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 | AO 0235+164 | 39.665 | 16.613 | 38.972105 | 16.397631 | 42.455706 | 1.088366 | 156.77598662 | -39.11106084 | 252.4352 | 56310.722337963 | 2013-01-18 17:20:10 | 56311.7418634259 | 2013-01-19 17:48:17 | 707021010 | 43.1028 | 40 | 43.1108 | 43.1188 | 0 | 43.1028 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 38.3583 | 38.3583 | 88.0698 | 0 | PROCESSED | 57608.5604166667 | 2016-08-08 13:27:00 | 56709 | 2014-02-21 00:00:00 | 56342.5387731482 | 2013-02-19 12:55:50 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071402 | We request observations of the variable blazar AO 0235+164, to be conducted simultaneously with Fermi and optical and radio telescopes, towards a multi-band campaign. This object has complex X-ray spectrum due to absorption by an intervening galaxy, and Suzaku will be essential in unraveling the effects and composition of that absorber, and for the first time, provide a robust measurement of the underlying blazar X-ray continuum, which, together with the Swift UVOT spectrum, will allow to verify the signature of the bulk-Compton component, due to cold electrons propagating in the relativistic jet. At the highest priority, we request 40 ks for a precise spectral measurement; at a lower priority, we wish to monitor the source for the total of 5 days, with the request of additional 160 ks. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | GRZEGORZ MADEJSKI | USA | 7 | AO7 | SUZAKU OBSERVATIONS OF THE GAMMA-RAY BLAZAR AO 0235+164 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707021010'
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