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 BL LACERTAE 330.6466 42.3471 330.130697 42.105096 354.282545 49.658149 92.61224541 -10.37092111 71.9797 53882.2303703704 2006-05-27 05:31:44 53883.305775463 2006-05-28 07:20:19 701073010 48.5294 50 48.5454 48.5454 48.5294 48.5374 2 2 2 2 1 0 0 35.5443 35.5443 92.902 1 PROCESSED 57534.4514236111 2016-05-26 10:50:03 54401 2007-10-28 00:00:00 53926.2373032407 2006-07-10 05:41:43 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011377 We propose two 50 ks Suzaku observations, one for each of gamma-ray bright blazars PKS 1510-089 and BL Lacertae, to be coordinated with optical and radio observations. The goal is to obtain broadband spectra and light-curves. The X-ray fluxes are known to be rapidly variable, but there is no information about the correlation between the spectral shape and flux, which is necessary to establish the origin of previously detected prominent soft X-ray excesses. They are crucial to discriminate between different radiation scenarios responsible for production of hard X-rays and gamma-rays, and to constrain the content and by extension, the acceleration process of the jet. These observations will be ingredients of a "pilot" campaigns for the future joint Suzaku-GLAST investigations. EXTRAGALACTIC COMPACT SOURCES 7 A GRZEGORZ MADEJSKI USA 1 AO1 SUZAKU OBSERVATIONS OF GAMMA-RAY BRIGHT BLAZARS BL LACERTAE AND PKS 1510-089 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701073010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701073010'

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