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 NGC1961BACKGROUND 85.5048 67.8763 84.182746 67.851301 87.633372 44.47331 145.2497599 18.81010884 72.0206 54748.602962963 2008-10-09 14:28:16 54749.1197222222 2008-10-10 02:52:24 803041010 24.1435 20 24.1435 24.1435 0 24.1435 2 2 0 2 1 0 0 20.099 20.099 44.6399 1 PROCESSED 57544.0915393518 2016-06-05 02:11:49 55148 2009-11-13 00:00:00 54780.6911342593 2008-11-10 16:35:14 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031401 Galaxies are missing most of their baryons when compared to the cosmological baryon to dark matter ratio. The Milky Way is missing at least 70% of its baryons while lower mass galaxies retain less than 10% of their baryons. Theory suggests that these baryons were expelled by intense galactic winds during the primary star formation period. These galactic winds carry gas far beyond the virial radius of small and modest galaxies, but the most massive galaxies should retain much of this gas. We propose to test this picture by searching for the missing baryons surrounding the very massive spiral galaxy, NGC 1961, which has 10 times the stellar content of M31 and with v_rot = 450 km/sec. If successful, we will detect a significant fraction of the 5E11 Msun of its missing baryons. EXTRAGALACTIC DIFFUSE SOURCES 8 B JOEL BREGMAN USA 3 AO3 THE BARYONS CONTENT OF THE MOST MASSIVE SPIRAL GALAXY XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '803041010'

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

Go to top of this page ⏏