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 1ES 1553+113 238.8999 11.1305 238.306227 11.275519 233.852477 30.750337 21.81691499 43.96274027 296.7536 53940.6127777778 2006-07-24 14:42:24 53941.8036342593 2006-07-25 19:17:14 701070010 55.6355 55 55.6435 55.6515 55.6515 55.6355 2 2 2 2 1 0 0 53.2015 53.2015 102.8819 0 PROCESSED 57535.0418171296 2016-05-27 01:00:13 54401 2007-10-28 00:00:00 53955.6133680556 2006-08-08 14:43:15 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011376 Detecting absorption effects in TeV blazar spectra from TeV photon collisions on the extragalactic IR background (EBL) is a powerful tool to probe the EBL. It requires a thorough understanding of the intrinsic blazar spectra. We propose XIS and HXD observations, with emphasis on the hard X-rays, for the 3 most distant HESS blazars, coordinated with HESS observations. Thanks to Suzaku's sensitivity in a broad energy range, we expect to set tight limits on the models' parameter space, and constrain emission and acceleration scenarios by studying the shape and evolution of the particle distribution, most sensitively conducted in the important hard X-ray energy range. In coordination with TeV observations, it allows us to disentangle EBL absorption effects from the blazar intrinsic spectra. EXTRAGALACTIC COMPACT SOURCES 7 A ANITA REIMER USA 1 AO1 CHALLENGING JET MODELS OF THE MOST DISTANT TEV-BLAZARS HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701070010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701070010'

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