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 | ULXs in NGC 1313 | 49.5245 | -66.5352 | 49.373425 | -66.716272 | 341.380796 | -74.178462 | 283.41323765 | -44.63106544 | 172.6337 | 53658.556400463 | 2005-10-15 13:21:13 | 53659.6252777778 | 2005-10-16 15:00:24 | 100032010 | 32.878 | 40 | 32.878 | 32.878 | 32.878 | 32.878 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 30.38 | 30.38 | 92.3439 | 1 | PROCESSED | 57527.587349537 | 2016-05-19 14:05:47 | 54247 | 2007-05-27 00:00:00 | 54036.1929398148 | 2006-10-28 04:37:50 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000032 | We propose Suzaku observation of a nearby (4.5 Mpc) galaxy NGC 1313 hosting two prototypical ULXs. These ASCA specta of many ULXs were described with a "high temperature diskbb" model, spectra obtained with XMM (and Chandra) prefer a "power-law plus low-temperature disk" modeling. The superior 5-10 keV sensitivity of Suzaku allows us to examine whether the spectra of luminous ULXs indeed exhibit a turn-over around 5 keV or extend up to 10 keV. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | ULXs in NGC 1313 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100032010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100032010'
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