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 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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