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 GB1428+4217 217.5879 42.0673 217.100189 42.288572 194.201902 52.635769 75.8575282 64.90635728 315.7011 53898.716400463 2006-06-12 17:11:37 53899.8336111111 2006-06-13 20:00:24 701092010 48.6956 50 48.6956 48.6956 48.6956 48.6956 2 2 2 2 1 0 0 43.4943 43.4943 96.5159 1 PROCESSED 57534.6334259259 2016-05-26 15:12:08 54394 2007-10-21 00:00:00 53926.3635069444 2006-07-10 08:43:27 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012043 We propose to observe GB1428+4217 at z=4.72 for 50ks with Suzaku in order to determine its spectrum up to 45 keV, corresponding to a rest-frame energy of ~250 keV. This will allow to robustly model the spectrum in terms of a hard power-law and a Comptonization component from the scattering of `cold' electrons in the jet onto the soft nuclear photon field, as qualitatively hinted by XMM-Newton available data. This would be the first detection of such a feature in blazars and would directly and uniquely give information on the power of the relativistic jets in this source. EXTRAGALACTIC COMPACT SOURCES 7 A ANDREW FABIAN EUR 1 AO1 JET POWER OF THE DISTANT EXTREME LUMINOSITY BLAZAR GB1428+4217 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701092010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701092010'

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