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".

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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 A1914_OFFSET2 216.7383 37.763 216.226328 37.986791 196.709268 48.583272 66.87630822 67.3091462 329.9943 55363.4747569444 2010-06-16 11:23:39 55364.3800115741 2010-06-17 09:07:13 805092010 28.5462 40 28.5542 28.5542 0 28.5462 2 2 0 2 1 0 0 25.8343 25.8343 78.204 0 PROCESSED 57552.3515856482 2016-06-13 08:26:17 55766 2011-07-24 00:00:00 55399.3275231482 2010-07-22 07:51:38 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805092010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805092010'

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