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 | A1914_OFFSET4 | 216.4424 | 37.6372 | 215.928949 | 37.861845 | 196.491265 | 48.360248 | 66.78881215 | 67.57279807 | 134.0011 | 55566.4311574074 | 2011-01-05 10:20:52 | 55566.8258912037 | 2011-01-05 19:49:17 | 805094020 | 17.3531 | 12 | 17.3531 | 17.3611 | 0 | 17.3691 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 16.0606 | 16.0606 | 34.1 | 0 | PROCESSED | 57600.564375 | 2016-07-31 13:32:42 | 55995 | 2012-03-09 00:00:00 | 55627.1583333333 | 2011-03-07 03:48:00 | 3.0.22.44 | 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/ver3.0/805094020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805094020'
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