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 RBS 315 36.2519 18.8398 35.555924 18.614311 40.065414 4.223463 151.73247281 -38.74296898 76.7825 53941.8167013889 2006-07-25 19:36:03 53943.0404976852 2006-07-27 00:58:19 701077010 47.8309 50 47.8309 47.8309 47.8309 47.8309 2 2 2 2 1 0 0 43.425 43.425 105.7299 1 PROCESSED 57535.0495023148 2016-05-27 01:11:17 54400 2007-10-27 00:00:00 53955.7322106482 2006-08-08 17:34:23 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012008 We propose to observe with Suzaku the X-ray bright blazar RBS 315, showing a very hard spectrum (Gamma<1.2) in the 2-10 keV range as determined by XMM. The requested observation will allow us to measure the continuum in the full Suzaku range (0.3-200 keV), fully exploiting the unique capabilities of the satellite. With its wide energy coverage and good response at soft energies, Suzaku will allow to determine with precision the spectral properties of the source in the hard medium and soft X-ray ranges, providing important clues on the physics and the environment of relativistic jets. A good measurement of the continuum will allow us to determine the luminosity emitted via the IC mechanism which usually dominates the radiative output and the total kinetic power carried by the outflow. EXTRAGALACTIC COMPACT SOURCES 7 B FABRIZIO TAVECCHIO EUR 1 AO1 SUZAKU OBSERVATION OF THE HARD BROAD BAND CONTINUUM OF THE POWERFUL BLAZAR RBS 315 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701077010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701077010'

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