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 | 1RXS J032613.6+02252 | 51.5615 | 2.4213 | 50.912043 | 2.246984 | 49.792333 | -15.817317 | 180.7494445 | -42.4285339 | 253.9336 | 55596.8403356482 | 2011-02-04 20:10:05 | 55597.6203125 | 2011-02-05 14:53:15 | 705038010 | 32.1971 | 32 | 32.1971 | 32.1971 | 0 | 32.1971 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 22.6441 | 22.6441 | 67.3879 | 1 | PROCESSED | 57600.8622106482 | 2016-07-31 20:41:35 | 55983 | 2012-02-26 00:00:00 | 55614.1886342593 | 2011-02-22 04:31:38 | 3.0.22.44 | 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/ver3.0/705038010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705038010'
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