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 | 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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