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 | NGC 7618 | 349.8326 | 42.9144 | 349.23867 | 42.640678 | 11.92237 | 42.546584 | 105.51742003 | -16.82119292 | 269.9991 | 55911.4056828704 | 2011-12-16 09:44:11 | 55913.6161458333 | 2011-12-18 14:47:15 | 506027010 | 101.1772 | 100 | 101.1852 | 101.1772 | 0 | 101.1852 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 95.774 | 95.774 | 190.9399 | 0 | PROCESSED | 57604.196712963 | 2016-08-04 04:43:16 | 56289 | 2012-12-28 00:00:00 | 55922.1112847222 | 2011-12-27 02:40:15 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060073 | We propose to observe nearby merging galaxy group NGC 7618. The asymmetric X-ray shape with a tail and a sharp brightness discontinuity were discoverd by observations of ASCA and Chandra. This is due to a merging with an another galaxy group, UGC 12491, which has similar mass of NGC 7618. The pair is in the primary stage of merging, then we need to obtain the information of the gas outside region to clarify the process of the merging. By taking advantage of low background and high energy resolution of XIS, we estimate accurately distribuion of temperature and metal abundances around both galaxy groups. Then we aim to clarify the process of the merging system of the galaxy groups. | GALACTIC DIFFUSE EMISSION | 5 | C | KATSUHIRO HAYASHI | JAP | 6 | AO6 | OBSERVATION OF NEARBY MERGING GALAXY GROUP NGC 7618 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506027010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506027010'
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