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 NGC3923 177.7599 -28.8047 177.126048 -28.526534 190.367331 -27.106442 287.27787622 32.22445477 293.1988 53899.8430671296 2006-06-13 20:14:01 53902.7293287037 2006-06-16 17:30:14 801054010 115.82 120 115.828 115.82 115.828 115.828 2 2 2 2 1 0 0 107.7313 107.7313 249.3528 3 PROCESSED 57534.7187731482 2016-05-26 17:15:02 54394 2007-10-21 00:00:00 53927.2880902778 2006-07-11 06:54:51 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010100 We propose to observe an isolated elliptical galaxy NGC3923, to meaasure a dark matter distribution. The large effective area and stable low background of XIS enable us to measure a faint extended X-ray emission such as the periphery of elliptical galaxies more accurately than ever. Since X-ray bright elliptical galaxies have been found to be surrounded by group-scale emission, X-ray faint elliptical galaxies are the best to investigate the dark matter associated with the galaxy itself. The dark matter around galaxies is a key to resolve the problem of why X-ray bright and faint elliptical galaxies exist. The oxygen abundance distribution is also useful to probe the above issue. EXTRAGALACTIC DIFFUSE SOURCES 8 B YASUSHI FUKAZAWA JAP 1 AO1 ACCURATE MEASUREMENT OF DARK MATTER DISTRIBUTION AROUND AN ISOLATED ELLIPTICAL GALAXY NGC3923 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801054010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801054010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏