00 54880.5781365741 2009-02-18 13:52:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031346 We propose a 200 ks observation of 3C279, the archetypal EGRET blazar to be conducted simultaneously with GLAST as well as many other facilities, with the goal of obtaining broadband spectra and light-curves. The flux in all observable bands is known to be rapidly variable, but the information regarding the correlation between the time history of flux in various bands is limited, and the proposed observations are designed to remedy this shortcoming. Such detailed spectral and variability studies are crucial to discriminate between different radiation scenarios responsible for production of X-rays and gamma-rays, and to constrain the matter content and by extension, the formation process of the jet, dissipation of the jet energy, and energization of the radiating particles. EXTRAGALACTIC COMPACT SOURCES 7 A GRZEGORZ MADEJSKI USA 3 AO3 SUZAKU AND GLAST OBSERVATIONS OF 3C279 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703049010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703049010'

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