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. |
observation_id
|
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
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 201052010 | RADIO_ARC | 266.59627 | -28.89568 | 265.80224 | -28.87722 | 267.00669 | -5.49175 | 0.1217 | -0.12191 | 80.0005 | 60750.66741 | 2025-03-16 16:01:04 | 60753.74032 | 2025-03-19 17:46:04 | 119.813 | 100.000 | 119.813 | 116.670 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 116.670 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-03-29 05:44:19 | 2026-04-05 00:00:00 | 2025-03-30 05:44:20 | 03.00.013.010 | gen20241115_xtd20241115_rsl20241115 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000013003 | The most characteristic spectral features of the Galactic center are bright fluorescence X-rays at 6.4 keV emitted from neutral Fe atoms in molecular clouds. Photoionization by X-rays from Sagittarius A* has been considered as its origin (the XRNe scenario). On the other hand, the Galactic center should have a high density of low-energy cosmic rays (CRs), and thus there is still a strong possibility that the neutral Fe line is due to CR bombardment. In this observation, we will explore new spectral features that could never be observed by X-ray CCD energy resolutions, and measure neutral emission lines from other elements so that we will quantitatively clarify the ratio of the XRNe and CR origins. | GALACTIC DIFFUSE EMISSION AND SURVEYS | 2 | A | KUMIKO NOBUKAWA | SHUO ZHANG | JUS | 1 | NOR | THE ORIGIN OF THE NEUTRAL FE LINE IN THE GALACTIC CENTER EXPLORED BY NEW SPECTRAL FEATURES | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201052010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201052010'
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