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 1RXS J111706.3+20141 169.2749 20.2432 168.614437 20.516401 162.09404 14.35752 225.56577108 67.37465885 120.2309 55510.3081944444 2010-11-10 07:23:48 55511.1543402778 2010-11-11 03:42:15 705036010 34.2125 32 34.2125 34.2125 0 34.2125 2 2 0 2 1 0 0 31.5366 31.5366 73.0979 0 PROCESSED 57554.0402199074 2016-06-15 00:57:55 55903 2011-12-08 00:00:00 55537.0979050926 2010-12-07 02:20:59 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051402 High frequency peaked BL Lacs are a peculiar subclass of Blazars characterized by non-thermal emission across the whole electromagnetic spectrum. Their spectral energy distributions (SEDs) include two main components: a low-energy component with power peaking in the range from the UV to the X-ray band, and a substantial high-energy component often dominated by gamma-rays. We propose 3 observations (32 ks each) of a selected sample of HBLs to study the behavior of the first component, widely interpreted as synchrotron radiation. First, we will be able to disentangle between different spectral shapes of the synchrotron SED of HBLs. Second, we will use the proposed observations to investigate the properties of the most representative sample of TeV candidate HBLs. EXTRAGALACTIC COMPACT SOURCES 7 C FRANCESCO MASSARO USA 5 AO5 X-RAY CURVED SPECTRA IN HIGH FREQUENCY PEAKED BL LACS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705036010'

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